There are few places on earth where the desert feels as cinematic as it does in Dubai. The dunes roll like waves, the light turns gold twice a day with almost theatrical precision, and the skyline, when you glimpse it from the outskirts, serves as a reminder that you're dancing on the frontier between wilderness and a city built on ambition. It's exactly this blend of spectacle and accessibility that has made quad biking in Dubai so popular-an experience that feels daring yet attainable, raw yet well-organized, and always photogenic.
If you've never ridden an ATV over sand, imagine trading the straight lines of a road for the soft contours of a living landscape. The bike hums beneath you; the dunes rise and fall like the ocean, and you learn to read them-how to feather the throttle on a climb, how to lean and let the rear tire squirm safely under you, how to crest a ridge without diving off the wrong side. Quad Biking And Dune Bashing Dubai Sand isn't intimidating once you respect it. It rewards smoothness and patience. On a good day, you'll find a rhythm: point, glide, rise, and sweep, the bike carving rooster tails that hang in the air behind you like punctuation marks.
Part of the appeal of quad biking in Dubai is the way it has been made beginner-friendly. Most tours are guided, the ATVs are automatic, and the briefing is straightforward: how to start and stop, where to look, how to space out in a convoy, what to do if you bog down. There's usually a practice loop on firmer ground before the group noses into the softer dunes. Helmets and goggles are standard, and the better operators are firm about safety: no risky overtakes, keep a sensible gap, follow the leader's tracks, and listen out for hand signals or radio calls. It feels structured without losing the thrill.
The setting amplifies everything. Popular riding areas include the Lahbab “Red Dunes,” where the sand blushes under late afternoon sun; Al Qudra, with its wide-open bowls; and the Al Marmoom Desert Conservation Reserve, where tours tread more lightly to respect wildlife and vegetation.
Resident Quad Biking Dubai
Resident Quad Biking Dubai
Open Desert Quad Biking Dubai
Abu Dhabi Quad Biking Tours
Corporate Quad Biking Dubai
Yamaha Grizzly Quad Biking Dubai
Quad Biking Dubai Rate Card
Some itineraries make a point of chasing the golden hour, timing departures to catch the sunrise when the sand is cool and unmarked, or sunset when the sky shifts through apricot and violet and the city lights begin to flicker in the distance. If you ride at those times, you learn quickly why so many photos from Dubai's dunes look like they stepped out of a travel magazine-this is a landscape built for backlighting and silhouettes.
Beyond the ride itself, quad biking tends to be part of a larger desert ritual. Many packages pair an hour on the ATVs with sandboarding, short camel rides, or a visit to a Bedouin-style camp. You might end the day with a barbecue dinner under strings of lights, the air scented with cardamom and smoke, and, depending on the season, traditional dance performances. In Ramadan, programming and entertainment may be more subdued; in the hotter months, operators often shift to early mornings and late evenings to avoid the midday heat. The sweet spot for weather is typically October through April, when the desert is cooler and the breeze takes the edge off the sun.
Practicalities are simple. Most tours include hotel pickup in 4x4 vehicles and a 45–60 minute drive out of the city, depending on the dune area. For drivers, minimum age rules vary by company, but many require you to be 16 or older (sometimes 14 with a guardian's consent).
Open Desert Quad Biking Dubai
Quad Biking Dubai Stag Party
Quad Biking Dubai Special Offer
Quad Biking And Dune Bashing Dubai
You don't need a driver's license for guided ATV sessions. Closed-toe shoes are a must; so are sunglasses, sunscreen, and breathable clothing you don't mind dusting off. A scarf can help with the occasional gust, and a small backpack keeps your water and essentials handy. If you plan to shoot photos, bring a lens cloth-fine sand sneaks into everything-and consider a simple action camera mount to keep your hands free.
Costs vary with duration, group size, and extras. Short rides-20 to 30 minutes on a shared track-are the budget-friendly entry point. Insured Quad Biking Dubai . Longer guided dune sessions, private tours, or packages that add dinner and transport are pricier.
Open Desert Quad Biking Dubai
Scenic Quad Biking Dubai
Reliable Quad Biking Dubai
Professional Quad Bike Guides Dubai
Insurance and safety gear are typically included, though you'll usually be asked to sign a waiver, and some premium operators offer more comprehensive coverage or newer machines. If the price seems too good to be true, ask a few questions: How big is the group? Is it open terrain or a fenced course? What's the guide-to-rider ratio? Are there clear briefings and recovery support if someone gets stuck? These details shape your experience more than you might think.
Skill levels are well served across the board. Beginners can stick to gentler slopes and gather confidence; confident riders can opt for tours that push deeper into the dunes, with longer climbs, sharper ridgelines, and the kind of sweeping descents that make you grin inside your helmet. If you're traveling with family, check whether there are two-seater buggies or side-by-sides available; they're a good compromise when not everyone wants to ride solo. And if you're an experienced off-roader thinking about going it alone, take a moment to study local rules and safety considerations-desert navigation is deceptively difficult, and a guided ride is not only safer but often more fun. Guides know the dunes like locals know side streets; they can stitch together a loop that flows.
There's also an ethic to riding here that matters. The desert might look empty, but it's alive. Larks nest in low shrubs, beetles trace dotted lines across slopes, and on lucky days you might glimpse a desert fox or, within reserves, an oryx herd. Open Desert Quad Biking Dubai Respecting designated areas, avoiding sensitive plants, and packing out your litter helps keep the dunes pristine. If you bring a drone, make sure you understand the UAE's strict regulations and any no-fly zones; permits are required in many areas, and fines are real.
What surprises many people is how calming the desert can be once the adrenaline settles. The engine's chatter fades when you stop, and the silence rolls in-broad, uncomplicated, the kind of quiet that cities seize from you without you noticing. It's here, standing on a ridge with a wide horizon and sand still cascading in tiny avalanches down the leeward side, that quad biking in Dubai becomes more than a quick thrill. It's an encounter with a landscape that shapes the region's identity, paired with a hospitality culture that makes it accessible.
Popular quad biking in Dubai didn't become popular by accident. It's the result of thoughtful curation: the right machines, capable guides, logistics that remove friction, and a canvas that's hard to improve upon. Whether you're a first-timer drawn by the photographs or a returning rider chasing a cleaner line across a steeper face, the dunes offer the same promise: a few hours where your world narrows to trajectory and texture and light-and opens, paradoxically, into something larger, older, and beautifully simple.
About Tourism in Dubai
The Al Fahidi Historical Neighbourhood, also called Al Bastakiya, is Dubai's historic district and major tourist destination.
Tourism in Dubai is a major part of the economy of Dubai. Dubai was the third most visited city in the world in 2023 with 17 million international visitors according to Euromonitor International.[1][2] Dubai hosts more than 800 hotels with more than 150,000 rooms.[3][4]
History
[edit]
The discovery of oil in 1966 kick-started the development of present Dubai, however Sheikh Hamad bin Maktoum (ruler from 1958 till 1990) realised one day Dubai would run out of oil and started building an economy that would outlast it.[5] A quote commonly attributed to Sheikh Rashid reflected his concern that Dubai's oil, which was discovered in 1966 and which began production in 1969, would run out within a few generations. Sheikh Rashid stated "My grandfather rode a camel, my father rode a camel, I drive a Mercedes, my son drives a Land Rover, his son will drive a Land Rover, but his son will ride a camel".[6] Sheikh Rashid realized early he needed to diversify the emirate of Dubai's economy by building on the city's trading history and therefore he set out to establish Dubai as the region's trade and service hub. By 1979, he was successful in establishing the Jebel Ali Port, which became the logical shipping centre for the entire United Arab Emirates and the world's largest man-made port. He also upgraded Dubai International Airport and built the Dubai World Trade Centre, which was then the tallest building in the Middle East. By the end of the 1970s, the stage was set for the diversification of Dubai's economy away from oil and into other areas such as tourism.[7]
In 1989 the Dubai Commerce and Tourism Promotion Board was established, to promote Dubai as a luxury destination for the up-tier market and influential business sectors. In January 1997, it was replaced with the Department of Tourism and Commerce Marketing (DTCM).[8]
In May 2013, the government of Dubai launched the Dubai Tourism Strategy 2020, with the key objective to attract 20 million visitors a year by 2020 and making Dubai a first choice destination for international leisure travellers as well as business travellers.[9] In 2018, the strategy was expanded by setting new goals of attracting 21-23 million visitors in 2022 and 23-25 million visitors by 2025.[10] The key objectives from 2013 and 2018 were not met due to the COVID-19 pandemic.
The need to maintain its tourism industry has hampered Dubai's response to the COVID-19 pandemic.[11] Along with COVID-19 Dubai's tourism sector has also been hurt by a greater international awareness of the status of human rights in the emirate and in particular the treatment of Princess Latifa bint Mohammed Al Maktoum.[12]
In November 2022, Sheikh Mohammed bin Rashid announced a national tourism strategy until 2031. The goal of the strategy is to attract Dh 100 billion in additional tourism investments (so that the tourism sector's contribution will be Dh450bn of Dubai's GDP in 2031) and receive 40 million hotel guests in 2031. The strategy includes 25 initiatives and policies to support the development of the tourism sector in the country.[13]
In April 2025, the Dubai Department of Economy and Tourism introduced a new programme offering media training to students for promotion of tourism in the UAE. Applicants are provided with flights, luxury apartment and three months of income, along with certification from Dubai College of Tourism for posting about traveling experiences in Dubai on social media. According to Middle East Eye, this program aims to whitewash its human rights violations and war crime accusations in Sudan.[14]
Visitors and visitor spending
[edit]
Since 1982, Dubai continued to be one of the fastest growing destinations for tourists. In 2002, visitors were mainly from other Gulf Cooperation Council members which accounted for 34% of tourists, South Asia accounted for 25%, other Arab states 16%, Europe 15%, and Africa 9%. In 2003, revenue from tourism exceeded $1 billion and surpassed oil revenues to directly and indirectly account for over 17% and 28% of GDP respectively.[15]
From January to June 2019 8.36 million international tourists visited Dubai. Most of the visitors were from India (997,000) followed by Saudi Arabia (755,000) and the United Kingdom (586,000).[16]
Mastercard's Global Destination Cities Index 2019 found that tourists spend more in Dubai than in any other country. In 2018, the country topped the list for the fourth year in a row with a total spend of $30.82 billion, a 3.8% increase over 2017 ($29.70 billion). The average spend per day was $553.[17]
In 2019, Dubai attracted a total of 16.73 million tourists, which was an increase of 5.09% on the previous year. However, in 2020, the number of visitors dropped to 5.51 million due to the coronavirus pandemic.[18]
Year
Total
international
visitors [19][20][21][15][22][23]
Increase/decrease
Visitor spending
($m)[24]
1982
374,400
—N/a
1990
632,903
69.04%
1991
716,642
13.23%
1992
944,350
31.77%
1993
1,088,000
15.21%
1994
1,239,000
13.88%
1995
1,601,000
29.22%
632.0
1996
1,768,000
10.43%
743.0
1997
1,792,000
1.36%
814.0
1998
2,184,000
21.88%
859.0
1999
2,481,000
13.60%
893.0
2000
3,027,000
22.01%
1,063.0
2001
3,626,625
19.81%
1,200.0
2002
4,756,280
31.15%
1,332.0
2003
4,980,228
4.71%
1,438.0
2004
5,420,000
8.83%
1,593.0
2005
6,160,003
13.65%
3,218.0
2006
6,441,670
4.57%
4,972.0
2007
6,951,798[25][26]
7.12%
6,072.0
2008
6,996,449[25]
0.64%
7,162.0
2009
7,580,000[27]
8.34%
7,352.0
2010
8,410,000
10.95%
8,577.0
2011
9,910,000
17.84%
9,204.0
2012
10,950,000
10.49%
10,924.0
2013
12,900,000
17.81%
12,389.0
2014
13,200,000
2.33%
15,221.0
2015
14,200,000
7.58%
25,587.1
2016
14,870,000
4.72%
28,657.4
2017
15,790,000
6.19%
29,705.5
2018
15,920,000
0.82%
34,609.5
2019
16,730,000
5.09%
38,413.3
2020
5,510,000[a]
-67.07%
24,615.4
2021
7,280,000[b]
32.12%
2022
14,360,000[28]
97.25%
2023
17,150,000[29]
19.4%
2024
18,720,000[30]
9.2%
Accommodation
[edit]
Main article: List of hotels in Dubai
Burj Al Arab hotel
In the last three years, Dubai saw an increase in 4 and 5 star hotels and number of rooms, but a decrease in standard hotel apartments. The total number of rooms increased by 9,098 from 2015 to 2017, an increase of 9.25%. Prior to the Expo 2020 hotels in Dubai were reducing room rates to stimulate demand as supply accelerated. Based on data of August 2019, Dubai hoteliers reported a 7.6% rise in supply against 7.4% increase in demand.[31] Average room rates stood at AED 486 in June 2019 while in the same month of 2018 average room rates were at 544 AED.[32] In July 2019, Dubai's Jumeirah Group LLC fired 500 people due to a decline in tourism. In the second quarter of 2019, hospitality sector has had the worst quarter since 2009.[33]
Hotel inventory numbers 2014-2023[19]
2014
2015
2016
2017
2018
2019
2020
2021
2022
2023
Total 5 star hotels
91
96
103
113
128
134
143
151
157
Total 5 star hotel rooms
31,551
33,122
35,853
38,543
43,133
44,067
47,035
49,585
51,809
Total 4 star hotels
106
112
122
146
158
161
181
189
194
Total 4 star hotel rooms
21,208
22,990
25,289
29,908
33,120
34,905
40,377
42,505
43,283
Total 1-3 star hotels
264
267
260
260
258
225
243
270
274
Total 1-3 star hotel rooms
19,714
21,767
21,591
22,634
24,491
21,732
25,384
28,512
28,789
Total hotel apartments (deluxe/superior)
66
66
65
68
68
74
80
82
85
Total deluxe/superior rooms
9,641
9,519
9,786
10,522
10,520
11,845
12,606
13,113
13,842
Total hotel apartments (standard)
150
140
131
129
129
117
108
112
111
Total standard rooms
16,219
15,447
14,930
14,360
14,856
14,398
12,548
12,781
12,568
Total establishments
657
677
681
681
716
741
711
755
804
821
Total available rooms
92,333
98,333
102,845
107,431
115,967
126,120
126,947
137,950
146,496
150,291
Average occupancy
79%
77%
78%
78%
76%
75%
54%
67%
73%
77%
Visitor Statistics
[edit]
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Rank
Country
6/2023
2022
1
India
1,223,000
1,842,000
5
Russia
616,000
758,000
4
United Kingdom
555,000
1,043,000
3
Saudi Arabia
538,000
1,216,000
2
Oman
511,000
1,311,000
6
United States
362,000
590,000
7
Germany
329,000
422,000
17
China
260,000
177,000
10
Iran
196,000
328,000
13
Israel
196,000
239,000
8
France
180,000
364,000
11
Egypt
168,000
288,000
12
Kuwait
152,000
260,000
9
Pakistan
152,000
356,000
14
Kazakhstan
145,000
234,000
15
Italy
130,000
212,000
19
Philippines
125,000
158,000
16
Australia
121,000
184,000
18
Canada
110,000
158,000
19
Japan
110,000
148,000
Attractions
[edit]
Main article: Tourist attractions in Dubai
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Al Fahidi Fort
Aspects of Dubai's old culture, while occasionally overshadowed by the boom in economic development, can be found by visiting places around the creek, which splits Dubai into two halves, Bur Dubai and Deira. The buildings lining the Bur Dubai side of the Creek provide the main flavor of the old city. Heritage Village is one of the few remaining parts of historical Dubai, containing preserved buildings. The adjoining Diving Village offers exhibits on pearl diving and fishing. The Diving Village forms part of an ambitious plan to turn the entire "Shindagha" area into a cultural city, recreating life in Dubai as it was in days gone by.
Boats on Dubai water line night view
Other attractions include the Sheikh Saeed Al Maktoum House; the Dubai Museum in the restored Al Fahidi Fort, which was erected around 1799; and the Heritage Village of Hatta, situated 115 kilometers southeast of Dubai City in the heart of the rocky Hatta Mountains. The history of the village can be traced back 2000 – 3000 years. It consists of 30 buildings, each differing in size, interior layout and building materials used. Great care was taken to use the same materials as those used when originally built during the renovation such as mud, hay, sandalwood and palm fronds. The Sharia Mosque is an old mosque built in the early 19th century using the same building materials and consists of a large prayer hall, a court and courtyard, minaret and other utility rooms.[34] Other museums include the Al Ahmadiya School.
Shopping
[edit]
Main article: List of shopping malls in Dubai
Dubai Fountain at the Dubai Mall
Dubai has been nicknamed the "shopping capital of the Middle East."[35][36] The city draws large numbers of shopping tourists from countries within the region and from as far as Eastern Europe, Africa and the Indian Subcontinent. Dubai is known for its souk districts. Souk is the Arabic word for market or place where any kind of goods are brought or exchanged. Traditionally, dhows from the Far East, China, Sri Lanka, and India would discharge their cargo and the goods would be bargained over in the souks adjacent to the docks.[37]
Modern shopping malls and boutiques are also found in the city. Dubai Duty Free at Dubai International Airport offers merchandise catering to the multinational passengers using Dubai International Airport. Outside of Duty Free areas and major sales, Dubai has a reputation for being one of the most expensive shopping destinations in the world.[38]
While boutiques, some electronics shops, department stores and supermarkets may operate on a fixed-price basis, most other outlets consider friendly negotiation as a way of life.
Dubai's numerous shopping centres cater for every consumer's need. Cars, clothing, jewellery, electronics, furnishing, sporting equipment and any other goods will all be likely to be under the same roof.[39]
The Dubai Shopping Festival is a month-long festival held during the month of January each year. During the festival the entire emirate becomes one massive shopping mall. Additionally, the festival brings together music shows, art exhibitions, and folk dances.[40]
The Dubai Summer Surprises (DSS) is the summer version of Dubai Shopping Festival held during June, July and August. Dubai Government launched Dubai Summer Surprises in 1998 in order to promote Dubai as a family holiday destination. DSS offers fun, entertainment, food deals and great offers on shopping.
Cultural sensitivity
[edit]
See also: Culture of Dubai
Tourists are required to obey some Muslim religious restrictions in public even if they are not Muslim themselves, such as refraining from eating or drinking in public places in the daytime during Ramadan.[41]
Dubai has a modest dress code as part of its criminal law.[42] Sleeveless tops and short dresses are not encouraged at Dubai Mall.[43][44] Clothes are advised to be in appropriate lengths.[42]
Homosexuality is criminalized in Dubai, including for tourists. However, there is a vibrant underground gay scene in Dubai and authorities do not actively search for homosexuals to enforce the law.[45]
Transportation
[edit]
Main article: Transportation in Dubai
Dubai International Airport is the world's busiest airport by international passenger traffic.
Most capitals and other major cities have direct flights to Dubai. More than 120 airlines operate to and from Dubai International Airport to more than 260 destinations. Dubai International Airport is the world's busiest airport by international passenger traffic.[46] Dubai is also the home base of the airline Emirates, which operates scheduled services to more than 100 destinations.
In June 2009 Emirates designated a special handling area at departures and arrivals for passengers with special needs, allowing wheelchair passengers to receive a more personalized service.[47][better source needed]
The establishment of the first cruise terminal in Dubai in 2001 and the opening of the enhanced New Dubai Cruise Terminal in February 2010 with higher handling capacity has drawn the attention of cruise line operators. Cruises to Dubai sail from: Singapore, Sydney, Athens, Dover, Venice, Cape Town, Civitavecchia, Piraeus, Alexandria, Istanbul, New York City, Southampton, Barcelona, Fort Lauderdale, Miami, Los Angeles, Mumbai, Hong Kong, Shanghai, Monte Carlo, Mombasa, Victoria, and Cairns among others.[48][better source needed]
The United Arab Emirates has a network of roads that connect major towns and villages, including a multi-lane highway between Dubai and Abu Dhabi, with access to and from the bordering countries of Saudi Arabia and Oman. Highways and main roads in Dubai and the United Arab Emirates are designated by an Emirate Route Number. Speed limits are displayed on road signs and are usually 60–80 km/h (37–50 mph) around town and 100–120 km/h (62–75 mph) elsewhere.[49][better source needed]
Dubai ranked third in the best taxi services behind Tokyo and Singapore.[50][better source needed]
Illicit drugs
[edit]
Travelers entering Dubai are warned for harsh penalties regarding illicit drug use or smuggling. Authorities in Dubai use highly sensitive equipment to conduct thorough searches to find trace amount of illegal substances.[51] A senior Dubai judge was quoted on February 11, 2008, by the Dubai City News saying, "These laws help discourage anyone from carrying or using drugs. Even if the quantity of illegal drugs found on someone is 0.05 grams, they will be found guilty. The penalty is a minimum of four years. The message is clear — drugs will not be tolerated."[51]
Health
[edit]
Further information: Healthcare in the United Arab Emirates
No special immunizations are required, but tourists are encouraged to purchase appropriate medical insurance before travelling. Government immunization programs have led to recognition by a travel magazine.[47] As a latest addition to the established modern health care system, Dubai offers online health care contacts of virtually all medical doctors in Dubai.[52]
Sports tourism
[edit]
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Dubai hosts the following international championships:
Dubai World Cup – the richest horse race in the world
Dubai Classic - the golf championship
Barclays Dubai Tennis for both men and women
UIM World Powerboat racing
Rugby Sevens
Dubai International Rally
Dubai Snooker Classic
The UAE Desert Challenge
The Standard Chartered Dubai Marathon
See also
[edit]
United Arab Emirates portal
Wikivoyage has a travel guide for Dubai.
Developments in Dubai
List of development projects in Dubai
List of tourist attractions in the United Arab Emirates
Palm Islands
Notes
[edit]
^Due to the COVID-19 pandemic.
^Due to the COVID-19 pandemic.
References
[edit]
^
"Two of the most-visited cities in the world are in Turkey - this one is the unsung hero". www.bbc.com. Retrieved 2024-07-15.
^Kelly, Liv (2 February 2024). "This surprising city was the world's most visited in 2023". TimeOut.
^"Dubai to host ATM 2024; city has 150,000 rooms and welcomed 17m tourists last year". Arabian Business. 2024-04-25. Retrieved 2024-07-15.
^"Enterprise". Enterprise. Retrieved 2024-07-15.
^"Dubai Tourist Information". Archived from the original on September 22, 2019. Retrieved Sep 27, 2019.
^Gluckman, Ron. "Hong Kong of the Desert?". Archived from the original on 4 February 2012. Retrieved 12 April 2012.
^Sharpley, Richard (2009). Tourism Development and the Environment:Beyond Sustainability?. Earthscan. p. 184. ISBN 978-1-84407-732-8. Archived from the original on 11 May 2022. Retrieved 16 November 2021.
^"Sorry, the page you requested was not found". www.zu.ac.ae. Archived from the original on November 10, 2020. Retrieved Jan 30, 2020.
^"Dubai Department of Tourism Vision". www.visitdubai.com. Archived from the original on September 22, 2019. Retrieved Sep 27, 2019.
^Bridge, Sam (5 October 2018). "Dubai expands tourism ambitions, sets new target for 2025". ArabianBusiness.com. Archived from the original on September 22, 2019. Retrieved Sep 27, 2019.
^Saifi, Zeena; Defterios, John; Swan, Melanie (6 February 2021). "How Dubai is paying the price for letting in tourists". CNN. Archived from the original on 18 October 2021. Retrieved 16 November 2021.
^Abdellatif, Reem (5 March 2021). "Dubai Faces Festering Tourism Challenges Beyond Pandemic". skift.com. Skift. Archived from the original on 16 November 2021. Retrieved 16 November 2021.
^National, The (November 11, 2022). "Sheikh Mohammed launches national tourism strategy to attract 40m hotel guests by 2031". The National.
^"UAE launches influencer academy to 'whitewash' country's reputation, say critics". Middle East Eye. 30 April 2025.
^ abHenderson, Joan c. (2006). "Tourism in Dubai: Overcoming Barriers to Destination Development". International Journal of Tourism Research. 8 (6): 84–85. CiteSeerX 10.1.1.606.2930. doi:10.1002/jtr.557. Archived from the original on 2021-03-04. Retrieved 2023-05-25.
^"8.36 million tourists visit Dubai in first half of 2019". Khaleej Times. Archived from the original on September 22, 2019. Retrieved Sep 27, 2019.
^"At $30 billion, Dubai takes in the most global tourist dollars by far". Consultancy-ME. 6 September 2019. Archived from the original on 15 September 2019. Retrieved 6 September 2019.
^"Dubai Tourism Statistics - Visitor Numbers, Number Of Hotels And Rooms". Dubai Online. Archived from the original on 2022-03-09. Retrieved 2022-04-29.
^ ab"About Dubai Tourism - DTCM Statistics & Performance | Visit Dubai". www.visitdubai.com. Archived from the original on September 16, 2019. Retrieved Sep 27, 2019.
^"Dubai tourism: number of visitors 2016". Statista. Archived from the original on November 7, 2019. Retrieved Sep 27, 2019.
^"Dubai received 15.92 million visitors in 2018 with most coming from India". The National. 24 February 2019. Archived from the original on 30 September 2019. Retrieved Sep 27, 2019.
^Fernandes, Cedwyn; Karnik, Ajit V. (2010). "Estimating Elasticity of Demand for Tourism in Dubai". Tourism Analysis. 15: 57–69. doi:10.3727/108354210X12724734223630. Archived from the original on January 26, 2022. Retrieved Jan 30, 2020 – via www.academia.edu.
^"Dubai welcomes 16.73 million tourists in 2019". Gulf Business. Jan 23, 2020. Archived from the original on September 2, 2020. Retrieved Jan 30, 2020.
^"UAE Tourism Statistics 1995-2021". www.macrotrends.net. Archived from the original on 2021-09-27. Retrieved 2021-03-04.
^ ab"Dubai hotels registered $4.1 bn revenues in 2008". The Economic Times. 10 March 2009. Archived from the original on 2022-05-11. Retrieved 2022-05-11.
^Stephenson, Marcus L.; Ali-Knight, Jane (December 1, 2010). "Dubai's tourism industry and its societal impact: social implications and sustainable challenges". Journal of Tourism and Cultural Change. 8 (4): 278–292. doi:10.1080/14766825.2010.521248. S2CID 115152557 – via Taylor and Francis+NEJM.
^Jain, Shweta (4 May 2010). "SPECIAL: Dubai's tourism sector bounces back - eb247 - News - National - Emirates24|7". www.emirates247.com. Archived from the original on 2021-12-05. Retrieved 2021-03-04.
^"Dubai receives 14.36 million international visitors in 2022".
^"Dubai annual visitor report 2023".
^"Tourism Performance Report January - December 2024".
^Bridge, Sam (12 September 2019). "Dubai hotels cut room rates to stimulate demand as supply accelerates". ArabianBusiness.com. Archived from the original on September 22, 2019. Retrieved Sep 27, 2019.
^Jr, Bernd Debusmann (29 August 2019). "Dubai hotel room rates fall, despite rise in occupancy". ArabianBusiness.com. Archived from the original on September 22, 2019. Retrieved Sep 27, 2019.
^Parasie, Nicolas; Pacheco, Filipe (29 July 2019). "Dubai's Jumeirah Cuts 500 Jobs as Tourism Industry Struggles". Bloomberg News. Archived from the original on 2019-07-31. Retrieved 2019-07-31.
^"Luxury Hotels Europe, Middle East & Far East - Jumeirah". www.jumeirah.com. Archived from the original on 2006-06-22.
^"Shopping in dubai". Archived from the original on 2006-06-25.
^"Shopping Guide in Dubai". Shopping Galore in Dubai. 17 October 2013. Archived from the original on 17 October 2013. Retrieved 17 October 2013.
^"Souq - DataDubai". Archived from the original on 2007-03-12.
^"How expensive is Dubai? A Budget for staying in Dubai". Travelaar. 2018-05-04. Archived from the original on 2019-05-09. Retrieved 2019-05-09.
^"Shopping at Dubai, Dubai Shopping Centers and Malls". www.dubai.com. Archived from the original on 2011-01-02. Retrieved 2008-12-18.
^"Dubai Shopping". www.mydsf.com. Archived from the original on 2006-05-15. Retrieved 2006-06-01.
^"Russian woman put in jail in Dubai for drinking juice in public", Pravda, 2008-09-23, archived from the original on 2015-02-03, retrieved 2010-04-08
^ ab"Know more about the Criminal Law of Dubai". Oct 23, 2012. Archived from the original on November 12, 2020. Retrieved Sep 27, 2019.
^"Dubai Mall dress code". Archived from the original on 2013-12-12. Retrieved 2014-10-14.
^"UAE: Dress Code Campaign Urges Extra Inches of Clothing · Global Voices". Jun 24, 2012. Archived from the original on November 27, 2020. Retrieved Sep 27, 2019.
^Boone, Jon (13 October 2017). "What not to do in Dubai". www.independent.co.uk. The Independent. Archived from the original on 16 November 2021. Retrieved 16 November 2021.
^"ACI World data reveals COVID-19's impact on world's busiest airports". www.aci.aero. 22 April 2021. Archived from the original on 2021-11-04. Retrieved 2021-11-04.
^ ab"Travel Tips to Visit Dubai | Dubai.com". www.dubai.com. Archived from the original on August 2, 2019. Retrieved Sep 27, 2019.
^"Cruise Hub of the Region". Dubai Tourism. Archived from the original on 2013-01-15. Retrieved 2012-12-23.
^"Routes to Dubai". Definitely Dubai. Archived from the original on 2012-12-13. Retrieved 2012-12-23.
^"Tourists rate Dubai taxis, shopping to top list". Khaleej Times. 20 December 2012. Archived from the original on 14 July 2014. Retrieved 11 May 2022.
^ abPaul McLennan and Ali Al-Shouk (2008-02-11). "Tourists get drug warning". Dubai City News. Archived from the original on 2008-05-10. Retrieved 2008-02-12.
^"Gulf News". Archived from the original on 2010-03-08.
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About ATV
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About Polaris
Northern pole-star; brightest star in Ursa Minor
This article is about the Earth's current north star. For such stars in general, see pole star. For other uses, see Polaris (disambiguation) and North Star (disambiguation).
"Stella Polaris" redirects here. For the military operation, see Operation Stella Polaris.
α UMi A: 1 Ursae Minoris, BD+88°8, FK5 907, GC 2243, HD 8890, HIP 11767, HR 424, SAO 308
α UMi B: NSV 631, BD+88°7, GC 2226, SAO 305
Database references
SIMBAD
α UMi A
α UMi B
Polaris is a star in the northern circumpolar constellation of Ursa Minor. It is designated α Ursae Minoris (Latinized to Alpha Ursae Minoris) and is commonly called the North Star. With an apparent magnitude that fluctuates around 1.98,[3] it is the brightest star in the constellation and is readily visible to the naked eye at night.[16] The position of the star lies less than 1° away from the north celestial pole, making it the current northern pole star. The stable position of the star in the Northern Sky makes it useful for navigation.[17]
Although appearing to the naked eye as a single point of light, Polaris is a triple star system, composed of the primary, a yellow supergiant designated Polaris Aa, in orbit with a smaller companion, Polaris Ab; the pair is almost certainly[14] in a wider orbit with Polaris B. The outer companion B was discovered in August 1779 by William Herschel, with the inner Aa/Ab pair only confirmed in the early 20th century.
As the closest Cepheid variable, Polaris Aa's distance is a foundational part of the cosmic distance ladder. The revised Hipparcos stellar parallax gives a distance to Polaris A of about 432 light-years (ly) (133 parsecs (pc)), while the successor mission Gaia gives a distance of 446.5 ly (136.9 pc) for Polaris B[9][a].
Stellar system
[edit]
Polaris components as seen by the Hubble Space Telescope
Polaris Aa is an evolved yellow supergiant of spectral type F7Ib with 5.4 solar masses (M☉). It is the first classical Cepheid to have a mass determined from its orbit. The two smaller companions are Polaris B, a 1.39 M☉ F3 main-sequence star orbiting at a distance of 2,400 astronomical units (AU),[18] and Polaris Ab (or P), a very close F6 main-sequence star with a mass of 1.26 M☉.[3] In January 2006, NASA released images, from the Hubble telescope, that showed the three members of the Polaris ternary system.[19][20]
Polaris B can be resolved with a modest telescope. William Herschel discovered the star in August 1779 using a reflecting telescope of his own, one of the best telescopes of the time.[21]
The variable radial velocity of Polaris A was reported by W. W. Campbell in 1899, which suggested this star is a binary system.[22] Since Polaris A is a known cepheid variable, J. H. Moore in 1927 demonstrated that the changes in velocity along the line of sight were due to a combination of the four-day pulsation period combined with a much longer orbital period and a large eccentricity of around 0.6.[23] Moore published preliminary orbital elements of the system in 1929, giving an orbital period of about 29.7 years with an eccentricity of 0.63. This period was confirmed by proper motion studies performed by B. P. Gerasimovič in 1939.[24]
As part of her doctoral thesis, in 1955 E. Roemer used radial velocity data to derive an orbital period of 30.46 y for the Polaris A system, with an eccentricity of 0.64.[25] K. W. Kamper in 1996 produced refined elements with a period of 29.59±0.02 years and an eccentricity of 0.608±0.005.[26] In 2019, a study by R. I. Anderson gave a period of 29.32±0.11 years with an eccentricity of 0.620±0.008.[10]
There were once thought to be two more widely separated components—Polaris C and Polaris D—but these have been shown not to be physically associated with the Polaris system.[18][27]
Observation
[edit]
Variability
[edit]
A light curve for Polaris, plotted from TESS data[28]
Polaris Aa, the supergiant primary component, is a low-amplitude population I classical Cepheid variable, although it was once thought to be a type II Cepheid due to its high galactic latitude. Cepheids constitute an important standard candle for determining distance, so Polaris, as the closest such star,[10] is heavily studied. The variability of Polaris had been suspected since 1852; this variation was confirmed by Ejnar Hertzsprung in 1911.[29]
The range of brightness of Polaris is given as 1.86–2.13,[4] but the amplitude has changed since discovery. Prior to 1963, the amplitude was over 0.1 magnitude and was very gradually decreasing. After 1966, it very rapidly decreased until it was less than 0.05 magnitude; since then, it has erratically varied near that range. It has been reported that the amplitude is now increasing again, a reversal not seen in any other Cepheid.[6]
The period, roughly 4 days, has also changed over time. It has steadily increased by around 4.5 seconds per year except for a hiatus in 1963–1965. This was originally thought to be due to secular redward evolution across the Cepheid instability strip, but it may be due to interference between the primary and the first-overtone pulsation modes.[20][30][31] Authors disagree on whether Polaris is a fundamental or first-overtone pulsator and on whether it is crossing the instability strip for the first time or not.[11][31][32]
The temperature of Polaris varies by only a small amount during its pulsations, but the amplitude of this variation is variable and unpredictable. The erratic changes of temperature and the amplitude of temperature changes during each cycle, from less than 50 K to at least 170 K, may be related to the orbit with Polaris Ab.[12]
A 4-day time lapse of Polaris illustrating its Cepheid type variability.
Research reported in Science suggests that Polaris is 2.5 times brighter today than when Ptolemy observed it, changing from third to second magnitude.[33] Astronomer Edward Guinan considers this to be a remarkable change and is on record as saying that "if they are real, these changes are 100 times larger than [those] predicted by current theories of stellar evolution".
Torres 2023 published a broad historical compilation of radial velocity and photometric data. He concludes that the change in the Cepheid period has reversed and is now decreasing since roughly 2010. Torres notes that TESS data is of limited utility: as a survey telescope, TESS is optimized for dimmer stars than Polaris, so Polaris significantly over-saturates TESS's cameras. Determining an accurate total brightness for Polaris from TESS is extremely difficult, although it remains suitable for timing the period.[34]
Furthermore, apparent irregularities in Polaris Aa's behavior may coincide with the periastron passage of Ab, although imprecision in the data prevents a definitive conclusion.[34] At the Gaia distance, the Aa-Ab closest approach is 6.2 AU; the radius of the primary supergiant is 46 R☉, meaning that the periastron separation is about 29 times its radius. This implies tidal forcing upon Aa's upper atmosphere by Ab. Such binary tidal forcing is known from heartbeat stars, where eccentric periastron approaches cause rich multimode pulsation akin to an electrocardiogram.
Szabados 1992 suggests that, among Cepheids, "phase slips" similar to what happened to Polaris in the mid 1960s are associated with binary systems.[35]
In 2024, researchers led by Nancy Evans at the Harvard & Smithsonian published a study with fresh data on the inner binary using the interferometric CHARA Array. They improved the solution of the orbit: combining CHARA data with previous Hubble data, and in tandem with the Gaia distance of 446±1 light-years, they confirmed the Cepheid radius estimate of 46 R☉ and re-determined its mass at 5.13±0.28M☉. The corresponding Polaris Ab mass is 1.316±0.028M☉. Polaris remains overluminous compared to the best Cepheid evolution models, something also seen in V1334 Cygni. Polaris's rapid period change and pulsation amplitude variations are still peculiar compared to other Cepheids, but may be related to the first-overtone pulsations.[9]
Evans et al also tentatively succeeded in imaging features on the surface of Polaris Aa: large bright and dark patches appear in close-up images, changing over time. Follow up imaging campaigns are required to confirm this detection.[9] Polaris's age is difficult to model; current best estimates find the Cepheid to be much younger than the two main sequence components, seemingly enough to exclude a common origin, which would be quite unlikely for a triple star system.[14][15]
Torres 2023 and Evans et al 2024 both suggest that recent literature cautiously agree that Polaris is a first overtone pulsator.[34][9]
Role as pole star
[edit]
Main article: Pole star
Polaris azimuths vis clock face analogy.[36]A typical Northern Hemisphere star trail with Polaris in the center.Polaris lying halfway between the asterisms Cassiopeia and the Big Dipper.
Because Polaris lies nearly in a direct line with the Earth's rotational axis above the North Pole, it stands almost motionless in the sky, and all the stars of the northern sky appear to rotate around it. It thus provides a nearly fixed point from which to draw measurements for celestial navigation and for astrometry. The elevation of the star above the horizon gives the approximate latitude of the observer.[16]
In 2018 Polaris was 0.66° (39.6 arcminutes) away from the pole of rotation (1.4 times the Moon disc) and so revolves around the pole in a small circle 1.3° in diameter. It will be closest to the pole (about 0.45 degree, or 27 arcminutes) soon after the year 2100.[37] Because it is so close to the celestial north pole, its right ascension is changing rapidly due to the precession of Earth's axis, going from 2.5h in AD 2000 to 6h in AD 2100. Twice in each sidereal day Polaris's azimuth is true north; the rest of the time it is displaced eastward or westward, and the bearing must be corrected using tables or a rule of thumb. The best approximation[36] is made using the leading edge of the "Big Dipper" asterism in the constellation Ursa Major. The leading edge (defined by the stars Dubhe and Merak) is referenced to a clock face, and the true azimuth of Polaris worked out for different latitudes.
The apparent motion of Polaris towards and, in the future, away from the celestial pole, is due to the precession of the equinoxes.[38] The celestial pole will move away from α UMi after the 21st century, passing close by Gamma Cephei by about the 41st century, moving towards Deneb by about the 91st century.[citation needed]
The celestial pole was close to Thuban around 2750 BCE,[38] and during classical antiquity it was slightly closer to Kochab (β UMi) than to Polaris, although still about 10° from either star.[39] It was about the same angular distance from β UMi as to α UMi by the end of late antiquity. The Greek navigator Pytheas in ca. 320 BC described the celestial pole as devoid of stars. However, as one of the brighter stars close to the celestial pole, Polaris was used for navigation at least from late antiquity, and described as ἀεί φανής (aei phanēs) "always visible" by Stobaeus (5th century), also termed Λύχνος (Lychnos) akin to a burner or lamp and would reasonably be described as stella polaris from about the High Middle Ages and onwards, both in Greek and Latin. On his first trans-Atlantic voyage in 1492, Christopher Columbus had to correct for the "circle described by the pole star about the pole".[40] In Shakespeare's play Julius Caesar, written around 1599, Caesar describes himself as being "as constant as the northern star", although in Caesar's time there was no constant northern star. Despite its relative brightness, it is not, as is popularly believed, the brightest star in the sky.[41]
Polaris was referenced in the classic Nathaniel Bowditch maritime navigation book American Practical Navigator (1802), where it is listed as one of the navigational stars.[42]
Names
[edit]
This artist's concept shows: supergiant Polaris Aa, dwarf Polaris Ab, and the distant dwarf companion Polaris B.
The modern name Polaris[43] is shortened from the Neo-Latin stella polaris ("polar star"), coined in the Renaissance when the star had approached the celestial pole to within a few degrees.[44][45]
Gemma Frisius, writing in 1547, referred to it as stella illa quae polaris dicitur ("that star which is called 'polar'"), placing it 3° 8' from the celestial pole.[44][45]
In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[46] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016 included a table of the first two batches of names approved by the WGSN; which included Polaris for the star α Ursae Minoris Aa.[47]
In antiquity, Polaris was not yet the closest naked-eye star to the celestial pole, and the entire constellation of Ursa Minor was used for navigation rather than any single star. Polaris moved close enough to the pole to be the closest naked-eye star, even though still at a distance of several degrees, in the early medieval period, and numerous names referring to this characteristic as polar star have been in use since the medieval period. In Old English, it was known as scip-steorra ("ship-star").[citation needed]
In the "Old English rune poem", the T-rune is apparently associated with "a circumpolar constellation", or the planet Mars.[48]
In the Hindu Puranas, it became personified under the name Dhruva ("immovable, fixed").[49]
In the later medieval period, it became associated with the Marian title of Stella Maris "Star of the Sea" (so in Bartholomaeus Anglicus, c. 1270s),[50] due to an earlier transcription error.[51]
An older English name, attested since the 14th century, is lodestar "guiding star", cognate with the Old Norse leiðarstjarna, Middle High German leitsterne.[52]
The ancient name of the constellation Ursa Minor, Cynosura (from the Greek κυνόσουρα "the dog's tail"),[53] became associated with the pole star in particular by the early modern period. An explicit identification of Mary as stella maris with the polar star (Stella Polaris), as well as the use of Cynosura as a name of the star, is evident in the title Cynosura seu Mariana Stella Polaris (i.e. "Cynosure, or the Marian Polar Star"), a collection of Marian poetry published by Nicolaus Lucensis (Niccolo Barsotti de Lucca) in 1655. [citation needed]
Ursa Minor as depicted in the 964 Persian work Book of Fixed Stars, Polaris named al-Judayy "الجدي" in the lower right.
Its name in traditional pre-Islamic Arab astronomy was al-Judayy الجدي ("the kid", in the sense of a juvenile goat ["le Chevreau"] in Description des Etoiles fixes),[54] and that name was used in medieval Islamic astronomy as well.[55][56] In those times, it was not yet as close to the north celestial pole as it is now, and used to rotate around the pole.[citation needed]
It was invoked as a symbol of steadfastness in poetry, as "steadfast star" by Spenser. Shakespeare's sonnet 116 is an example of the symbolism of the north star as a guiding principle: "[Love] is the star to every wandering bark / Whose worth's unknown, although his height be taken."[57]
In Julius Caesar, Shakespeare has Caesar explain his refusal to grant a pardon: "I am as constant as the northern star/Of whose true-fixed and resting quality/There is no fellow in the firmament./The skies are painted with unnumbered sparks,/They are all fire and every one doth shine,/But there's but one in all doth hold his place;/So in the world" (III, i, 65–71). Of course, Polaris will not "constantly" remain as the north star due to precession, but this is only noticeable over centuries.[citation needed]
In Inuit astronomy, Polaris is known as Nuutuittuq (syllabics: ᓅᑐᐃᑦᑐᖅ).[58]
In traditional Lakota star knowledge, Polaris is named "Wičháȟpi Owáŋžila". This translates to "The Star that Sits Still". This name comes from a Lakota story in which he married Tȟapȟúŋ Šá Wíŋ, "Red Cheeked Woman". However, she fell from the heavens, and in his grief Wičháȟpi Owáŋžila stared down from "waŋkátu" (the above land) forever.[59]
The Plains Cree call the star in Nehiyawewin: acâhkos êkâ kâ-âhcît "the star that does not move" (syllabics: ᐊᒑᐦᑯᐢ ᐁᑳ ᑳ ᐋᐦᒌᐟ).[60]
In Mi'kmawi'simk the star is named Tatapn.[61]
In the ancient Finnish worldview, the North Star has also been called taivaannapa and naulatähti ("the nailstar") because it seems to be attached to the firmament or even to act as a fastener for the sky when other stars orbit it. Since the starry sky seemed to rotate around it, the firmament is thought of as a wheel, with the star as the pivot on its axis. The names derived from it were sky pin and world pin.[citation needed]
Distance
[edit]
Since Leavitt's discovery of the Cepheid variable period-luminosity relationship, and corresponding utility as a standard candle, the distance to Polaris has been highly sought-after by astronomers. It is the closest Cepheid to Earth, and thus key to calibrating the Cepheid standard candle; Cepheids form the base of the cosmic distance ladder by which to probe the cosmological nature of the universe.[62]
Distance measurement techniques depend on whether or not components A and B are a physical pair, that is, gravitationally bound. If they are, then their estimated distance can be presumed to be equal.[b] Gravitational binding of this pair is well supported by observations, and the presumption of common distance is widely adopted in historical and recent estimates.[64][65][66][26][67][62][14][9]
For most of the 20th century, available observation technologies remained inadequate to precisely measure absolute parallax.[68][62] Instead, the main technique was to use theoretical models of stellar evolution for both main sequence and giant stars, combined with spectroscopic and photometric data to estimate distances. Such modeling relies on theoretical assumptions and guesses, and contains much systematic error and statistical uncertainties in population data. Even by 2013, these techniques were still struggling to achieve even 10% precision in either main sequence[69] or Cepheid[14] modeling.
Further progress was thus limited until the advent of Hipparcos, the first instrument able to engage in all-sky absolute parallax astrometry.[68] Its first data release was in 1997.
Selected distance estimates to Polaris
Published
Component
Distance
Source
Notes
ly
pc
1966
B
(359)[c]
(110)[c]
Fernie[64]
Photometry and modeling of B[c]
1977
B
(399)[d]
(122)[d]
Turner[65]
Photometry and modeling of B[d]
1978
A
356*
109*
Gauthier and Fernie[66]
Modeling extinction and Cepheid evolution of A
1996
B
359*
110*
Kamper[26]
Photometry and modeling of B, reproducing prior estimates
1997
A
431±29
132±9
Hipparcos[70]
All-sky/absolute[68] parallax observations, of the primary variable[e]
2004-2013
A, B
307±13
94±4
Turner/Turner et al
Cepheid evolution modeling[30], cluster kinematics and ZAMS fitting[30][67], photometry and modeling of B[67], spectral line ratios of A calibrated on yellow supergiants[62]
329±10
101±3
323±7
99±2
2007[f]
A
432±6
133±2
Hipparcos[2][69]
All-sky/absolute parallax observations, revised analysis, of the primary variable[f]
2008
B
357*
109.5*
Usenko & Klochkova[7]
Photometry and modeling of B
2014
A
>385
>118
Neilson[71]
Cepheid evolution modeling, independent of any distance prior
2018
B
521±20
160±6
Hubble, Bond et al.[14]
Relative[68] parallax of the wide component referencing photometrically-calibrated background stars
2018
B
445.3±1.7
136.6±0.5
Gaia DR2[72]
All-sky/absolute[68] parallax observations, of the wide component[g]
2020
B
446.5±1.1
136.9±0.3
Gaia DR3[5][9]
All-sky/absolute parallax observations, of the wide component[h]
^ * This estimate didn't state its uncertainty
After the arrival of the Hipparcos data, the distance to Polaris and consequent analysis of its Cepheid variation was controversial. The Hipparcos distance for Polaris was broadly but not universally adopted.[20] Immediately, the Hipparcos data for the nearest few hundred Cepheids appeared to clarify Cepheid models and to clear up then-tension in higher rungs of the distance ladder.[70] However alternatives remained; particularly by Turner et al, who published several papers between 2004 and 2013.[62]
Stellar parallax is the basis for the parsec, which is the distance from the Sun to an astronomical object which has a parallax angle of one arcsecond. (1 AU and 1 pc are not to scale, 1 pc = about 206265 AU)
In 2018, Bond et al[14] used the Hubble Space Telescope to provide an alternate direct measurement of Polaris's parallax; they summarize the back-and-forth:
However, Turner et al. (2013, hereafter TKUG13)[62] argue that the parallax of Polaris is considerably larger, 10.10 ± 0.20 mas (d = 99±2 pc). The evidence cited by TKUG13 for this “short” distance includes (1) a photometric parallax for Polaris B based on measured photometry, spectral classification, and main-sequence fitting; (2) a claim that there is a sparse cluster of A-, F-, and G-type stars within 3° of Polaris, with proper motions and radial velocities similar to that of the Cepheid, for which the Hipparcos parallaxes combined with main-sequence fitting give a distance of 99 pc; and (3) a determination of the absolute visual magnitude of Polaris based on line ratios in high-resolution spectra, calibrated against supergiants with well-established luminosities. [...]
[...]
In a critique of the TKUG13 paper, van Leeuwen (2013, hereafter L13)[69] defended the Hipparcos parallax by presenting details of the solution, concluding that “the Hipparcos data cannot in any way support” the large parallax advocated by TKUG13. Using Hipparcos data, L13 also questioned the reality of the sparse cluster proposed by TKUG13, presenting evidence against it both from the color versus absolute-magnitude diagram for stars within 3° of Polaris, and their non-clustered distribution of proper motions. Lastly, L13 examined the absolute magnitudes of nearly 400 stars of spectral type F3 V in the Hipparcos catalog with parallax errors of less than 10%, and showed that the absolute magnitude of Polaris B would fall well within the observed MV distribution for F3 V stars, based on either the Hipparcos parallax of A or the larger parallax proposed by TKUG13. Thus, he concluded that the photometric parallax of B does not give a useful discriminant.
— [14]
Bond et al go on to find a trigonometric parallax (independent of Hipparcos) that implies a distance further-still than the "long" Hipparcos distance, well outside the plausible range of the "short" distance estimates.
The next major step in high precision parallax measurements comes from Gaia, a space astrometry mission launched in 2013 and intended to measure stellar parallax to within 25 microarcseconds (μas).[74] Although it was originally planned to limit Gaia's observations to stars fainter than magnitude 5.7, tests carried out during the commissioning phase indicated that Gaia could autonomously identify stars as bright as magnitude 3. When Gaia entered regular scientific operations in July 2014, it was configured to routinely process stars in the magnitude range 3 – 20.[75] Beyond that limit, special procedures are used to download raw scanning data for the remaining 230 stars brighter than magnitude 3; methods to reduce and analyse these data are being developed; and it is expected that there will be "complete sky coverage at the bright end" with standard errors of "a few dozen μas".[76]
Gaia DR2 does not include a parallax for Polaris A, but a distance inferred from Polaris B is 136.6±0.5 pc (445.5±1.7 ly),[72] somewhat further than most previous estimates and (in principle) considerably more accurate. There are known to be considerable systematic uncertainties in DR2.[77]
Gaia DR3 significantly improved both the statistical and systematic uncertainties, although the latter remain numerous and on the order of 10–60 μas[63]; the new estimate is 136.9±0.3 pc (446.5±1.1 ly) using the baseline parallax zeropoint correction.[5][9][h]
Gaia DR4 (expected December 2026) will further improve the statistical and systematic uncertainties in general, and the data pipelines for variable and multiple stars in particular.[78] Multistar orbital solutions will become available, greatly aiding the study of Cepheids and Polaris, and in particular, may enable solving the outer AB orbit.[9]
In popular culture
[edit]
Polaris is depicted in the flag and coat of arms of the Canadian Inuit territory of Nunavut,[79] the flag of the U.S. states of Alaska and Minnesota,[80] and the flag of the U.S. city of Duluth, Minnesota.[81][82]
Vexillology
[edit]
Flag of Nunavut
Flag of Alaska
Flag of Minnesota
Flag of Duluth, Minnesota
Flag of Maine
Flag of Maine (1901–1909)
Flag of the Pan-American Exposition (1901)[83]
Sledge flag used by Francis Leopold McClintock in the Arctic (1852–1854)[84]
Heraldry
[edit]
Coat of arms of Nunavut
Seal of Minnesota
Seal of Maine
Coat of arms of Utsjoki[citation needed]
Ships
[edit]
The Chinese spy ship Beijixing is named after Polaris.
USS Polaris is named after Polaris
Gallery
[edit]
Polaris is the brightest star in the constellation of Ursa Minor (upper right).
Big Dipper and Ursa Minor in relation to Polaris
A view of Polaris in a small telescope. Polaris B is separated by 18 arc seconds from the primary star, Polaris A.
Polaris, its surrounding integrated flux nebula, and NGC188[dubious – discuss]
See also
[edit]
Stars portal
Astronomy portal
Extraterrestrial sky (for the pole stars of other celestial bodies)
List of nearest supergiants
Polar alignment
Sigma Octantis
Polaris Flare
Regiment of the North Pole
Notes
[edit]
^If A and B are a physical pair, then they share the same parallax; see #Distance
^Their minimum spatial separation is the angular separation: 0.09 mrad (18.2 arcseconds), i.e. 0.009% of their distance from Earth; it could be higher (2x-5x) depending on the orbital eccentricity and orientation of the apsides to Earth's sightline. In any case, distance estimate uncertainties have far exceeded 0.2%, with only Gaia approaching the latter precision, when neglecting systematic uncertainties.[63] Future Gaia data may enable solving this outer orbit, constraining the apsides and thus precisely determining the distance between the components.
^ abcThe paper only estimates an absolute magnitude of roughly 3.3 with an apparent magnitude of 8.51. That implies a distance modulus of 5.21, implying a distance around 110 pc. A notional magnitude error of ±0.3 would correspond to roughly ±16 pc error.
^ abcThe paper only estimates an absolute magnitude of roughly 3.16. Taken with the quoted apparent magnitude 8.6, that implies a distance modulus of 5.44, implying a distance around 122 pc. A notional magnitude error of ±0.1 would correspond to roughly ±6 pc error. Extinction was concluded to be negligible.
^Parallax 7.56±0.48 mas
^ abParallax 7.54±0.11 mas; observations from 1989 to 1993, first analysis published 1997, revised analysis published 2007.
^Statistical distance calculated using a weak distance prior
^ abThe raw parallax is 7.2869±0.0178 mas; applying a basic systematic[63] correction[73] gives 7.3045±0.0178 mas
References
[edit]
^
"Polaris | meaning in the Cambridge English Dictionary". Cambridge English Dictionary. Retrieved 11 December 2020.
^ abcdefVan Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.
^ abcdefghijklmEvans, N. R.; Schaefer, G. H.; Bond, H. E.; Bono, G.; Karovska, M.; Nelan, E.; Sasselov, D.; Mason, B. D. (2008). "Direct Detection of the Close Companion of Polaris with The Hubble Space Telescope". The Astronomical Journal. 136 (3): 1137. arXiv:0806.4904. Bibcode:2008AJ....136.1137E. doi:10.1088/0004-6256/136/3/1137. S2CID 16966094.
^ abcdSamus, N. N.; Kazarovets, E. V.; et al. (2017). "General Catalogue of Variable Stars". Astronomy Reports. 5.1. 61 (1): 80–88. Bibcode:2017ARep...61...80S. doi:10.1134/S1063772917010085. S2CID 125853869.
^ abcdVallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
^ abcdLee, B. C.; Mkrtichian, D. E.; Han, I.; Park, M. G.; Kim, K. M. (2008). "Precise Radial Velocities of Polaris: Detection of Amplitude Growth". The Astronomical Journal. 135 (6): 2240. arXiv:0804.2793. Bibcode:2008AJ....135.2240L. doi:10.1088/0004-6256/135/6/2240. S2CID 12176373.
^ abcdefghiUsenko, I. A.; Klochkova, V. G. (2008). "Polaris B, an optical companion of the Polaris (α UMi) system: Atmospheric parameters, chemical composition, distance and mass". Monthly Notices of the Royal Astronomical Society: Letters. 387 (1): L1. arXiv:0708.0333. Bibcode:2008MNRAS.387L...1U. doi:10.1111/j.1745-3933.2008.00426.x. S2CID 18848139.
^Campbell, William Wallace (1913). "The radial velocities of 915 stars". Lick Observatory Bulletin. 229: 113. Bibcode:1913LicOB...7..113C. doi:10.5479/ADS/bib/1913LicOB.7.113C.
^ abcdefghijklmEvans, Nancy Remage; Schaefer, Gail H.; Gallenne, Alexandre; Torres, Guillermo; Horch, Elliott P.; Anderson, Richard I.; Monnier, John D.; Roettenbacher, Rachael M.; Baron, Fabien; Anugu, Narsireddy; Davidson, James W.; Kervella, Pierre; Bras, Garance; Proffitt, Charles; Mérand, Antoine (2024-08-01). "The Orbit and Dynamical Mass of Polaris: Observations with the CHARA Array". The Astrophysical Journal. 971 (2): 190. arXiv:2407.09641. Bibcode:2024ApJ...971..190E. doi:10.3847/1538-4357/ad5e7a. ISSN 0004-637X.
^ abcAnderson, R. I. (March 2019). "Probing Polaris' puzzling radial velocity signals. Pulsational (in-)stability, orbital motion, and bisector variations". Astronomy & Astrophysics. 623: 17. arXiv:1902.08031. Bibcode:2019A&A...623A.146A. doi:10.1051/0004-6361/201834703. S2CID 119467242. A146.
^ abFadeyev, Y. A. (2015). "Evolutionary status of Polaris". Monthly Notices of the Royal Astronomical Society. 449 (1): 1011–1017. arXiv:1502.06463. Bibcode:2015MNRAS.449.1011F. doi:10.1093/mnras/stv412. S2CID 118517157.
^ abUsenko, I. A.; Miroshnichenko, A. S.; Klochkova, V. G.; Yushkin, M. V. (2005). "Polaris, the nearest Cepheid in the Galaxy: Atmosphere parameters, reddening and chemical composition". Monthly Notices of the Royal Astronomical Society. 362 (4): 1219. Bibcode:2005MNRAS.362.1219U. doi:10.1111/j.1365-2966.2005.09353.x.
^Cayrel de Strobel, G.; Soubiran, C.; Ralite, N. (2001). "Catalogue of [Fe/H] determinations for FGK stars: 2001 edition". Astronomy and Astrophysics. 373: 159–163. arXiv:astro-ph/0106438. Bibcode:2001A&A...373..159C. doi:10.1051/0004-6361:20010525. S2CID 17519049.
^ abcdefghiBond, Howard E; Nelan, Edmund P; Remage Evans, Nancy; Schaefer, Gail H; Harmer, Dianne (2018). "Hubble Space Telescope Trigonometric Parallax of Polaris B, Companion of the Nearest Cepheid". The Astrophysical Journal. 853 (1): 55. arXiv:1712.08139. Bibcode:2018ApJ...853...55B. doi:10.3847/1538-4357/aaa3f9. S2CID 118875464.
^ abcdNeilson, H. R.; Blinn, H. (2021). The Curious Case of the North Star: The Continuing Tension Between Evolution Models and Measurements of Polaris. RR Lyrae/Cepheid 2019: Frontiers of Classical Pulsators. Vol. 529. p. 72. arXiv:2003.02326. Bibcode:2021ASPC..529...72N.
^McNamee, Gregory (2021-05-26). "How the stars, planets and other celestial objects got their names". CNN. Retrieved 2024-08-28.
^ abWielen, R.; Jahreiß, H.; Dettbarn, C.; Lenhardt, H.; Schwan, H. (2000). "Polaris: Astrometric orbit, position, and proper motion". Astronomy and Astrophysics. 360: 399–410 [400–402, 406]. arXiv:astro-ph/0002406. Bibcode:2000A&A...360..399W.
^"There's More to the North Star Than Meets the Eye". Hubblesite.org. 2006-01-09. Retrieved 2020-02-27.
^ abcEvans, N. R.; Sasselov, D. D.; Short, C. I. (2002). "Polaris: Amplitude, Period Change, and Companions". The Astrophysical Journal. 567 (2): 1121. Bibcode:2002ApJ...567.1121E. doi:10.1086/338583.
^Argyle, Bob; et al. (August 29, 2019). An Anthology of Visual Double Stars. Cambridge University Press. p. 265. ISBN 9781108601702.
^Campbell, W. W. (October 1899). "On the variable velocity of Polaris in the line of sight". Publications of the Astronomical Society of the Pacific. 11: 195–199. Bibcode:1899PASP...11..195C. doi:10.1086/121339. S2CID 122429136.
^Moore, J. H. (August 1927). "Note on the Longitude of the Lick Observatory". Publications of the Astronomical Society of the Pacific. 39 (230): 249. Bibcode:1927PASP...39..249M. doi:10.1086/123734. S2CID 119469812.
^Roemer, Elizabeth (May 1965). "Orbital Motion of Alpha Ursae Minoris from Radial Velocities". Astrophysical Journal. 141: 1415. Bibcode:1965ApJ...141.1415R. doi:10.1086/148230.
^Wyller, A. A. (December 1957). "Parallax and orbital motion of spectroscopic binary Polaris from photographs taken with the 24-inch Sproul refractor". Astronomical Journal. 62: 389–393. Bibcode:1957AJ.....62..389W. doi:10.1086/107559.
^ abcKamper, Karl W. (June 1996). "Polaris Today". Journal of the Royal Astronomical Society of Canada. 90: 140. Bibcode:1996JRASC..90..140K.
^Evans, Nancy Remage; Guinan, Edward; Engle, Scott; Wolk, Scott J.; Schlegel, Eric; Mason, Brian D.; Karovska, Margarita; Spitzbart, Bradley (2010). "Chandra Observation of Polaris: Census of Low-mass Companions". The Astronomical Journal. 139 (5): 1968. Bibcode:2010AJ....139.1968E. doi:10.1088/0004-6256/139/5/1968.
^"MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
^Hertzsprung, Ejnar (August 1911). "Nachweis der Veränderlichkeit von α Ursae Minoris". Astronomische Nachrichten (in German). 189 (6): 89. Bibcode:1911AN....189...89H. doi:10.1002/asna.19111890602.
^ abcTurner, D. G.; Savoy, J.; Derrah, J.; Abdel-Sabour Abdel-Latif, M.; Berdnikov, L. N. (2005). "The Period Changes of Polaris". Publications of the Astronomical Society of the Pacific. 117 (828): 207. Bibcode:2005PASP..117..207T. doi:10.1086/427838.
^ abNeilson, H. R.; Engle, S. G.; Guinan, E.; Langer, N.; Wasatonic, R. P.; Williams, D. B. (2012). "The Period Change of the Cepheid Polaris Suggests Enhanced Mass Loss". The Astrophysical Journal. 745 (2): L32. arXiv:1201.0761. Bibcode:2012ApJ...745L..32N. doi:10.1088/2041-8205/745/2/L32. S2CID 118625176.
^Engle, Scott G; Guinan, Edward F; Harmanec, Petr (2018). "Toward Ending the Polaris Parallax Debate: A Precise Distance to Our Nearest Cepheid from Gaia DR2". Research Notes of the AAS. 2 (3): 126. Bibcode:2018RNAAS...2..126E. doi:10.3847/2515-5172/aad2d0. S2CID 126329676.
^Irion, R (2004). "American Astronomical Society meeting. As inconstant as the Northern Star". Science. 304 (5678): 1740–1. doi:10.1126/science.304.5678.1740b. PMID 15205508. S2CID 129246155.
^ abcTorres, Guillermo (2023). "The spectroscopic orbit of Polaris and its pulsation properties". Monthly Notices of the Royal Astronomical Society. 526 (2): 2510. arXiv:2309.03257. Bibcode:2023MNRAS.526.2510T. doi:10.1093/mnras/stad2735.
^Szabados, L. (1992). "Effects of Duplicity on the Period Changes of Cepheids". IAU Colloquium 135: Complementary Approaches to Double and Multiple Star Research. 32: 255. Bibcode:1992ASPC...32..255S.
^ ab"A visual method to correct a ship's compass using Polaris using Ursa Major as a point of reference". Archived from the original on 2010-08-27. Retrieved 2016-08-07.
^Meeus, J. (1990). "Polaris and the North Pole". Journal of the British Astronomical Association. 100: 212. Bibcode:1990JBAA..100..212M.
^ abRidpath, Ian, ed. (2004). Norton's Star Atlas. New York: Pearson Education. p. 5. ISBN 978-0-13-145164-3. Around 4800 years ago Thuban (
α Draconis) lay a mere 0°.1 from the pole. Deneb (α Cygni) will be the brightest star near the pole in about 8000 years' time, at a distance of 7°.5.
^Ridpath, Ian (2018). "Ursa Minor, the Little Bear". Star Tales. Retrieved 20 August 2016.
^Columbus, Ferdinand (1960). The Life of the Admiral Christopher Columbus by His Son Fredinand. Translated by Keen, Benjamin. London: Folio Society. p. 74.
^Geary, Aidan (June 30, 2018). "Look up, be patient and 'think about how big the universe is': Expert tips for stargazing this summer". Canadian Broadcasting Corporation. Retrieved June 29, 2024.
^Bowditch, Nathaniel; National Imagery and Mapping Agency (2002). "15". The American practical navigator : an epitome of navigation. Paradise Cay Publications. p. 248. ISBN 978-0-939837-54-0.
^IAU Working Group on Star Names "IAU Catalog of Star Names". Retrieved 2016-07-28.
^ abGemmae Frisii de astrolabo catholico liber: quo latissime patentis instrumenti multiplex usus explicatur, & quicquid uspiam rerum mathematicarum tradi possit continetur. Steelsius. 1556. p. 20.
^ abKunitzsch, Paul; Smart, Tim (2006). A Dictionary of Modern star Names: A Short Guide to 254 Star Names and Their Derivations (2nd rev. ed.). Cambridge, Massachusetts: Sky Publishing. p. 23. ISBN 978-1-931559-44-7.
^"International Astronomical Union | IAU". www.iau.org. Retrieved 2019-01-19.
^"Bulletin of the IAU Working Group on Star Names, No. 1" (PDF).
^Dickins, Bruce (1915). Runic and heroic poems of the old Teutonic peoples. p. 18; Dickins' "a circumpolar constellation" is attributed to L. Botkine, La Chanson des Runes (1879).
^Daniélou, Alain (1991). The Myths and Gods of India: The Classic Work on Hindu Polytheism. Princeton/Bollingen (1964); Inner Traditions/Bear & Co. p. 186. ISBN 978-0-892-813544.
^Halliwell-Phillipps, James Orchard, ed. (1856). The Works of William Shakespeare. Vol. 5. p. 40.
^Herbermann, Charles, ed. (1913). "The Name of Mary". Catholic Encyclopedia. New York: Robert Appleton Company.
^Kluge, Friedrich; Götze, Alfred (1943). Etymologisches Wörterbuch der deutschen Sprache. Walter de Gruyter. p. 355. ISBN 978-3-111-67185-7. cite book: ISBN / Date incompatibility (help)
^Ridpath, Ian (2018-06-28). Star Tales. Lutterworth Press. ISBN 978-0-7188-4782-1.
^ʻAbd al-Raḥmān ibn ʻUmar Ṣūfī (1874). Description des Etoiles fixes. Commissionnaires de lÁcadémie Impériale des sciences. p. 45.
^Al-Sufi, AbdulRahman (964). "Book Of Fixed Stars".
^Schjellerup, Hans (1874). Description des Etoiles fixes. p. 45.
^Beach, Richard; Thein, Amanda Haertling; Webb, Allen (2012-06-25). Teaching to Exceed the English Language Arts Common Core State Standards: A Literacy Practices Approach for 6-12 Classrooms. Routledge. pp. Chp 6. ISBN 978-1-136-50288-0.
^Penprase, Bryan E. (2011). "Northern Circumpolar Sky from Around the World: The Arctic Inuit Sky". The Power of Stars. New York, NY: Springer. p. 45. ISBN 978-1-4419-6802-9.
^Wind, Dakota (2019-12-27). "Winter Solstice is Sacred Time a Time to Carry One Another by Dakota Wind". Last Real Indians.
^"Polaris". Plains Cree Dictionary. Retrieved 13 December 2022.
^Lebans, Jim (2022-09-29). "Mi'kmaw astronomer says we should acknowledge we live under Indigenous skies". Canadian Broadcasting Corporation. Retrieved 2022-12-21.
^ abcdefTurner, D. G.; Kovtyukh, V. V.; Usenko, I. A.; Gorlova, N. I. (2013). "The Pulsation Mode of the Cepheid Polaris". The Astrophysical Journal Letters. 762 (1): L8. arXiv:1211.6103. Bibcode:2013ApJ...762L...8T. doi:10.1088/2041-8205/762/1/L8. S2CID 119245441.
^ abcKhan, S.; Anderson, R. I.; Miglio, A.; Mosser, B.; Elsworth, Y. P. (2023). "Investigating Gaia EDR3 parallax systematics using asteroseismology of cool giant stars observed by Kepler, K2, and TESS. II. Deciphering Gaia parallax systematics using red clump stars". Astronomy and Astrophysics. 680: A105. arXiv:2310.03654. Bibcode:2023A&A...680A.105K. doi:10.1051/0004-6361/202347919.
^ abFernie, J. D. (1966). "Classical Cepheids with companions. II. Polaris". Astronomical Journal. 71: 732. Bibcode:1966AJ.....71..732F. doi:10.1086/110179.
^ abTurner, D. G. (1977). "A Note on the Reddening of Polaris B". Publications of the Astronomical Society of the Pacific. 89: 550. Bibcode:1977PASP...89..550T. doi:10.1086/130161.
^ abGauthier, R. P.; Fernie, J. D. (1978). "The reddening of Polaris". Publications of the Astronomical Society of the Pacific. 90: 739. Bibcode:1978PASP...90..739G. doi:10.1086/130422.
^ abcTurner, D. G. (2005). "Is Polaris Leaving the Cepheid Instability Strip?". Odessa Astronomical Publications. 18: 115. Bibcode:2005OAP....18..115T.
^ abcdeBrown, Anthony G. A. (2021). "Microarcsecond Astrometry: Science Highlights from Gaia". Annual Review of Astronomy and Astrophysics. 59: 59. arXiv:2102.11712. Bibcode:2021ARA&A..59...59B. doi:10.1146/annurev-astro-112320-035628.
^ abcVan Leeuwen, F. (2013). "The HIPPARCOS parallax for Polaris". Astronomy and Astrophysics. 550: L3. arXiv:1301.0890. Bibcode:2013A&A...550L...3V. doi:10.1051/0004-6361/201220871.
^ abFeast, M. W.; Catchpole, R. M. (1997). "The Cepheid period-luminosity zero-point from HIPPARCOS trigonometrical parallaxes". Monthly Notices of the Royal Astronomical Society. 286 (1): L1 –L5. Bibcode:1997MNRAS.286L...1F. doi:10.1093/mnras/286.1.L1.
^Neilson, H. R. (2014). "Revisiting the fundamental properties of the Cepheid Polaris using detailed stellar evolution models". Astronomy & Astrophysics. 563: A48. arXiv:1402.1177. Bibcode:2014A&A...563A..48N. doi:10.1051/0004-6361/201423482. S2CID 119252434.
^ abBailer-Jones, C. A. L; Rybizki, J; Fouesneau, M; Mantelet, G; Andrae, R (2018). "Estimating Distance from Parallaxes. IV. Distances to 1.33 Billion Stars in Gaia Data Release 2". The Astronomical Journal. 156 (2): 58. arXiv:1804.10121. Bibcode:2018AJ....156...58B. doi:10.3847/1538-3881/aacb21. S2CID 119289017.
^Lindegren, L.; Bastian, U.; Biermann, M.; Bombrun, A.; De Torres, A.; Gerlach, E.; Geyer, R.; Hernández, J.; Hilger, T.; Hobbs, D.; Klioner, S. A.; Lammers, U.; McMillan, P. J.; Ramos-Lerate, M.; Steidelmüller, H.; Stephenson, C. A.; Van Leeuwen, F. (2021). "Gaia Early Data Release 3. Parallax bias versus magnitude, colour, and position". Astronomy and Astrophysics. 649. arXiv:2012.01742. Bibcode:2021A&A...649A...4L. doi:10.1051/0004-6361/202039653.
^Liu, C.; Bailer-Jones, C. A. L.; Sordo, R.; Vallenari, A.; et al. (2012). "The expected performance of stellar parametrization with Gaia spectrophotometry". Monthly Notices of the Royal Astronomical Society. 426 (3): 2463. arXiv:1207.6005. Bibcode:2012MNRAS.426.2463L. doi:10.1111/j.1365-2966.2012.21797.x. S2CID 1841271.
^Martín-Fleitas, J.; Sahlmann, J.; Mora, A.; Kohley, R.; Massart, B.; l'Hermitte, J.; Le Roy, M.; Paulet, P. (2014). Oschmann, Jacobus M; Clampin, Mark; Fazio, Giovanni G; MacEwen, Howard A (eds.). "Enabling Gaia observations of naked-eye stars". Space Telescopes and Instrumentation 2014: Optical. Space Telescopes and Instrumentation 2014: Optical, Infrared, and Millimeter Wave. 9143: 91430Y. arXiv:1408.3039. Bibcode:2014SPIE.9143E..0YM. doi:10.1117/12.2056325. S2CID 119112009.
^T. Prusti; et al. (GAIA Collaboration) (2016). "The Gaia mission". Astronomy and Astrophysics (forthcoming article). 595: A1. arXiv:1609.04153. Bibcode:2016A&A...595A...1G. doi:10.1051/0004-6361/201629272. S2CID 9271090.
^Khan, S.; Miglio, A.; Mosser, B.; Arenou, F.; Belkacem, K.; Brown, A. G. A.; Katz, D.; Casagrande, L.; Chaplin, W. J.; Davies, G. R.; Rendle, B. M.; Rodrigues, T. S.; Bossini, D.; Cantat-Gaudin, T.; Elsworth, Y. P.; Girardi, L.; North, T. S. H.; Vallenari, A. (2019). "New light on the Gaia DR2 parallax zero-point: Influence of the asteroseismic approach, in and beyond the Kepler field". Astronomy and Astrophysics. 628: A35. arXiv:1904.05676. Bibcode:2019A&A...628A..35K. doi:10.1051/0004-6361/201935304.
^Brown, Anthony G. A. (2025). "Gaia: Ten Years of Surveying the Milky Way and Beyond". arXiv:2503.01533v1 [astro-ph.GA].
^"The Coat of Arms of Nunavut. (n.d.)". Legislative Assembly of Nunavut. Retrieved 2021-09-15.
^Swanson, Stephen (2023-12-15). "YouTuber's critique of Minnesota state flag finalists draws 1 million views". CBS Minnesota. Retrieved 2024-08-28.
^"Duluth Picks New City Flag". Fox 21. 2019-08-14. Retrieved 2024-09-03.
^Van Daele, Kate (2019-08-14). "City of Duluth selects new flag" (PDF). City of Duluth. Retrieved 2024-09-05.
^"Pan-American Flag". panam1901.org. Retrieved 16 November 2024.
^"Sir Francis McClintock Explorer - Arctic Fox Exhibition, Louth County Museum (Gallery Section)". arcticfoxtrail.com. Retrieved 14 January 2025.
Wikimedia Commons has media related to Polaris.
Preceded by
Kochab & Pherkad
Pole star
500–3000
Succeeded by
Gamma Cephei
v
t
e
Pole star
Earth
Current
Northern
Polaris
Southern
Polaris Australis
Past and future
Northern
Vega
ι Herculis
τ Herculis
Thuban
Kochab
Errai
ι Cephei
Alfirk
Alderamin
Deneb
Fawaris
Southern
β Hydri
γ Chamaeleontis
I Carinae
ω Carinae
υ Carinae
Aspidiske
Alsephina
Canopus
Sirius
Other planets
Mercury
Northern
o Draconis
Southern
α Pictoris
Venus
Northern
η1 Doradus
Southern
Fafnir
Mars
Northern
Markeb
Southern
Sadr
Deneb
Jupiter
Northern
Aldhibah
Southern
δ Doradus
Saturn
Northern
Polaris
Southern
δ Octantis
Uranus
Northern
Sabik
Southern
15 Orionis
Neptune
Northern
Sadr
Fawaris
Southern
Regor
Other bodies
Moon
Northern
o Draconis
Southern
δ Doradus
Past and future
ω Draconis
36 Draconis
See also
Polarissima Borealis
Polarissima Australis
v
t
e
Constellation of Ursa Minor
List of stars in Ursa Minor
Ursa Minor in Chinese astronomy
Stars
Bayer
α (Polaris)
β (Kochab)
γ (Pherkad)
δ (Yildun)
ε
ζ
η
θ
λ
π1
π2
Flamsteed
3
4
5
6
8 (Baekdu)
9
10
11
12
14
17
19
20
24
Variable
R
S
T
U
V
W
Z
RR
RU
RW
SS
UY
VX
HR
5184
5596
HD
150706
Other
Calvera
H1504+65
LP 40-365
WD 1337+705
WISE 1506+7027
Exoplanets
β Ursae Minoris b
8 Ursae Minoris b (Halla)
11 Ursae Minoris b
TOI-4138 b
Galaxies
NGC
5034
5144
5939
6217
6251
6331
Other
3C 303.1
3C 309.1
Galaxy clusters
Abell 2256
Category
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Yale LUX
About Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates
It was an amazing experience driving through the desert with a 4x4, having a great dinner in the camp with good entertainment. And our driver Mohammed was awesome: very friendly, always pointing out interesting things to see and thankfully very skilled when driving through the dunes.
Arabian Nights Tours Camp in Abu Dhabi, UAE, offers an immersive desert adventure experience. Located in the heart of the Arabian desert, the camp provides guests with a traditional Bedouin-style setting, complete with comfortable tents and authentic decor. Visitors can enjoy a range of activities, including dune bashing, camel rides, and sandboarding. The camp also features cultural entertainment such as belly dancing, henna painting, and traditional music. Guests are treated to a sumptuous buffet of Arabic cuisine under the stars, making for a memorable and picturesque desert experience. Arabian Nights Tours Camp combines adventure, culture, and relaxation in a stunning desert landscape.
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
Desert Safari Dubai - Dune Buggy Rental & ATV Quad Bike Tours - Marasi Drive - Dubai - United Arab Emirates, Lake Central Tower 4th Floor - Office 404 مراسي درايف - الخليج التجاري - دبي - United Arab Emirates
What payment methods are accepted for Quad Biking Tours Dubai?
We accept card payments online through our secure booking system and cash payments on the day of your Quad Biking Tours Dubai visit. All major credit cards are welcome.
How do I book Quad Biking Tours Dubai?
Book your Quad Biking Tours Dubai by calling our 24 hour line at 971 52 440 9525 or email info@dunebuggyrentalsdubai.com. Online booking and WhatsApp reservations are also available.
Can I cancel my Quad Biking Tours Dubai reservation?
Yes we offer flexible cancellation policies for Quad Biking Tours Dubai. Contact our team in advance if your plans change and we will assist with rescheduling or cancellation.