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Doha vs. Vega - Comparison of sizes
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Doha
Vega

Doha vs Vega

Doha
Vega
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Doha

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Doha (Arabic: الدوحة‎, ad-Dawḥa or ad-Dōḥa, pronounced [adˈdawħa]) is the capital and most populous city of the State of Qatar. It has a population of 956,460 (2015). The city is located on the shore of the Persian Gulf in the east of the country, North of Al Wakrah and South of Al Khor. It is Qatar's fastest growing city, with over 80 percent of the country's population living in Doha or its surrounding suburbs, and it's the political and economic center of the nation. Doha was founded in the 1820s as an offshoot of Al Bidda. It was officially declared as the nation's capital in 1971, when Qatar gained independence from being a British Protectorate. As the commercial capital of Qatar and one of the emergent financial centers in the Middle East, Doha is considered a beta-level global city by the Globalization and World Cities Research Network. Doha accommodates Education City, an area dedicated to education and research; Hamad Medical City, an Hamad Medical Corporation administrative area of medical care which includes Hamad General Hospital, Heart Hospital, Women's Wellness and Research Center and Qatar Rehabilitation Institute as well as a number of specialty clinics and support infrastructure.



Finally, it also includes Doha Sports City, or Aspire Zone, a global sports destination which includes Khalifa International Stadium, a FIFA WorldCup 2022 stadium, as well as Hamad Aquatic Center, and the Aspire Dome. The city was host to the first ministerial-level meeting of the Doha Development Round of World Trade Organization negotiations. It was also selected as host city of a number of sporting events, including the 2006 Asian Games, the 2011 Pan Arab Games and the majority of the games in the 2011 AFC Asian Cup. In December 2011, the World Petroleum Council held the 20th World Petroleum Conference in Doha. Furthermore, the city hosted the 2012 UNFCCC Climate Negotiations and is set to host the 2022 FIFA World Cup. The city has also hosted the 140th Inter-Parliamentary Union Assembly in April 2019.

Source: Wikipedia
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Vega

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Vega is the brightest star in the northern constellation of Lyra. It has the Bayer designation α Lyrae, which is Latinised to Alpha Lyrae and abbreviated Alpha Lyr or α Lyr. This star is relatively close at only 25 light-years from the Sun, and, together with Arcturus and Sirius, one of the most luminous stars in the Sun's neighborhood. It is the fifth-brightest star in the night sky, and the second-brightest star in the northern celestial hemisphere, after Arcturus. Vega has been extensively studied by astronomers, leading it to be termed "arguably the next most important star in the sky after the Sun". Vega was the northern pole star around 12,000 BC and will be so again around the year 13,727, when its declination will be +86° 14′. Vega was the first star other than the Sun to be photographed and the first to have its spectrum recorded. It was one of the first stars whose distance was estimated through parallax measurements. Vega has functioned as the baseline for calibrating the photometric brightness scale and was one of the stars used to define the zero point for the UBV photometric system.



Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive, its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their life expectancies. Vega has an unusually low abundance of the elements with a higher atomic number than that of helium. Vega is also a variable star that varies slightly in brightness. It is rotating rapidly with a velocity of 236 km/s at the equator. This causes the equator to bulge outward due to centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is observed from the direction of one of these poles.Based on an observed excess emission of infrared radiation, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess due to dust emission are termed Vega-like stars.

Source: Wikipedia

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