Vega vs Makó

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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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Makó ([ˈmɒkoː], German: Makowa, Yiddish: מאַקאָווע‎ Makowe, Romanian: Macău or Macovia, Slovak: Makov) is a town in Csongrád County, in southeastern Hungary, 10 km (6 mi) from the Romanian border. It lies on the Mureș River. Makó is home to 23,272 people and it has an area of 229.23 square kilometres (88.51 square miles), of which 196.8 km2 (76.0 sq mi) is arable land. Makó is the fourth-largest town in Csongrád County after Szeged, Hódmezővásárhely and Szentes. The town is 28.6 km (17.8 mi) from Hódmezővásárhely, 36.2 km (22.5 mi) from Szeged, 75.4 km (46.9 mi) from Arad, 85 km (52.8 mi) from Gyula, 93.5 km (58.1 mi) from Timișoara (Temesvár), and 200 km (124 mi) from Budapest.

The climate is warmer than anywhere else in Hungary, with hot, dry summers. The town is noted for its onion which is a hungarikum, the spa and the thermal bath. The Makó International Onion Festival, the largest of its kind, is held annually. Makó is a popular tourist destination in Hungary. The Makó gas field, located near the town, is the largest natural gas field in Central Europe. The gas volume is more than 600 billion cubic metres (21 trillion cubic feet), according to a report by the Scotia Group. The town's floodplain forests are protected as part of Körös-Maros National Park.

Source: Wikipedia