Bagé vs Vega

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Fulham Football Club is an English professional association football club based in Fulham, London. They will compete in the Premier League in the 2022–23 season following their promotion. Founded in 1879, they are London's oldest football club playing professionally.The club has spent 27 seasons in English football's top division, the majority of which have come in two periods during the 1960s and 2000s. The latter period was associated with former chairman Mohamed Al-Fayed, after the club had climbed up from the fourth tier in the 1990s.

Fulham have reached two major finals: in 1975 they lost 2–0 against West Ham United in the FA Cup Final as a Second Division team, and in 2010 they played Atlético Madrid in the UEFA Europa League Final, losing 2–1 after extra time. Fulham's main rivalries are with fellow West London clubs Chelsea, Queens Park Rangers and Brentford. The club adopted a white shirt and black shorts as its kit in 1903, which has been used ever since.

Source: Wikipedia

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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