베가

3Alp Lyr

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Vega — Alpha Lyrae, the leading star of the small constellation Lyra — is a white A-type star whose B–V colour index of −0.001 is almost exactly neutral, long making it a photometric benchmark for stellar colour. It shines at apparent magnitude 0.03 from a distance of 25 light-years, and its absolute magnitude of 0.6 shows an intrinsic brightness only modestly above the value it presents to Earth. Positioned at a northern declination of +38°, Vega climbs high overhead from mid-northern latitudes and forms one apex of the Summer Triangle. Its brilliance and pure white light make it one of the most recognisable stars of the northern summer evening.

물리적 특성

분광형 A Class A — A-type (White)
색지수 (B−V) -0.001

관측

겉보기 등급 +0.03
절대 등급 0.60
거리 25.0 ly
별자리 Lyra

위치

적경 18h 36.94m
적위 38° 47.02′

Related Chemistry

Explore the chemical elements connected to 베가 on our sister site ChemFYI.

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Frequently Asked Questions

What type of star is 베가?
베가 is a Class A — A-type (White) star.
How far is 베가 from Earth?
베가 is approximately 25.0 light-years from Earth.
Can you see 베가 with the naked eye?
With an apparent magnitude of 0.03, 베가 is visible to the naked eye.
What constellation is 베가 in?
베가 is located in the constellation Lyra.