Betelgeuse
HIP 27989; Alpha Ori; 58 Ori
Range: 0.0 - 1.6, Period: 420.0d, Type: SRC
물리적 특성
위치 & 식별자
가시성
사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.
광도 곡선
다중 항성계
접안렌즈 시야
Sep: 37.5″ · PA: 113° · 위=북, 왼쪽=동
분해됨 · Rayleigh: 2.3″ · Dawes: 1.9″ · Eff: 3.1″
크기 비교
항성의 진화
분광 분류
헤르츠스프룽-러셀 도표
흑체 복사 스펙트럼
항성 흡수 스펙트럼
스펙트럼 유형을 기반으로 한 시뮬레이션 흡수 스펙트럼. 선 위에 마우스를 올려 원소를 식별하세요.
항성 참고사항
서베이 이미지
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Betelgeuse 소개
설명
Betelgeuse is a red supergiant of spectral type M1-M2Ia-Iab, one of the largest stars visible to the naked eye. Located about 650 light-years from Earth, it marks the upper left shoulder of Orion. Betelgeuse is roughly 700-1,000 times the diameter of the Sun — if placed at the center of our solar system, its surface would extend beyond the orbit of Jupiter. It is a semiregular variable star, fluctuating between about magnitude 0.0 and 1.6 over periods of roughly 400 days. Its luminosity is about 100,000 times that of the Sun.
관측 팁
Betelgeuse is instantly recognizable as the distinctly red-orange star at Orion's upper left shoulder. Its color contrast with blue-white Rigel at the opposite corner of Orion is one of the most striking sights in the sky. Monitoring Betelgeuse's brightness changes relative to nearby reference stars (Aldebaran, Pollux, Procyon) is an excellent visual variable star project. Best observed from November through March. In late 2019-early 2020, Betelgeuse underwent an unprecedented dimming event that sparked worldwide attention.
역사
The name Betelgeuse likely derives from the Arabic 'Yad al-Jawza' meaning 'hand of the central one,' though the precise etymology is debated. It was among the first stars to have its angular diameter measured, by Albert Michelson and Francis Pease using the Mount Wilson 100-inch telescope's interferometer in 1920. Its variable nature was first noted by Sir John Herschel in 1836.
재미있는 사실
Betelgeuse will almost certainly explode as a Type II supernova within the next 100,000 years. When it does, it will briefly shine as bright as the full Moon and be visible in daylight. The 'Great Dimming' of 2019-2020 was likely caused by a massive surface eruption that ejected material which condensed into dust, temporarily blocking part of the star's light.