Capella
HIP 24608; Alpha Aur; 13 Aur
물리적 특성
위치 & 식별자
가시성
사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.
다중 항성계
접안렌즈 시야
Sep: 91.5″ · PA: 6° · 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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Capella 소개
설명
Capella is the sixth brightest star in the night sky at magnitude 0.08, located in the constellation Auriga about 43 light-years from Earth. It is actually a spectroscopic binary system consisting of two yellow giant stars: Capella Aa (spectral type G8III, about 79 solar luminosities) and Capella Ab (G1III, about 78 solar luminosities), orbiting each other every 104 days at a separation of about 0.74 AU. A distant pair of red dwarfs (Capella H and L) also belongs to the system.
관측 팁
Capella is easily recognized as the brilliant yellowish star high in the northern sky during winter evenings. It forms a distinctive pentagon shape with the other bright stars of Auriga. The binary nature of Capella cannot be resolved visually — the two giant stars orbit too closely (0.05 arcseconds) — but their combined light makes a striking golden beacon. The nearby open clusters M36, M37, and M38 in Auriga make excellent binocular targets in the same region. Best observed from October through April. Capella is circumpolar from latitudes north of about 44°N.
역사
The name Capella means 'little she-goat' in Latin, associated with the mythological goat Amalthea that suckled the infant Zeus. The Romans called it 'Capra.' It was listed in most ancient star catalogs, including Ptolemy's Almagest. The binary nature of Capella was discovered spectroscopically in 1899, and interferometric observations have since directly measured the orbit of the two giant components.
재미있는 사실
Both giant stars of Capella are in a relatively brief evolutionary phase — they have exhausted the hydrogen in their cores and are now expanding and cooling. In a few million years, they will swell further into red giants. Capella is the closest first-magnitude star to the north celestial pole and one of the best-studied binary systems in the sky.