Achernar
HIP 7588; Alpha Eri
물리적 특성
위치 & 식별자
가시성
사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.
다중 항성계
접안렌즈 시야
Sep: 0.3″ · PA: 309° · 위=북, 왼쪽=동
미분해 · 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
서베이 이미지 로드 중…
Achernar 소개
설명
Achernar is the brightest star in the constellation Eridanus and the ninth brightest in the night sky at magnitude 0.46. It is a blue main-sequence star of spectral type B6V, located about 139 light-years from Earth. Achernar is roughly 6-7 times the mass of the Sun and about 3,000 times more luminous. It is one of the flattest stars known, spinning so rapidly (at about 250 km/s at its equator) that its equatorial diameter is about 56% larger than its polar diameter.
관측 팁
Achernar marks the southern end of the long, winding constellation Eridanus (the River). It is visible only from latitudes south of about 33°N. Its brilliant blue-white color and isolated position make it easy to identify from the Southern Hemisphere. There are few other bright stars in its immediate vicinity, which makes it stand out dramatically. Best observed from October through January from southern latitudes.
역사
The name Achernar derives from the Arabic 'Akhir an-Nahr' meaning 'the end of the river,' referring to its position at the southern terminus of Eridanus. Because of its far southern declination (-57°), it was unknown to ancient Greek and Roman astronomers, who instead placed the end of their river constellation at the star Acamar (Theta Eridani). Achernar was added to European star catalogs after the great southern voyages of exploration.
재미있는 사실
Achernar's extreme oblateness was directly measured by ESO's VLTI interferometer in 2003, confirming that it is the flattest star ever directly observed. If the Sun rotated as fast as Achernar, a day would last only about 5 hours. Achernar also has a close companion star (spectral type A) that orbits with a period of about 15 years.