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Achernar

HIP 7588; Alpha Eri

HIP 7588; Alpha Eri DoubleStar Eri 관측 가능 난이도 5 Expert level - Requires steady seeing
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물리적 특성

등급 0.46
변광성 유형 Eclipsing Binary (Beta Lyrae-type)
분광형 B6Vep
항성 색상 파랑 (B-V -0.16)
온도 14988 K
반지름 9.3 R☉
거리 144.0 ly

위치 & 식별자

RA 01h 37m 42.9s
Dec -57° 14' 12.0"
별자리 Eri
HR 472
HIP 7588
Bayer Alpha
Variable ID Var

가시성

사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.

다중 항성계

이격 0.3″
동반성 등급 2.1
동반성 분광형 A2V
위치각 309°
항성 색상 A: 파랑 B: 흰색
발견자 KRV 54

접안렌즈 시야

80x Dawes: 1.9″ TFOV: 0.6°
실제 = 실제 각크기
N E 309° A (0.5) B (2.1)

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

HR 도표 로드 중…

흑체 복사 스펙트럼

항성 흡수 스펙트럼

스펙트럼 유형을 기반으로 한 시뮬레이션 흡수 스펙트럼. 선 위에 마우스를 올려 원소를 식별하세요.

항성 참고사항

EB or Ell, amp. 0.02V. H alpha var. emission and possible high-velocity mass loss. Expanding circumstellar shell.
Member of Pleiades group.
Lyman alpha and Lyman beta observed from COPERNICUS. H alpha and H beta var. emission and possible high-velocity mass | loss. Expanding circumstellar shell.
Period in RV and light (1.26d) seems best explained by rotation. Weak but significant variations in strength of | MgII 4481. RV of H gamma and HeI 4471 consistent with period, amp. 30k/s. Variable light amp. 0.02V.
ACHERNAR.
Diam. = 0.00185 - 0.00192".

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.