Agena
HIP 68702; Beta Cen
물리적 특성
위치 & 식별자
가시성
사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.
다중 항성계
접안렌즈 시야
Sep: 0.2″ · PA: 142° · 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…
Agena 소개
설명
Agena (also known as Hadar) is the second brightest star in Centaurus and the 11th brightest in the night sky at magnitude 0.61. It is a giant star of spectral type B1III located about 390 light-years from Earth. Agena is actually a triple star system: the primary is a spectroscopic binary of two blue giant stars orbiting each other every 357 days, with a more distant third companion. The system's combined luminosity is about 41,000 times that of the Sun.
관측 팁
Agena is a Southern Hemisphere object, visible only from latitudes south of about 30°N. Together with Alpha Centauri, it forms the 'Southern Pointers' — the two bright stars that point toward the Southern Cross (Crux), a vital navigation aid in the southern sky. The two stars are about 4.5 degrees apart and make a striking pair. Best observed from March through September from southern latitudes.
역사
The name Hadar comes from the Arabic for 'ground' or 'soil,' possibly referring to its low position as seen from Arabian latitudes. The alternative name Agena is Latin, possibly meaning 'the knee.' Along with Alpha Centauri, it has been used by Polynesian and Aboriginal Australian navigators for centuries. Its spectroscopic binary nature was discovered in the early 20th century.
재미있는 사실
Despite being 100 times farther away than Alpha Centauri, Agena appears almost as bright because it is intrinsically far more luminous. The two stars serve as reliable pointers to the Southern Cross — a line drawn through them leads directly to Gacrux (Gamma Crucis) at the top of the Cross.