Spica
HIP 65474; Alpha Vir; 67 Vir
물리적 특성
위치 & 식별자
가시성
사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.
다중 항성계
접안렌즈 시야
Sep: 151.9″ · PA: 33° · 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
서베이 이미지 로드 중…
Spica 소개
설명
Spica is the brightest star in Virgo and the 15th brightest in the night sky at magnitude 0.98. It is a blue giant of spectral type B1III-IV, located about 250 light-years from Earth. Spica is actually a close spectroscopic binary: two hot stars orbiting each other every 4.01 days at a separation of only about 0.12 AU. The primary is about 10 times the mass of the Sun and 12,000 times more luminous. The two stars are so close that they are tidally distorted into egg shapes.
관측 팁
Spica is easy to find using the arc-to-Arcturus, spike-to-Spica mnemonic — follow the arc of the Big Dipper's handle through Arcturus and continue the curve to reach Spica. Its blue-white color contrasts sharply with the orange of nearby Arcturus. Spica is a useful reference star for the zodiac, as planets and the Moon frequently pass near it along the ecliptic. Best observed from March through July.
역사
The name Spica comes from the Latin 'Spica Virginis' meaning 'ear of grain,' as it represents the sheaf of wheat held by the constellation Virgo. Hipparchus used observations of Spica around 130 BC to discover the precession of the equinoxes — one of the most important discoveries in ancient astronomy. Nicolaus Copernicus also observed Spica to refine his understanding of precession.
재미있는 사실
The two stars of Spica are so close together that they are tidally distorted into ellipsoidal shapes, causing the system's brightness to vary by about 0.03 magnitudes as the elongated stars present different cross-sections to our line of sight. Spica is one of the 'pointer stars' for navigators and was critical to the discovery of precession over 2,000 years ago.