Shaula
HIP 85927; Lambda Sco; 35 Sco
물리적 특성
위치 & 식별자
가시성
사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.
다중 항성계
접안렌즈 시야
Sep: 42.4″ · PA: 106° · 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…
Shaula 소개
설명
Shaula (Lambda Scorpii) is a blue subgiant of spectral type B2IV, located about 570 light-years from Earth. At magnitude 1.63, it is the second brightest star in Scorpius (after Antares) and marks the tip of the Scorpion's tail, where the stinger would be. Shaula is actually a triple star system with a combined luminosity of about 36,000 times the Sun's. The primary is a Beta Cephei variable, pulsating with a period of about 4.7 hours.
관측 팁
Shaula forms a close pair with Lesath (Upsilon Scorpii, magnitude 2.7) — together they are sometimes called the 'Cat's Eyes' at the tip of the Scorpion's tail. This close pair is a pretty sight in binoculars. The open clusters M6 (Butterfly Cluster) and M7 (Ptolemy's Cluster) lie just a few degrees to the north, making this region rich territory for binocular sweeping. Shaula is best observed from May through August from locations with a good southern horizon.
역사
The name Shaula comes from the Arabic 'al-Shawla' meaning 'the raised tail,' describing its position at the tip of the scorpion's tail. The Shaula-Lesath pair was noted by many ancient cultures. In Polynesian navigation, these stars served as important waypoints for oceanic voyaging.
재미있는 사실
Shaula's close visual pairing with Lesath is a line-of-sight coincidence — the two stars are at very different distances (Lesath is about 580 light-years away, nearly the same as Shaula, but they are unrelated gravitationally). The pair's proximity earned them the nickname 'Cat's Eyes' from Australian observers.