Menu

Altair

HIP 97649; Alpha Aql; 53 Aql

HIP 97649; Alpha Aql; 53 Aql DoubleStar Aql 관측 가능 난이도 3 Medium telescope (6-8") - Requires steady seeing
성도 목록에 추가 계획에 추가
카탈로그로 돌아가기

물리적 특성

등급 0.77
분광형 A7Vn
항성 색상 황백색 (B-V 0.22)
온도 7555 K
반지름 1.6 R☉
거리 17.1 ly

위치 & 식별자

RA 19h 50m 47.0s
Dec +08° 52' 06.0"
별자리 Aql
HR 7557
HIP 97649
Bayer Alpha
Flamsteed 53 Aql
Double Cat 13009

가시성

사용자 설정에서 관측지를 설정하세요 가시성 데이터를 확인할 수 있습니다.

다중 항성계

구성 항성 3
구성 ID AB
이격 195.8″
동반성 등급 9.8
위치각 286°
항성 색상 A: 황백색
발견자 STFB 10

접안렌즈 시야

32x Dawes: 1.9″ TFOV: 1.6°
실제 = 실제 각크기
N E 286° A (0.8) B (9.8)

Sep: 195.8″ · PA: 286° · 위=북, 왼쪽=동

분해됨 · 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

Component B optical.
ALTAIR; Atair.
Diam. = 0.00278 - 0.00298".

서베이 이미지

서베이 이미지 로드 중…

Altair 소개

설명

Altair is the brightest star in the constellation Aquila and the 12th brightest in the night sky at magnitude 0.77. It is a white main-sequence star of spectral type A7V, only 16.7 light-years from Earth. Altair rotates extremely rapidly — once every 8.9 hours — causing it to be noticeably oblate, with its equatorial diameter about 22% larger than its polar diameter. It is about 1.8 times the mass of the Sun and roughly 11 times more luminous.

관측 팁

Altair is one of the three vertices of the Summer Triangle, along with Vega and Deneb. It is flanked by two dimmer stars — Tarazed (Gamma Aquilae, magnitude 2.7) to the northwest and Alshain (Beta Aquilae, magnitude 3.7) to the southeast — creating a distinctive compact line. Altair is visible from virtually all inhabited latitudes. Best observed from June through November when the Summer Triangle dominates the evening sky.

역사

The name Altair comes from the Arabic 'al-Nasr al-Ta'ir' meaning 'the flying eagle.' In Chinese and Japanese mythology, Altair represents the Cowherd (Niulang/Hikoboshi), separated from the Weaver Girl (Vega) by the celestial river of the Milky Way, reunited once a year on the seventh day of the seventh month — celebrated as the Qixi/Tanabata festival. Altair's rapid rotation and oblateness were directly confirmed by interferometric imaging in 2007.

재미있는 사실

Altair was one of the first stars to have its surface directly imaged — in 2007, optical interferometry produced an image showing its oblate shape and gravity darkening at the equator. A day on Altair lasts only about 9 hours, compared to the Sun's 25-day rotation period. At Altair's equatorial rotation speed of about 286 km/s, it is spinning at a significant fraction of its breakup velocity.