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I don't have enough context to write an accurate 2-sentence overview. The provided information only mentions that Arcturus shows variable H and K emission, which is a technical detail insufficient for a general reader to understand what Arcturus is or why it matters.
AI-generated from the Wikipedia summary — may contain errors.
Wikidata facts
Show 21 more facts
- located in/on physical feature
- Local Interstellar Cloud
- Commons category
- Arcturus
- spectral class
- K0III
- catalog code
- UBV M 20076
- topic's main category
- Category:Arcturus
- color index
- 1.27
- apparent magnitude
- -2.911
- absolute magnitude
- -0.304
- parallax
- 0.12
- metallicity
- -0.52
- radial velocity
- -4.45165
- right ascension
- 213.915300295
- declination
- 19.182409162
- effective temperature
- 4291
- epoch
- J2000.0
- stellar rotational velocity
- 8
- surface gravity
- 20
- right ascension component of proper motion
- -1093
- luminosity
- 215
- declination component of proper motion
- -1998
- on focus list of Wikimedia project
- Wikipedia:Vital articles/Level/4
via Wikidata · CC0
Article · 中文
大角星(α Boo / 牧夫座α)英文名Arcturus(發音: /ɑːrkˈtjʊərəs/),是牧夫座中最明亮的恆星。以肉眼觀看大角星,它是橘黃色的,視星等-0.04,是全夜空第3亮的恆星,僅次於-1.46等的天狼星與-0.86等的老人星。雖然半人馬座的南門二(半人馬座α星)視星等是-0.27等,但它是由-0.01等的α1和+1.33等的α2組成的聯星,個別的亮度都低於大角星,只因為它們太過接近,所以肉眼無法分辨出來。因此,南門二雖然是相當明亮的恆星,但半人馬α1比大角星暗了一些,只是全天第4亮的恆星。大角星和南門二都位在本星際雲(Local Interstellar Cloud)中。 大角星雖然位於北半球,但距離天球赤道的緯度少於20度,因此在南北兩個半球都能看見。大角星大約在4月30日的子夜中天,因此在北半球的春天,南半球的秋天可以看見這顆恆星。北半球的觀察者可以沿著北斗星弧狀的柄來找到大角星。順著這個弧線繼續延伸,也可以觀測到角宿一。大角星與室女座角宿一、獅子座五帝座一共同組成春季大三角,如果再加上獵犬座的常陳一就成為春季大鑽石。
Abstract from DBpedia / Wikipedia · CC BY-SA
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