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扶筐四

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(重定向自HD 175306
扶筐四(Omicron Draconis)
扶筐四的位置(紅圈)
觀測資料
曆元 J2000
星座 天龍座
星官 扶筐女宿
赤經 18h 51m 12.09530s[1]
赤緯 +59° 23′ 18.0627″[1]
視星等(V) 4.65[2]
特性
光谱分类G9III[3]
U−B 色指数+1.19[2]
变星类型RS CVn + 食變星[4]
天体测定
徑向速度 (Rv)−19.52[5] km/s
自行 (μ) 赤经:77.47[1] mas/yr
赤纬:25.37[1] mas/yr
视差 (π)9.54 ± 0.21[1] mas
距离106.8[4] pc
绝对星等 (MV)−0.344[6]
軌道[4]
繞行週期 (P)138.444 ± 0.003 days
半長軸 (a)0.00651 ± 0.00003"
偏心率 (e)0.158 ± 0.003
倾斜角 (i)89.6 ± 0.3°
升交点黃經 (Ω)22.9 ± 0.2°
近心点 曆元 (T)2454983.0 ± 0.2
近心點幅角 (ω)
(secondary)
293.0 ± 0.6°
半振幅 (K1)
(primary)
23.42 ± 0.05 km/s
半振幅 (K2)
(secondary)
32.0 ± 0.4 km/s
詳細資料
ο Dra A
質量1.35[4] M
半徑25.1[4] R
表面重力 (log g)1.769[4]
亮度220[4] L
溫度4400[7] K
金属量 [Fe/H]−0.5[3] dex
自轉79[4]
自轉速度 (v sin i)20.0[6] km/s
年齡3.0[4] Gyr
ο Dra B
質量0.99[4] M
半徑1.0[4] R
表面重力 (log g)4.43[4]
亮度1.3[4] L
溫度6,000[4] K
其他命名
Omicron Draconis、47 Draconis、HR 7125、, HD 175306、HIP 92512、BD+59°1925
參考資料庫
SIMBAD资料

扶筐四Omicron Draconis,拉丁化為ο Draconis,縮寫為ο Dra)是星座天龍座的一顆巨星,距地球322.93光年。在北緯31o以北的地區,它是一顆拱極星,這意味著這顆恆星在夜空中永遠不會升起或落下。

扶筐四的 可見光波段光變曲線。改編自 羅滕巴赫(英語:Roettenbacher)等人(2015)[4]

這是一個單線光譜聯星系統[7],但已使用干涉測量術檢測到伴星。它是帶有食的獵犬座RS型變星系統,變化的總幅度只有百分之幾星等[8][4]。伴星與太陽相似,大概是一顆主序星,而主星是一顆比太陽大25倍,亮度高出200倍的巨星

極星的身份

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扶筐四是距離水星北天極最近的恆星,因此可以認為是水星的極星[9]。除此之外,這顆恆星每18.6年會成為月球的北極星一次[10]。這是因為月球自轉軸的進動,使其極星的狀態定期變化。

參考文獻

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  1. ^ 1.0 1.1 1.2 1.3 1.4 Van Leeuwen, F. Validation of the new Hipparcos reduction. Astronomy and Astrophysics. 2007, 474 (2): 653–664. Bibcode:2007A&A...474..653V. S2CID 18759600. arXiv:0708.1752可免费查阅. doi:10.1051/0004-6361:20078357. 
  2. ^ 2.0 2.1 Hoffleit, Dorrit; Jaschek, Carlos. The Bright star catalogue. New Haven. 1991. Bibcode:1991bsc..book.....H. 
  3. ^ 3.0 3.1 Keenan, Philip C.; McNeil, Raymond C. The Perkins catalog of revised MK types for the cooler stars. Astrophysical Journal Supplement Series. 1989, 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373. 
  4. ^ 4.00 4.01 4.02 4.03 4.04 4.05 4.06 4.07 4.08 4.09 4.10 4.11 4.12 4.13 4.14 4.15 Roettenbacher, Rachael M.; Monnier, John D.; Fekel, Francis C.; Henry, Gregory W.; Korhonen, Heidi; Latham, David W.; Muterspaugh, Matthew W.; Williamson, Michael H.; Baron, Fabien; Ten Brummelaar, Theo A.; Che, Xiao; Harmon, Robert O.; Schaefer, Gail H.; Scott, Nicholas J.; Sturmann, Judit; Sturmann, Laszlo; Turner, Nils H. Detecting the Companions and Ellipsoidal Variations of RS CVn Primaries. II. O Draconis, a Candidate for Recent Low-mass Companion Ingestion. The Astrophysical Journal. 2015, 809 (2): 159. Bibcode:2015ApJ...809..159R. S2CID 119228345. arXiv:1507.03601可免费查阅. doi:10.1088/0004-637X/809/2/159. 
  5. ^ Karataș, Yüksel; Bilir, Selçuk; Eker, Zeki; Demircan, Osman; Liebert, James; Hawley, Suzanne L.; Fraser, Oliver J.; Covey, Kevin R.; Lowrance, Patrick; Kirkpatrick, J. Davy; Burgasser, Adam J. Kinematics of chromospherically active binaries and evidence of an orbital period decrease in binary evolution. Monthly Notices of the Royal Astronomical Society. 2004, 349 (3): 1069–1092. Bibcode:2004MNRAS.349.1069K. S2CID 15290475. arXiv:astro-ph/0404219可免费查阅. doi:10.1111/j.1365-2966.2004.07588.x可免费查阅. 
  6. ^ 6.0 6.1 Böhm-Vitense, Erika; et al. Ultraviolet Emission Lines in BA and Non-BA Giants. The Astrophysical Journal. December 2000, 545 (2): 992–999. Bibcode:2000ApJ...545..992B. doi:10.1086/317850可免费查阅. 
  7. ^ 7.0 7.1 Pourbaix, D.; Boffin, H. M. J. Reprocessing the Hipparcos Intermediate Astrometric Data of spectroscopic binaries. II. Systems with a giant component. Astronomy and Astrophysics. February 2003, 398 (3): 1163–1177. Bibcode:2003A&A...398.1163P. S2CID 12361870. arXiv:astro-ph/0211483可免费查阅. doi:10.1051/0004-6361:20021736. 
  8. ^ omi Dra. The International Variable Star Index. AAVSO. [15 July 2022]. 
  9. ^ Sharrah, Paul C. Pole Stars of Other Planets (pdf). Arkansas Academy of Sciences Proceedings. 1975, XXIX: 62–63. 
  10. ^ Patrick Moore. The Guinness Book of Astronomy Facts & Feats. 1983: 29. In 1968 the north pole star of the Moon was Omega Draconis; by 1977 it was 36 Draconis. The south pole star is Delta Doradus.