格利泽526 (Lalande 25372 , Wolf 498 )是一顆位於牧夫座 的紅矮星 。它的視星等 為 8.5[ 2] ,因此無法用肉眼看到。該系統距離地球17.7光年(5.43秒差距)。[ 10]
特性
格利泽526是一顆耀星 ,這意味著它的亮度偶爾會增加1-6個星等。[ 5] 它是一顆位於主序星階段的紅矮星,恆星分類為M1.5V。[ 3] 格利泽526比太陽小,質量為太陽的28%[ 5] ,半徑為太陽的58.2%。[ 2] 它的光度僅為太陽的1.1%[ 7] 。其恆星溫度為3,474K[ 2] 。
格利泽526已經過紅外輻射檢查。如果紅外線存在過量可以被視為碎片盤圍繞恆星運行的跡象。然而,在格利泽526周圍並沒有發現這樣的超量[ 7] 。
參考資料
^ 1.0 1.1 1.2 Brown, A. G. A.; et al. Gaia Early Data Release 3: Summary of the contents and survey properties. Astronomy & Astrophysics . 2021, 649 : A1. Bibcode:2021A&A...649A...1G . S2CID 227254300 . arXiv:2012.01533 . doi:10.1051/0004-6361/202039657 . (勘误: doi :10.1051/0004-6361/202039657e ) . Gaia EDR3 record for this source at VizieR .
^ 2.0 2.1 2.2 2.3 2.4 2.5 2.6 2.7 Houdebine, E. R., Observation and modelling of main-sequence star chromospheres - XVI. Rotation of dK5 stars, Monthly Notices of the Royal Astronomical Society , September 2011, 407 (3): 1657–1673, Bibcode:2011MNRAS.416.2233H , doi:10.1111/j.1365-2966.2011.19199.x .
^ 3.0 3.1 3.2 Frasca, A.; et al, REM near-IR and optical photometric monitoring of pre-main sequence stars in Orion. Rotation periods and starspot parameters, Astronomy and Astrophysics, December 2009, 508 (3): 1313–1330, Bibcode:2009A&A...508.1313F , S2CID 118361131 , arXiv:0911.0760 , doi:10.1051/0004-6361/200913327 .
^ 4.0 4.1 Cowley, A. P.; Hiltner, W. A.; Witt, A. N., Spectral classification and photometry of high proper motion stars, Astronomical Journal , December 1967, 72 : 1334–1340, Bibcode:1967AJ.....72.1334C , doi:10.1086/110413 .
^ 5.0 5.1 5.2 5.3 Gershberg, R. E.; et al, Catalogue and bibliography of the UV Cet-type flare stars and related objects in the solar vicinity, Astronomy and Astrophysics Supplement, November 1999, 139 (3): 555–558, Bibcode:1999A&AS..139..555G , doi:10.1051/aas:1999407 .
^ Evans, D. S., The Revision of the General Catalogue of Radial Velocities, Batten, Alan Henry; Heard, John Frederick (编), Determination of Radial Velocities and their Applications, Proceedings from IAU Symposium no. 30 30 , University of Toronto: International Astronomical Union : 57, June 20–24, 1966, Bibcode:1967IAUS...30...57E .
^ 7.0 7.1 7.2 Avenhaus, H.; et al, The nearby population of M-dwarfs with WISE: a search for warm circumstellar dust, Astronomy & Astrophysics, December 2012, 548 : A105, Bibcode:2012A&A...548A.105A , S2CID 56397054 , arXiv:1209.0678 , doi:10.1051/0004-6361/201219783 .
^ Suárez Mascareño, A.; et al, Rotation periods of late-type dwarf stars from time series high-resolution spectroscopy of chromospheric indicators, Monthly Notices of the Royal Astronomical Society, September 2015, 452 (3): 2745–2756, Bibcode:2015MNRAS.452.2745S , S2CID 119181646 , arXiv:1506.08039 , doi:10.1093/mnras/stv1441 .
^ HD 119850 . SIMBAD . 斯特拉斯堡天文資料中心 .
^ Gatewood, George. Astrometric Studies of Aldebaran, Arcturus, Vega, the Hyades, and Other Regions . The Astronomical Journal . 2008, 136 (1): 452–460. Bibcode:2008AJ....136..452G . doi:10.1088/0004-6256/136/1/452 .
註釋
左栏标出的是恒星系统中主要恒星的恒星类型。‡若考虑距离误差容限,恒星系统有可能在此范围外。 粗体字 突出的恒星系统为拥有至少一颗绝对星等 在+8.5或以上的恒星的系统。斜体字 突出的是有可能在此范围之外的恒星系统。