Gliese 445
Gambar dari of AC +79 3888 (dibulatkan), juga dikenal dengan Gliese 445, terletak 17.1 tahun cahaya dari Bumi
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Data pengamatan Epos J2000.0 Ekuinoks J2000.0 (ICRS)
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Rasi bintang
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Camelopardalis
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Asensio rekta
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11j 47m 41.3885d[1]
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Deklinasi
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+78° 41′ 28.179″[1]
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Magnitudo tampak (V)
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10.80[2]
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Ciri-ciri
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Kelas spektrum
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M4.0Ve[3]
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Indeks warna B−V
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1.572[2]
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Astrometri |
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Kecepatan radial (Rv) | −111.707[1] km/s |
Gerak diri (μ) | RA: 748.111[1] mdb/thn Dek.: 480.804[1] mdb/thn |
Paralaks (π) | 190,3251±0,0194[4] mdb |
Jarak | 17,137 ± 0,002 tc (5,2542 ± 0,0005 pc) |
Magnitudo mutlak (MV) | 12.227[5] |
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Detail |
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Massa | 0.14[6] M☉ |
Radius | 0.285[5] R☉ |
Luminositas | 0.008[7] L☉ |
Gravitasi permukaan (log g) | 4.72[7] |
Suhu | 3,507[1] K |
Metalisitas [Fe/H] | −0,30[5] |
Kecepatan rotasi (v sin i) | <2.5[8] km/s |
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Penamaan lain |
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Referensi basis data |
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SIMBAD | data |
ARICNS | data |
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Gliese 445 (Gl 445 atau AC +79 3888) adalah sebuah bintang deret utama Tipe M yang terletak pada bagian utara dari konstelasi Camelopardalis.
- ^ a b c d e f Brown, A. G. A.; et al. (kolaborasi Gaia) (Agustus 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365
. Bibcode:2018A&A...616A...1G
. doi:10.1051/0004-6361/201833051
. Catatan Gaia DR2 untuk sumber tersebut di VizieR.
- ^ a b Urban, S. E.; Zacharias, N.; Wycoff, Observatory G. L. U. S. Naval; Washington, 2004-2006 D. C. (2004). "VizieR Online Data Catalog: The UCAC2 Bright Star Supplement (Urban+, 2006)". VizieR On-line Data Catalog. Bibcode:2004yCat.1294....0U.
- ^ Lépine, Sébastien; Hilton, Eric J.; Mann, Andrew W.; Wilde, Matthew; Rojas-Ayala, Bárbara; Cruz, Kelle L.; Gaidos, Eric (2013). "A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky". The Astronomical Journal. 145 (4): 102. arXiv:1206.5991
. Bibcode:2013AJ....145..102L. doi:10.1088/0004-6256/145/4/102.
- ^ Templat:Cite Gaia EDR3
- ^ a b c Houdebine, Éric R.; Mullan, D. J.; Doyle, J. G.; de la Vieuville, Geoffroy; Butler, C. J.; Paletou, F. (2019). "The Mass-Activity Relationships in M and K Dwarfs. I. Stellar Parameters of Our Sample of M and K Dwarfs". The Astronomical Journal. 158 (2): 56. arXiv:1905.07921
. Bibcode:2019AJ....158...56H. doi:10.3847/1538-3881/ab23fe
.
- ^ Gaidos, E.; Mann, A. W.; Lépine, S.; Buccino, A.; James, D.; Ansdell, M.; Petrucci, R.; Mauas, P.; Hilton, E. J. (2014). "Trumpeting M dwarfs with CONCH-SHELL: A catalogue of nearby cool host-stars for habitable exoplanets and life". Monthly Notices of the Royal Astronomical Society. 443 (3): 2561. arXiv:1406.7353
. Bibcode:2014MNRAS.443.2561G. doi:10.1093/mnras/stu1313.
- ^ a b McDonald, I.; Zijlstra, A. A.; Watson, R. A. (2017). "Fundamental parameters and infrared excesses of Tycho-Gaia stars". Monthly Notices of the Royal Astronomical Society. 471 (1): 770. arXiv:1706.02208
. Bibcode:2017MNRAS.471..770M. doi:10.1093/mnras/stx1433.
- ^ Stelzer, B.; Marino, A.; Micela, G.; López-Santiago, J.; Liefke, C. (2013). "The UV and X-ray activity of the M dwarfs within 10 pc of the Sun". Monthly Notices of the Royal Astronomical Society. 431 (3): 2063. arXiv:1302.1061
. Bibcode:2013MNRAS.431.2063S. doi:10.1093/mnras/stt225.
- ^ "GJ 445". SIMBAD. Centre de données astronomiques de Strasbourg.