Proxima Centauri
 Citra Proxima Centauri | |
| Data pengamatan Epos J2000.0 Ekuinoks J2000.0 (ICRS) | |
|---|---|
| Rasi bintang | Centaurus |
| Asensio rekta | 14j 29m 42.9487d[1] |
| Deklinasi | −62° 40′ 46.141″[1] |
| Magnitudo tampak (V) | 11,05[1] |
| Ciri-ciri | |
| Kelas spektrum | M5.5 Ve[1] |
| Indeks warna U−B | 1,43[1] |
| Indeks warna B−V | 1,90[1] |
| Jenis variabel | Bintang suar |
| Astrometri | |
| Kecepatan radial (Rv) | −21,7 ± 1,8[2] km/s |
| Gerak diri (μ) | RA: −3775,40[1] mdb/thn Dek.: 769,33[1] mdb/thn |
| Paralaks (π) | 768.7±0.3[3] mdb |
| Jarak | Mal:ErrorBar2 tc (Mal:ErrorBar2 pc) |
| Magnitudo mutlak (MV) | 15,49[4] |
| Detail | |
| Massa | 0,123 ± 0,006[5] M☉ |
| Radius | 0,145 ± 0,011[5] R☉ |
| Luminositas (bolometrik) | 0,0017[6] L☉ |
| Gravitasi permukaan (log g) | 5,20 ± 0,23[5] |
| Suhu | 3,042 ± 117[5] K |
| Rotasi | 83,5 hari[7] |
| Usia | 4,85Mal:Esp[8] tahun |
| Penamaan lain | |
| Referensi basis data | |
| SIMBAD | data |
Proxima Centauri[9] inggih punika bintang alit mamassa éndép sané magenah 4.2465 warsa cahaya (1.3020 pc) dohné saking Surya ring rasi bintang kelod saking Centaurus. Aran Latiné maartos '[bintang] pinih nampek saking Centaurus'. Ipun kacunduk duk warsa 1915 olih Robert Innes saha pinaka bintang pinih nampek sané kauningin sareng Surya. Antuk magnitudo semu mendem agengné 11,13, ipun bes redup antuk kacingak nganggén panyingakan malalung. Proxima Centauri inggih punika anggota Alpha Centauri sistem bintang, sané kaidentifikasi dados komponén Alpha Centauri C, lan magenah 2,18° kelod kauh pasangan Alpha Centauri AB. Sané mangkin magenah 12,950 AU (0.2 ly) saking AB, sané mangorbitné sareng period sawatara 550.000 warsa.
- ↑ 1,0 1,1 1,2 1,3 1,4 1,5 1,6 1,7 1,8 "SIMBAD query result: V* V645 Cen -- Flare Star". Centre de Données astronomiques de Strasbourg. Kaaksés 2008-08-11.—some of the data is located under "Measurements".
- ↑ García-Sánchez, J. (2001). "Stellar encounters with the solar system". Astronomy and Astrophysics. 379: 634–659. doi:10.1051/0004-6361:20011330. Kaaksés 2008-06-12. Unknown parameter
|coauthors=ignored (|author=suggested) (help) - ↑ Pikobet nganggit: Tag
<ref>tidak sah; tidak ditemukan teks untuk ref bernamaapj118 - ↑ Kamper, K. W. (1978). "Alpha and Proxima Centauri". Astronomical Journal. 83: 1653–1659. doi:10.1086/112378. Kaaksés 2008-08-03. Unknown parameter
|coauthors=ignored (|author=suggested) (help) - ↑ 5,0 5,1 5,2 5,3 Ségransan, D. (2003). "First radius measurements of very low mass stars with the VLTI". Astronomy and Astrophysics. 397: L5–L8. doi:10.1051/0004-6361:20021714. Kaaksés 2008-08-07. Unknown parameter
|coauthors=ignored (|author=suggested) (help) - ↑ See Table 1, Doyle, J. G. (1990). "Optical and infrared photometry of dwarf M and K stars". Astronomy and Astrophysics. 235: 335–339. Bibcode:1990A&A...235..335D. Unknown parameter
|coauthors=ignored (|author=suggested) (help) dan hal. 57, Peebles, P. J. E. (1993). Principles of Physical Cosmology. Princeton, New Jersey: Princeton University Press. ISBN 0691019339. - ↑ Benedict, G. Fritz; et al. (1998). "Photometry of Proxima Centauri and Barnard's Star Using Hubble Space Telescope Fine Guidance Sensor 3: A Search for Periodic Variations". The Astronomical Journal. 116 (1): 429–439. doi:10.1086/300420. Kaaksés 2007-07-09. Explicit use of et al. in:
|author=(help) - ↑ Kervella, Pierre; Thevenin, Frederic (2003-03-15). "A Family Portrait of the Alpha Centauri System: VLT Interferometer Studies the Nearest Stars". ESO. Kaarsipin saking versi asli tanggal 2008-06-16. Kaaksés 2007-07-09. Unknown parameter
|dead-url=ignored (help)CS1 maint: multiple names: authors list (link) - ↑ "Latin Resources". Joint Association of Classical Teachers. Kaarsipin saking versi asli tanggal 2007-07-08. Kaaksés 2007-07-15. Unknown parameter
|dead-url=ignored (help)
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Wikimédia Commons madué média indik Proxima Centauri. |
- (Inggris) Keterangan bintang yang terdekat dengan Bumi Archived 2005-09-24 at the Wayback Machine
- (Inggris) Galeri foto Proxima Centauri
- (Inggris) Sistem Alpha Centauri