Templat:Matoari
 Diproyeksikan dalam cahayo tampak dangan filter surya pado taun 2013 dangan bintiak matoari dan panggolokan topi | |
 Gamba bawarno semu nan diambiak pado taun 2010 nan diproyeksikan dek sinar ultraungu (panjang galombang 30,4 nm) | |
| Namo | Matoari, Matahari, Surya,[1] Mentari,[2] Syamsu,[3] Syamsi,[4] Rawi,[5] Sun, Sol,[6] Helios[7] |
|---|---|
| Kato sifat | Solar,[8][9] Surya |
| Data pengamatan | |
| Jarak rato-rato dari Bumi | 1 AU ≈ 1,496×108 km[10] 8 min 19 s (laju cahaya) |
| Kacarahan visual (V) | −26,74[11] |
| Magnitudo mutlak | 4,83[11] |
| Klasifikasi spektrum | G2V[12] |
| Kalogaman | Z = 0,0122[13] |
| Diameter suduik | 31,6–32,7 menit busur[14] |
| Ciri-ciri orbit | |
| Jarak rato-rato dari pusek Bima Sakti | ≈ 2,7×1017 km 27.200 tahun cahaya |
| Pariode galaksi | (2,25–2,50)×108 a |
| Kacapatan | ≈ 220 km/s (orbit mangitari pusek Bima Sakti) ≈ 20 km/s (relatif tahadok kacapatan rato-rato bintang lain dalam kalompok bintang) ≈ 370 km/s[15] (relatif tahadok latar balakang galombang mikrokosmis) |
| Ciri-ciri fisik | |
| Jari-jari khatulistiwa | 695.700 km[16] 696.342 km[17] 109 × Bumi[18] |
| Kaliliang khatulistiwa | 4,379×106 km[18] 109 × Bumi[18] |
| Kepepatan | 9×10−6 |
| Laweh parmukoan | 6,09×1012 km2[18] 12.000 × Bumi[18] |
| Volume | 1,41×1018 km3[18] 1.300.000 × Bumi |
| Massa | 1,9891×1030 kg[11] 333.000 × Bumi[11] |
| Kapadekan rato-rato | 1,408×103 kg/m3[11][18][19] 1,408 g/cm3[11][18][20] 0,255 × Bumi[11][18] |
| Kapadekan | pusek (permodelan) 1,622×105 kg/m3[11] 162,2 g/cm3[11] 12,4 × Bumi fotosfer 2×10−4 kg/m3 kromosfer 5×10−6 kg/m3 korona (rata-rata) 1×10−12 kg/m3[21] |
| Gravitasi parmukoan khatulistiwa | 274 m/s2[11] 28 × Bumi[18] |
| Faktor momen inersia | 0,070[11] (parkiroan) |
| Kacapatan lapeh (dari parmukoan) | 617,7 km/s[18] 55 × Bumi[18] |
| Suhu | pusek (permodelan) 1,57×107 K[11] fotosfer (efektif) 5772 K[11] korona ≈ 5×106 K |
| Luminositas (Lsol) | 3,828×1026 W[11] ≈ 3,75×1028 lm ≈ 98 lm/W efikasi |
| Warno (B-V) | 0,63 |
| Radians rato-rato (Isol) | 2,009×107 W·m−2·sr−1 |
| Umua | ≈ 4,6 miliar tahun[22][23] |
| Ciri-ciri rotasi | |
| Kamiringan sumbu | 7,25°[11] (tahadok ekliptika) 67,23° (tahadok bidang galaksi) |
| Asensio rekta pado kutub utara[24] | 286,13° 19 jam 4 menit 30 detik |
| Deklinasi pado kutub utaro | +63,87° 63° 52' LU |
| Pariode rotasi sideris | tahadok khatulistiwa 25,05 hari[11] tahadok lintang 16° 25,38 hari[11] 25 hari 9 jam 7 menit 12 detik[24] tahadok kutub 34,4 hari[11] |
| Kacapatan rotasi (tahadok khatulistiwa) | 7,189×103 km/h[18] |
| Komposisi fotosfer (manuruik massa) | |
| Hidrogen | 73,46%[25] |
| Helium | 24,85% |
| Oksigen | 0,77% |
| Karbon | 0,29% |
| Basi | 0,16% |
| Neon | 0,12% |
| Nitrogen | 0,09% |
| Silikon | 0,07% |
| Magnesium | 0,05% |
| Balerang | 0,04% |
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Templat:Daftar referensi templat
- ↑ Surya — KBBI Daring
- ↑ Mentari — KBBI Daring
- ↑ Syamsu — KBBI Daring
- ↑ Syamsi — KBBI Daring
- ↑ Rawi — KBBI Daring
- ↑ "Sol". Oxford English Dictionary (edisi ke-3rd). Oxford University Press. September 2005. (Subscription or UK public library membership required.) "Sol". Oxford English Dictionary (edisi ke-3rd). Oxford University Press. September 2005. (Subscription or UK public library membership required.)
- ↑ Templat:Lexico
- ↑ "solar". Oxford English Dictionary (edisi ke-3rd). Oxford University Press. September 2005. (Subscription or UK public library membership required.) "solar". Oxford English Dictionary (edisi ke-3rd). Oxford University Press. September 2005. (Subscription or UK public library membership required.)
- ↑ Solar2 — KBBI Daring
- ↑ Pitjeva, E. V.; Standish, E. M. (2009). "Proposals for the masses of the three largest asteroids, the Moon–Earth mass ratio and the Astronomical Unit". Celestial Mechanics and Dynamical Astronomy (dalam bahasa Inggris). 103 (4): 365–372. Bibcode:2009CeMDA.103..365P. doi:10.1007/s10569-009-9203-8. ISSN 1572-9478.
- ↑ a b c d e f g h i j k l m n o p q r Williams, D.R. (1 Juli 2013). "Sun Fact Sheet". NASA Goddard Space Flight Center. Diarsipkan dari versi asli tanggal 15 Juli 2010. Diakses tanggal 12 Agustus 2013.
- ↑ Zombeck, Martin V. (1990). Handbook of Space Astronomy and Astrophysics 2nd edition. Cambridge University Press. http://ads.harvard.edu/books/hsaa/.
- ↑ Asplund, M.; Grevesse, N.; Sauval, A.J. (2006). "The new solar abundances – Part I: the observations" (PDF). Communications in Asteroseismology. 147: 76–79. Bibcode:2006CoAst.147...76A. doi:10.1553/cia147s76.
- ↑ "Eclipse 99: Frequently Asked Questions". NASA. Diarsipkan dari versi asli tanggal 27 Mei 2010. Diakses tanggal 24 Oktober 2010.
- ↑ Hinshaw, G.; et al. (2009). "Five-year Wilkinson Microwave Anisotropy Probe observations: data processing, sky maps, and basic results". The Astrophysical Journal Supplement Series. 180 (2): 225–245. arXiv:0803.0732
. Bibcode:2009ApJS..180..225H. doi:10.1088/0067-0049/180/2/225.
- ↑ Templat:Cite arxiv
- ↑ Emilio, Marcelo; Kuhn, Jeff R.; Bush, Rock I.; Scholl, Isabelle F. (2012), "Measuring the Solar Radius from Space during the 2003 and 2006 Mercury Transits", The Astrophysical Journal, 750 (2): 135, arXiv:1203.4898 , Bibcode:2012ApJ...750..135E, doi:10.1088/0004-637X/750/2/135
- ↑ a b c d e f g h i j k l m "Solar System Exploration: Planets: Sun: Facts & Figures". NASA. Diarsipkan dari versi asli tanggal 2 Januari 2008.
- ↑ Ko, M. (1999). Elert, G., ed. "Density of the Sun". The Physics Factbook.
- ↑ Ko, M. (1999). Elert, G., ed. "Density of the Sun". The Physics Factbook.
- ↑ "Principles of Spectroscopy". Universitas Michigan, Astronomy Department. 30 Agustus 2007.
- ↑ Bonanno, A.; Schlattl, H.; Paternò, L. (2002). "The age of the Sun and the relativistic corrections in the EOS". Astronomy and Astrophysics. 390 (3): 1115–1118. arXiv:astro-ph/0204331 . Bibcode:2002A&A...390.1115B. doi:10.1051/0004-6361:20020749.
- ↑ Connelly, JN; Bizzarro, M; Krot, AN; Nordlund, Å; Wielandt, D; Ivanova, MA (2 November 2012). "The Absolute Chronology and Thermal Processing of Solids in the Solar Protoplanetary Disk". Science. 338 (6107): 651–655. Bibcode:2012Sci...338..651C. doi:10.1126/science.1226919. PMID 23118187. Templat:Registration required
- ↑ a b Seidelmann, P.K.; et al. (2000). "Report Of The IAU/IAG Working Group On Cartographic Coordinates And Rotational Elements Of The Planets And Satellites: 2000". Diakses tanggal 22 Maret 2006.
- ↑ "The Sun's Vital Statistics". Stanford Solar Center. Diakses tanggal 29 Juli 2008. Citing Eddy, J. (1979). A New Sun: The Solar Results From Skylab. NASA. p. 37. NASA SP-402. https://history.nasa.gov/SP-402/contents.htm.
