Mata panas
Gamal
The Sun, filmed through a clear solar filter | |
| Names | Sun, Sol,[1] Sól, Helios[2] |
|---|---|
| Adjectives | Solar[3] |
| Symbol | |
| Observation data | |
| Mean distance from Earth | 1 AU 149,600,000 km 8 min 19 s, light speed[4] |
| −26.74 (V)[5] | |
| 4.83[5] | |
| G2V[6] | |
| Metallicity | Z = 0.0122[7] |
| Angular size | 0.527–0.545°[8] |
| Orbital characteristics | |
Mean distance from Milky Way core | 24,000 to 28,000 light-years[9] |
| Galactic period | 225–250 million years |
| Velocity |
|
| Obliquity |
|
Right ascension North pole | 286.13° (286° 7′ 48″)[5] |
Declination of North pole | +63.87° (63° 52′ 12"N)[5] |
Sidereal rotation period |
|
Equatorial rotation velocity | 1.997 km/s[11] |
| Physical characteristics | |
Equatorial radius | 6.957 x 108 m[12] 109 × Earth radii[11] |
| Flattening | 0.00005[5] |
| Surface area | 6.09×1012 km2 12,000 × Earth[11] |
| Volume |
|
| Mass | |
| Average density | 1.408 g/cm3 0.255 × Earth[5][11] |
| Age | 4.6 billion years[13][14] |
Equatorial surface gravity | 274 m/s2[5] 27.9 g0[11] |
| ≈0.070[5] | |
Surface escape velocity | 617.7 km/s 55 × Earth[11] |
| Temperature |
|
| Luminosity | |
| Color (B-V) | 0.656[15] |
| Mean radiance | 2.009×107 W·m−2·sr−1 |
Photosphere composition by mass | |
Mata panas nya siti bintang ba tengah Sistem Solar. Iya nya sfera plasma angat ti besai sereta nyau deka sempurna, dipanas nyentukka nyadi pijar nengah reaksyen fusi nuklear dalam teras iya, mansutka tenaga ari permukaan iya tebal agi nyadi penampak ti tampak enggau radiasyen inframerah enggau 10% ba tenaga ultraviolet. Iya jauh nyadi pun penatai kuasa ti pemadu beguna ngagai pengidup ba Bumi. Mata panas udah nyadi objek ti dipebasaka dalam mayuh budaya. Iya udah nyadi subjek tengah ungkup pansik astronomi kenyau ari jeman kelia.
Penerang
[edit | edit bunsu]- ↑ Penyalat nyebut: Tag
<ref>tidak sah; tiada teks disediakan bagi rujukan yang bernamaOED - ↑ Penyalat nyebut: Tag
<ref>tidak sah; tiada teks disediakan bagi rujukan yang bernamaLexico - ↑ Penyalat nyebut: Tag
<ref>tidak sah; tiada teks disediakan bagi rujukan yang bernamaOED2 - ↑ 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 (in Inggeris). 103 (4): 365–372. Bibcode:2009CeMDA.103..365P. doi:10.1007/s10569-009-9203-8. ISSN 1572-9478. S2CID 121374703. Archived from the original on 9 July 2019. Retrieved 13 July 2019.
- ↑ 5.00 5.01 5.02 5.03 5.04 5.05 5.06 5.07 5.08 5.09 5.10 5.11 5.12 5.13 Williams, D. R. (1 July 2013). "Sun Fact Sheet". NASA Goddard Space Flight Center. Archived from the original on 15 July 2010. Retrieved 12 August 2013.
- ↑ Zombeck, Martin V. (1990). Handbook of Space Astronomy and Astrophysics 2nd edition. Cambridge University Press. Archived from the original on 3 February 2021. Retrieved 13 January 2016.
- ↑ Asplund, M.; Grevesse, N.; Sauval, A. J. (2006). "The new solar abundances – Part I: the observations". Communications in Asteroseismology. 147: 76–79. Bibcode:2006CoAst.147...76A. doi:10.1553/cia147s76. ISSN 1021-2043. S2CID 123824232.
- ↑ "Eclipse 99: Frequently Asked Questions". NASA. Archived from the original on 27 May 2010. Retrieved 24 October 2010.
- ↑ Francis, Charles; Anderson, Erik (June 2014). "Two estimates of the distance to the Galactic Centre". Monthly Notices of the Royal Astronomical Society. 441 (2): 1105–1114. arXiv:1309.2629. Bibcode:2014MNRAS.441.1105F. doi:10.1093/mnras/stu631. S2CID 119235554.
- ↑ Hinshaw, G.; Weiland, J. L.; Hill, R. S.; Odegard, N.; Larson, D.; 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. S2CID 3629998.
- ↑ 11.0 11.1 11.2 11.3 11.4 11.5 "Solar System Exploration: Planets: Sun: Facts & Figures". NASA. Archived from the original on 2 January 2008.
- ↑ 12.0 12.1 Prša, Andrej; Harmanec, Petr; Torres, Guillermo; et al. (2016-08-01). "NOMINAL VALUES FOR SELECTED SOLAR AND PLANETARY QUANTITIES: IAU 2015 RESOLUTION B3 * †". The Astronomical Journal. 152 (2): 41. arXiv:1510.07674. doi:10.3847/0004-6256/152/2/41. ISSN 0004-6256.
- ↑ 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. S2CID 119436299.
- ↑ Connelly, J. N.; Bizzarro, M.; Krot, A. N.; Nordlund, Å.; Wielandt, D.; Ivanova, M. A. (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. S2CID 21965292.Templat:Registration required
- ↑ Gray, David F. (November 1992). "The Inferred Color Index of the Sun". Publications of the Astronomical Society of the Pacific. 104 (681): 1035–1038. Bibcode:1992PASP..104.1035G. doi:10.1086/133086.
- ↑ "The Sun's Vital Statistics". Stanford Solar Center. Archived from the original on 14 October 2012. Retrieved 29 July 2008. Citing Eddy, J. (1979). A New Sun: The Solar Results From Skylab. NASA. p. 37. NASA SP-402. Archived from the original on 30 July 2021. Retrieved 12 July 2017.