28 Bellona is a large main-belt asteroid. It was discovered by German astronomer R. Luther on March 1, 1854, and named after Bellōna, the Roman goddess of war; the name was chosen to mark the beginning of the Crimean War. Its historical symbol was Bellona's whip and spear; it is in the pipeline for Unicode 17.0 as U+1CECE ().[8][9]
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Discovery | |
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Discovered by | R. Luther |
Discovery date | 1 March 1854 |
Designations | |
(28) Bellona | |
Pronunciation | /bɛˈloʊnə/[2] |
Named after | Bellona |
1951 CC2 | |
Main belt | |
Adjectives | Bellonian /bɛˈloʊniən/[2] |
Symbol | ![]() |
Orbital characteristics | |
Epoch Sept 30, 2012 (JD 2456200.5) | |
Aphelion | 477.240 Gm (3.196 AU) |
Perihelion | 353.977 Gm (2.358 AU) |
415.608 Gm (2.777 AU) | |
Eccentricity | 0.151 |
1690.19 d (4.63 a) | |
121.574° | |
Inclination | 9.430° |
144.330° | |
344.461° | |
Physical characteristics | |
Dimensions | 97 ± 11 km[3] 120.9 ± 3.4 km (IRAS)[4] 108.10 ± 11.49 km[5] |
Mass | (2.62±0.15)×1018 kg[5] |
Mean density | 3.95 ± 1.28 g/cm3[5] |
15.706 h[4][6] | |
0.1763[4][7] | |
S [4] | |
7.09[4] | |
Bellona is a stony (S-type) asteroid with a cross-section size of around 100–120 km. 28 Bellona is orbiting the Sun with a period of 4.63 years.
Bellona has been studied by radar.[10] Photometric observations of this asteroid at the Palmer Divide Observatory in Colorado Springs, Colorado in 2007 gave a light curve with a period of 15.707 ± 0.002 hours and a brightness variation of 0.27 ± 0.03 in magnitude. This report is in close agreement with a period estimate of 15.695 hours reported in 1983, and rejects a longer period of 16.523 hours reported in 1979.[11]
References
edit- ^ "Astrometry.net job 1005148". Astrometry.net. Retrieved 6 February 2015.
- ^ a b "Bellona". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ Ďurech, Josef; Kaasalainen, Mikko; Herald, David; Dunham, David; Timerson, Brad; Hanuš, Josef; et al. (2011). "Combining asteroid models derived by lightcurve inversion with asteroidal occultation silhouettes" (PDF). Icarus. 214 (2): 652–670. arXiv:1104.4227. Bibcode:2011Icar..214..652D. doi:10.1016/j.icarus.2011.03.016. S2CID 119271216. Archived from the original (PDF) on 3 March 2016. Retrieved 26 January 2012.
- ^ a b c d e "JPL Small-Body Database Browser: 28 Bellona". Jet Propulsion Laboratory. Retrieved 28 January 2012.
2012-01-02 last obs
- ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009, S2CID 119226456. See Table 1.
- ^ "Archived copy". Archived from the original on 13 September 2006. Retrieved 12 August 2006.
{{cite web}}
: CS1 maint: archived copy as title (link) - ^ "Archived copy". Archived from the original on 22 July 2012. Retrieved 12 August 2006.
{{cite web}}
: CS1 maint: archived copy as title (link) - ^ Bala, Gavin Jared; Miller, Kirk (18 September 2023). "Unicode request for historical asteroid symbols" (PDF). unicode.org. Unicode. Retrieved 26 September 2023.
- ^ Unicode. "Proposed New Characters: The Pipeline". unicode.org. The Unicode Consortium. Retrieved 6 November 2023.
- ^ "Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. Retrieved 30 October 2011.
- ^ Warner, Brian D. (December 2007), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory - March-May 2007", The Minor Planet Bulletin, 34 (4): 104–107, Bibcode:2007MPBu...34..104W.
External links
edit- Lightcurve plot of 28 Bellona, Palmer Divide Observatory, B. D. Warner (2007)
- Asteroid Lightcurve Database (LCDB), query form (info Archived 16 December 2017 at the Wayback Machine)
- Dictionary of Minor Planet Names, Google books
- Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
- Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
- 28 Bellona at AstDyS-2, Asteroids—Dynamic Site
- 28 Bellona at the JPL Small-Body Database