28 Bellona

28 Bellona
A light curve model of 28 Bellona on the top and an image of 28 Bellona on the bottom.
Discovery
Discovered byRobert Luther
Discovery date1 March 1854
Designations
Pronunciation/bɛˈloʊnə/
Named after
Bellona
1951 CC2
Main belt
AdjectivesBellonian /bɛˈloʊniən/
Symbol𜻎 (historical)
Orbital characteristics
Epoch 21 November 2025 (JD 2461000.5)
Aphelion3.191 AU
Perihelion2.364 AU
2.777 AU
Eccentricity0.149
4.628 yr (1690.55 d)
65.459°
Inclination9.432°
144.151°
343.462°
Jupiter MOID1.872 AU
TJupiter3.299
Physical characteristics
Dimensions135 ± 7 km (ADAM)
Mass(2.62±0.15)×1018 kg (composite estimate)
(1.57±0.31)×1018 kg
Mean density
2.0 ± 0.3 g/cm3
1.22±0.31 g/cm3
15.70785 h
99° ± 4°
−16° ± 6°
0.1763
S
7.09

28 Bellona is a large asteroid located in the main-belt. It was discovered by German astronomer Robert Luther on 1 March 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 was encoded in Unicode 17.0 as U+1CECE 𜻎 ().

Bellona is a stony (S-type) asteroid with a cross-section size of around 135 km. 28 Bellona is orbiting the Sun with a period of 4.63 years.

Bellona has been studied by radar. 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.

A three-dimensional model of 28 Bellona based on its light curve

Notes

  1. ↑ Calculated from its standard gravitational parameter GM = 0.105±0.021 km3/s2.

References

  1. 1 2 "Bellona". Oxford English Dictionary (online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  2. 1 2 3 4 "JPL Small-Body Database Browser: 28 Bellona". Jet Propulsion Laboratory. Retrieved 22 January 2026. 2025-07-08 last obs
  3. 1 2 3 4 5 Viikinkoski, M.; Hanuš, J.; Kaasalainen, M.; Marchis, F.; Ďurech, J. (November 2017). "Adaptive optics and lightcurve data of asteroids: twenty shape models and information content analysis". Astronomy & Astrophysics. 607: A117. arXiv:1708.05191. Bibcode:2017A&A...607A.117V. doi:10.1051/0004-6361/201731456. ISSN 0004-6361. S2CID 67813915.
  4. ↑ 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.
  5. 1 2 Fuentes-Muñoz, Oscar; Farnocchia, Davide; Giorgini, Jon D.; Park, Ryan S. (1 December 2025). "Asteroid Mass Estimation by Mutual Perturbations During Close Encounters After Gaia Focused Product Release". The Astronomical Journal. 170 (6): 353. Bibcode:2025AJ....170..353F. doi:10.3847/1538-3881/ae0cc9. ISSN 0004-6256. S2CID 283347135.
  6. ↑ "Archived copy". Archived from the original on 22 July 2012. Retrieved 12 August 2006.{{cite web}}: CS1 maint: archived copy as title (link)
  7. ↑ Bala, Gavin Jared; Miller, Kirk (18 September 2023). "Unicode request for historical asteroid symbols" (PDF). unicode.org. Unicode. Retrieved 26 September 2023.
  8. ↑ "Miscellaneous Symbols Supplement" (PDF). unicode.org. The Unicode Consortium. 2025. Retrieved 9 September 2025.
  9. ↑ "Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. Retrieved 30 October 2011.
  10. ↑ 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.