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
(28) Bellona
Pronunciation/bɛˈlnə/[1]
Named after
Bellona
1951 CC2
Main belt
AdjectivesBellonian /bɛˈlniən/[1]
Symbol (historical)
Orbital characteristics[2]
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
Dimensions97 ± 11 km[3]
120.9 ± 3.4 km (IRAS)[2]
108.10 ± 11.49 km[4]
Mass(2.62±0.15)×1018 kg[4]
Mean density
3.95 ± 1.28 g/cm3[4]
15.706 h[2][5]
0.1763[2][6]
S[2]
7.09[2]

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 𜻎 ().[7][8]

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.[9] 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.[10]

References

  1. ^ a b "Bellona". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
  2. ^ a b c d e f "JPL Small-Body Database Browser: 28 Bellona". Jet Propulsion Laboratory. Retrieved 22 January 2026. 2025-07-08 last obs
  3. ^ 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.
  4. ^ 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.
  5. ^ "Archived copy". Archived from the original on 13 September 2006. Retrieved 12 August 2006.{{cite web}}: CS1 maint: archived copy as title (link)
  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.