Astronomy:28 Bellona

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Short description: Main-belt asteroid
28 Bellona Bellona symbol (bold).svg (historical)
28Bell-LB1-mag12.jpg
Bellona (apmag 11.8) near a magnitude 12 star, next to Abell 2670[1]
Discovery
Discovered byR. Luther
Discovery date1 March 1854
Designations
(28) Bellona
Pronunciation/bɛˈlnə/[2]
Named afterBellona
1951 CC2
Minor planet categoryMain belt
AdjectivesBellonian /bɛˈlniən/[2]
Orbital characteristics
Epoch Sept 30, 2012 (JD 2456200.5)
|{{{apsis}}}|helion}}477.240 Gm (3.196 AU)
|{{{apsis}}}|helion}}353.977 Gm (2.358 AU)
415.608 Gm (2.777 AU)
Eccentricity0.151
Orbital period1690.19 d (4.63 a)
Mean anomaly121.574°
Inclination9.430°
Longitude of ascending node144.330°
344.461°
Physical characteristics
Dimensions97 ± 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 density3.95 ± 1.28 g/cm3[5]
Rotation period15.706 h[4][6]
Geometric albedo0.1763[4][7]
S[4]
Absolute magnitude (H)7.09[4]


Bellona (minor planet designation: 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 𜻎 (Bellona symbol (fixed width).svg).[8][9]

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

  1. "Astrometry.net job 1005148". http://nova.astrometry.net/user_images/567142#annotated. Retrieved 6 February 2015. 
  2. 2.0 2.1 Bellona (3rd ed.), Oxford University Press, September 2005, http://oed.com/search?searchType=dictionary&q=Bellona  (Subscription or UK public library membership required.)
  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". Icarus 214 (2): 652–670. doi:10.1016/j.icarus.2011.03.016. Bibcode2011Icar..214..652D. http://astro.troja.mff.cuni.cz/projects/asteroids3D/download/durech_et_al_2011_occ_paper.pdf. Retrieved 26 January 2012. 
  4. 4.0 4.1 4.2 4.3 4.4 "JPL Small-Body Database Browser: 28 Bellona". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=28. Retrieved 2012-01-28. "2012-01-02 last obs" 
  5. 5.0 5.1 5.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73 (1): 98–118, doi:10.1016/j.pss.2012.03.009, Bibcode2012P&SS...73...98C.  See Table 1.
  6. "Archived copy". http://www.psi.edu/pds/asteroid/EAR_A_5_DDR_DERIVED_LIGHTCURVE_V8_0/data/lc.tab. 
  7. "Archived copy". http://www.psi.edu/pds/asteroid/EAR_A_5_DDR_ALBEDOS_V1_1/data/albedos.tab. 
  8. Bala, Gavin Jared; Miller, Kirk (18 September 2023). "Unicode request for historical asteroid symbols". Unicode. https://www.unicode.org/L2/L2023/23207-historical-asteroids.pdf. 
  9. Unicode. "Proposed New Characters: The Pipeline". The Unicode Consortium. https://unicode.org/alloc/Pipeline.html. 
  10. "Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. http://echo.jpl.nasa.gov/asteroids/. Retrieved 2011-10-30. 
  11. Warner, Brian D. (December 2007), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory - March-May 2007", The Minor Planet Bulletin 34 (4): 104–107, Bibcode2007MPBu...34..104W. 

External links