From Wikipedia, the free encyclopedia
(Redirected from (28) Bellona)

28 Bellona
Bellona ( apmag 11.8) near a magnitude 12 star, next to Abell 2670 [1]
Discovery
Discovered by R. Luther
Discovery date1 March 1854
Designations
(28) Bellona
Pronunciation /bɛˈlnə/ [2]
Named after
Bellona
1951 CC2
Main belt
AdjectivesBellonian /bɛˈlniən/ [2]
Symbol (historical)
Orbital characteristics
Epoch Sept 30, 2012 ( JD 2456200.5)
Aphelion477.240 Gm (3.196 AU)
Perihelion353.977 Gm (2.358 AU)
415.608 Gm (2.777 AU)
Eccentricity0.151
1690.19 d (4.63 a)
121.574°
Inclination9.430°
144.330°
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 density
3.95 ± 1.28 g/cm3 [5]
15.706 h [4] [6]
0.1763 [4] [7]
S [4]
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 𜻎 ( ). [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". Astrometry.net. Retrieved 6 February 2015.
  2. ^ a b "Bellona". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution 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" (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 d e "JPL Small-Body Database Browser: 28 Bellona". Jet Propulsion Laboratory. Retrieved 28 January 2012. 2012-01-02 last obs
  5. ^ 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.
  6. ^ "Archived copy". Archived from the original on 13 September 2006. Retrieved 12 August 2006.{{ cite web}}: CS1 maint: archived copy as title ( link)
  7. ^ "Archived copy". Archived from the original on 22 July 2012. Retrieved 12 August 2006.{{ cite web}}: CS1 maint: archived copy as title ( link)
  8. ^ Bala, Gavin Jared; Miller, Kirk (18 September 2023). "Unicode request for historical asteroid symbols" (PDF). unicode.org. Unicode. Retrieved 26 September 2023.
  9. ^ Unicode. "Proposed New Characters: The Pipeline". unicode.org. The Unicode Consortium. Retrieved 6 November 2023.
  10. ^ "Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. Retrieved 30 October 2011.
  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, Bibcode: 2007MPBu...34..104W.
From Wikipedia, the free encyclopedia
(Redirected from (28) Bellona)

28 Bellona
Bellona ( apmag 11.8) near a magnitude 12 star, next to Abell 2670 [1]
Discovery
Discovered by R. Luther
Discovery date1 March 1854
Designations
(28) Bellona
Pronunciation /bɛˈlnə/ [2]
Named after
Bellona
1951 CC2
Main belt
AdjectivesBellonian /bɛˈlniən/ [2]
Symbol (historical)
Orbital characteristics
Epoch Sept 30, 2012 ( JD 2456200.5)
Aphelion477.240 Gm (3.196 AU)
Perihelion353.977 Gm (2.358 AU)
415.608 Gm (2.777 AU)
Eccentricity0.151
1690.19 d (4.63 a)
121.574°
Inclination9.430°
144.330°
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 density
3.95 ± 1.28 g/cm3 [5]
15.706 h [4] [6]
0.1763 [4] [7]
S [4]
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 𜻎 ( ). [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". Astrometry.net. Retrieved 6 February 2015.
  2. ^ a b "Bellona". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution 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" (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 d e "JPL Small-Body Database Browser: 28 Bellona". Jet Propulsion Laboratory. Retrieved 28 January 2012. 2012-01-02 last obs
  5. ^ 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.
  6. ^ "Archived copy". Archived from the original on 13 September 2006. Retrieved 12 August 2006.{{ cite web}}: CS1 maint: archived copy as title ( link)
  7. ^ "Archived copy". Archived from the original on 22 July 2012. Retrieved 12 August 2006.{{ cite web}}: CS1 maint: archived copy as title ( link)
  8. ^ Bala, Gavin Jared; Miller, Kirk (18 September 2023). "Unicode request for historical asteroid symbols" (PDF). unicode.org. Unicode. Retrieved 26 September 2023.
  9. ^ Unicode. "Proposed New Characters: The Pipeline". unicode.org. The Unicode Consortium. Retrieved 6 November 2023.
  10. ^ "Radar-Detected Asteroids and Comets". NASA/JPL Asteroid Radar Research. Retrieved 30 October 2011.
  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, Bibcode: 2007MPBu...34..104W.

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