From Wikipedia, the free encyclopedia

695 Bella
A three-dimensional model of 695 Bella based on its light curve
Discovery
Discovered by Joel Hastings Metcalf
Discovery site Taunton, Massachusetts
Discovery date7 November 1909
Designations
(695) Bella
1909 JB
Orbital characteristics [1]
Epoch 31 July 2016 ( JD 2457600.5)
Uncertainty parameter 0
Observation arc102.48 yr (37432 d)
Aphelion2.9457  AU (440.67  Gm)
Perihelion2.1375 AU (319.77 Gm)
2.5416 AU (380.22 Gm)
Eccentricity0.15900
4.05 yr (1480.0 d)
183.825 °
0° 14m 35.7s / day
Inclination13.838°
275.632°
79.589°
Physical characteristics
24.09±0.75 km
14.222  h (0.5926  d)
0.1450±0.009
9.30

695 Bella is a minor planet orbiting the Sun.

Although this asteroid has dynamic properties that make it a candidate for the Maria family, the spectral properties of the object indicate it is most likely an interloper. Instead, it may have been spalled off from 6 Hebe or its parent body. 695 Bella and 6 Hebe orbit on opposite sides of the 3:1 Kirkwood gap, and the two have similar orbital elements. [2]

References

  1. ^ "695 Bella (1909 JB)". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 5 May 2016.
  2. ^ Fieber-Beyer, Sherry K.; et al. (June 2011), "The Maria asteroid family: Genetic relationships and a plausible source of mesosiderites near the 3:1 Kirkwood Gap", Icarus, 213 (2): 524–537, Bibcode: 2011Icar..213..524F, doi: 10.1016/j.icarus.2011.03.009, retrieved 23 December 2015.

External links


From Wikipedia, the free encyclopedia

695 Bella
A three-dimensional model of 695 Bella based on its light curve
Discovery
Discovered by Joel Hastings Metcalf
Discovery site Taunton, Massachusetts
Discovery date7 November 1909
Designations
(695) Bella
1909 JB
Orbital characteristics [1]
Epoch 31 July 2016 ( JD 2457600.5)
Uncertainty parameter 0
Observation arc102.48 yr (37432 d)
Aphelion2.9457  AU (440.67  Gm)
Perihelion2.1375 AU (319.77 Gm)
2.5416 AU (380.22 Gm)
Eccentricity0.15900
4.05 yr (1480.0 d)
183.825 °
0° 14m 35.7s / day
Inclination13.838°
275.632°
79.589°
Physical characteristics
24.09±0.75 km
14.222  h (0.5926  d)
0.1450±0.009
9.30

695 Bella is a minor planet orbiting the Sun.

Although this asteroid has dynamic properties that make it a candidate for the Maria family, the spectral properties of the object indicate it is most likely an interloper. Instead, it may have been spalled off from 6 Hebe or its parent body. 695 Bella and 6 Hebe orbit on opposite sides of the 3:1 Kirkwood gap, and the two have similar orbital elements. [2]

References

  1. ^ "695 Bella (1909 JB)". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 5 May 2016.
  2. ^ Fieber-Beyer, Sherry K.; et al. (June 2011), "The Maria asteroid family: Genetic relationships and a plausible source of mesosiderites near the 3:1 Kirkwood Gap", Icarus, 213 (2): 524–537, Bibcode: 2011Icar..213..524F, doi: 10.1016/j.icarus.2011.03.009, retrieved 23 December 2015.

External links



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