117 Lomia

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117 Lomia
Discovery
Discovered by Alphonse Borrelly
Discovery date 12 September 1871
Designations
MPC designation (117) Lomia
Pronunciation /ˈlmiə/
 
Main belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 123.03 yr (44938 d)
Aphelion 3.0759 AU (460.15 Gm)
Perihelion 2.90810 AU (435.046 Gm)
2.99201 AU (447.598 Gm)
Eccentricity 0.028045
5.18 yr (1890.4 d)
17.22 km/s
317.47°
0° 11m 25.584s / day
Inclination 14.902°
348.790°
52.461°
Earth MOID 1.92459 AU (287.915 Gm)
Jupiter MOID 2.0407 AU (305.28 Gm)
TJupiter 3.204
Physical characteristics
Dimensions 148.71±6.6 km[1]
146.78 ± 3.96 km[2]
Mass (6.08 ± 0.63) × 1018 kg[2]
Mean density
3.67 ± 0.48 g/cm3[2]
Equatorial surface gravity
0.0416 m/s²
Equatorial escape velocity
0.0786 km/s
9.127 h (0.3803 d)
0.0528±0.005[1]
0.053[3]
Temperature ~161 K
XC[3]
7.95

117 Lomia is a large main-belt asteroid that has a nearly circular orbit; the orbital eccentricity is 0.029.[1] It was discovered by French astronomer Alphonse Borrelly on September 12, 1871, from the Marseilles Observatory.[4] The preliminary orbital elements were published in the following year by German astronomer Friedrich Tietjen.[5] The reason for the name is uncertain, but Lutz D. Schmadel believes it is most likely a misspelling of Lamia, the female demon of Greek mythology (the asteroid 248 Lameia is also named after this figure).[4]

Photometric observations of this asteroid in 1985 gave a light curve with a period of 9.127 ± 0.009 hours and a brightness variation of 0.29 ± 0.03 in magnitude. The curve is symmetrical with a single maxima and minima. This object has a spectrum that matches an XC classification; occupying the transition range between an X-type and a C-type asteroid.[3]

Two occultations of stars by Lomia have so far been observed, in 2000 and 2003.

References[edit]

  1. ^ a b c d Yeomans, Donald K., "117 Lomia", JPL Small-Body Database Browser, NASA Jet Propulsion Laboratory, retrieved 12 May 2016. 
  2. ^ a b c Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73, pp. 98–118, arXiv:1203.4336Freely accessible, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009.  See Table 1.
  3. ^ a b c di Martino, M.; et al. (July 1995), "Intermediate size asteroids: Photoelectric photometry of 8 objects.", Astronomy and Astrophysics Supplement, 112, pp. 1–7, Bibcode:1995A&AS..112....1D. 
  4. ^ a b Schmadel, Lutz D. (2003). Dictionary of Minor Planet Names. Springer Science & Business Media. p. 25. ISBN 978-3-540-00238-3. 
  5. ^ Tietjen, F. (1872), "Elemente und Ephemeride des Planeten (117) Lomia", Astronomische Nachrichten, 78 (21), pp. 329–330, doi:10.1002/asna.18710782106.  See Table 1.

External links[edit]