411 REFERENCE · Wikipedia
117 Lomia
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Main-belt asteroid
Lomia the village in Poland Łomia
October 2019
yes
#D6D6D6
117 Lomia
Alphonse Borrelly
12 September 1871
(117) Lomia
000117-asteroid shape model (117) Lomia.png
3D convex shape model of 117 Lomia
A871 RB;1900 DA;1900 MC
' l oʊ m i əPer 'Lamia', which this may be a misspelling of.
Lomian
Main belt
31 July 2016 (JD 2457600.5)
2.99201 AU Gm on
2.90810 AU Gm on
3.0759 AU Gm on on
0.028045
5.18 yr (1890.4 d)
14.902°
348.790°
52.461°
317.47°
17.22 km/s
148.71 6.6 km146.78 ± 3.96 km
(6.08 ± 0.63) × 1018 kg
3.67 ± 0.48 g/cm3
0.0416 m/s²
0.0786 km/s
9.127 h d on on
XC
7.95
0.0528 0.0050.053
~161 K
0.19044 ms / day
123.03 yr (44938 d)
0
1.92459 AU Gm on
2.0407 AU Gm on
3.204
117 Lomia is a large main-belt asteroid that has a nearly circular orbit; the orbital eccentricity is 0.029. It was discovered by French astronomer Alphonse Borrelly on September 12, 1871, from the Marseilles Observatory. The preliminary orbital elements were published in the following year by German astronomer Friedrich Tietjen. 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).Schmadel Lutz D. Dictionary of Minor Planet Names https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA20 2003 Springer Science & Business Media 978-3-540-00238-3 25
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. It has an estimated cross-section diameter of ~148 km.
Eight occultations of stars by Lomia have so far been observed, between 2000 and 2018. Four of these events provided two or more chords across the asteroid, including a four-chord event in 2003.
References
Donald K.
Yeomans
117 Lomia
JPL Small-Body Database Browser
NASA Jet Propulsion Laboratory
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=117
12 May 2016
.
F.
Tietjen
Elemente und Ephemeride des Planeten (117) Lomia
Astronomische Nachrichten
78
21
329–330
1872
10.1002/asna.18710782106
. https://zenodo.org/record/1424683
See Table 1.
B.
Carry
Density of asteroids
Planetary and Space Science
73
1
98–118
December 2012
10.1016/j.pss.2012.03.009
2012P&SS...73...98C
.
1203.4336 See Table 1.
di Martino
M.
Dotto
E.
Cellino
A.
Barucci
M. A.
Fulchignoni
M.
1
Intermediate size asteroids: Photoelectric photometry of 8 objects.
Astronomy and Astrophysics Supplement
112
1–7
July 1995
1995A&AS..112....1D
.
External links
117
116 Sirona 117 118 Peitho
000117
000117
000117
Category:Discoveries by Alphonse Borrelly
Category:Named minor planets
000117
18710912