Remus (moon)

Remus
Adaptive Optics observations of (87) Sylvia, showing its two satellites, Remus and Romulus.
Discovery[1]
Discovered byFranck Marchis, Pascal Descamps,
Daniel Hestroffer, Jérôme Berthier
Discovery dateAugust 9, 2004
Designations
Sylvia II
Pronunciation/ˈrməs/
Named after
Rēmus
S/2004 (87) 1
Main belt (Cybele)
AdjectivesRemian /ˈrmiən/[2]
Orbital characteristics[3]
706 ± 5 km
Eccentricity0.016 ± 0.011
1.3788 ± 0.0007 d
37.2 m/s
Inclination2.0 ± 1.0°
(with respect to Sylvia equator)
Satellite of87 Sylvia
Physical characteristics
Dimensions7 ± 2 km [3][a]
Mass~ 2×1014 kg (estimate)[b]
Equatorial escape velocity
~ 4 m/s (estimate)
unknown, probably synchronous[c]
unknown, zero expected
11.1[3]

Remus is the inner and smaller moon of the main-belt asteroid 87 Sylvia. It follows an almost-circular and close-to-equatorial orbit around the parent asteroid. In this respect it is similar to the other Sylvian moon Romulus.

  1. ^ IAUC 8582, announcing the discovery of S/2004 (87) 1 and naming Romulus and Remus.
  2. ^ William Coe Collar (1891) The Gate to Caesar, p. 117
  3. ^ a b c F. Marchis; et al. (2005). "Discovery of the triple asteroidal system 87 Sylvia" (PDF). Nature. 436 (7052): 822–4. Bibcode:2005Natur.436..822M. doi:10.1038/nature04018. PMID 16094362. S2CID 4412813.


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