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Asteroids with Satellites Database--Johnston's Archive

(87) Sylvia, Romulus,and Remus

compiled by Wm. Robert Johnston
last updated21 September 2014

--Orbital and physical data--

(Seethis page for definitions of quantities; source codes in brackets, seethis link for full references; *A, *D, and *E indicate assumed, derived, and estimated values, respectively.)

dynamical type, primary:main belt asteroid, outer


orbital data, primary (osculating elements)[JPL]:

semimajor axisa:3.481808398 AU
orbital periodP:6.497039467 yr
(= 2373.043665 d)
eccentricitye:0.091145156
perihelion distanceq:3.16445843 AU
aphelion distanceQ:3.799158367 AU
inclinationi:10.8768036°
argument of perihelionω:263.685494°
ascending nodeΩ:73.083782°
mean anomalyM:179.424861°
perihelion passageTP:2011 Feb 25.2693
Epoch:2014 May 23
data arc:1894-2013(2348 obs.)
Earth MOID:2.1794 AU
Jupiter Tisserand invariantTJ:3.094

orbital data, Romulus:

binary dynamical type:L [P07f]
semimajor axisas:1351.35± 0.01 km[B14h]
separation/primary radiusas/rp:9.5 [*D]
separation/Hill radiusas/rH:0.021 [*D]
orbital periodPs:3.654± 0.024d [F12b]
eccentricityes:0.0069± 0.0037[B14h]
inclinationis:1.7° ± 1.0° [M05a]
ascending nodeΩs:193.17° ± 1.85° [B14h]
argument of pericenterωs:175° ± 23° []
mean anomalyM:167° ± 23° [B14h]
Epoch:2004 Sep 01.0
normalized ang. mom.αL:0.65[P07f]

orbital data, Remus:

binary dynamical type:L [M09a]
semimajor axisas:701.64± 0.02 km[B14h]
separation/primary radiusas/rp:4.9 [*D]
separation/Hill radiusas/rH:0.011 [*D]
orbital periodPs:1.373± 0.01d [F12b]
eccentricityes:0.093± 0.021[B14h]
inclinationis:2.0° ± 1.0° [M05a]
ascending nodeΩs:194.28° ± 6.27° [B14h]
argument of pericenterωs:135° ± 9° []
mean anomalyM:-79° ± 9° [B14h]
Epoch:2004 Sep 01.0
normalized ang. mom.αL:0.65[M09a]
other data, system (combined):
absolute mag.H:6.94[MPC]
slope parameterG:(0.15) [*A]
effective diameterdE:286± 11 km [M05a]
geometric albedo:0.036± 0.008[M11b]
color indexU-B:0.251[T95a]
color indexB-V:0.71[JPL]
taxonomic type:X (SMASSII) [JPL]
P (Tholen) [JPL]
massm:1.48x1019 ± 6x1016kg [B14h]
densityρ:1.2± 0.1 g/cm3[M05a]
Hill radiusrH:64000 km [*D]

other data, primary:

diameterdp:286± 11 km [M05a]
dimensions:384 x 264 x 232km []
axial ratiosa/b, b/c:1.46, 1.14 [M05a]
rotation periodRPp:5.183640± 0.000005h [D95a]
amplitude in mag., rotationalΔM:?
pole directionΒ, λ:86 ± 6°,45 ± 10° [D95a]

other data, Romulus:

diameterds:10.8± 5.6km [F12b]
axial ratiosa/b, b/c:2.7;? [B14i]
diameter ratiods/dp:0.038± 0.02 [*D]
component mag. differenceΔM:6.24± 0.20 [I7590]
rotation periodRPs:?

other data, Remus:

diameterds:10.6± 1.6km [F12b]
diameter ratiods/dp:0.037± 0.006 [*D]
component mag. differenceΔM:7.2 [*D]
rotation periodRPs:?

--(87) Sylvia, Romulus, and Remus --discovery and notes:

Primary discovered1866 May 16from Madras, Indiaby N. R. Pogson.Alternate designation(s): A909 GA.Permanent number assigned 1866 May 28.

Named 1866 May 28 for the Roman mythological character and/or Sylvie Petiaux-Hugo Flammarion.

Second component discovered2001 Feb 18 by M. E. Brown and J. L. Margotusingadaptive optics telescope observations from W. M. Keck II Telescope, Mauna Kea, Hawaii, USA.Announced2001 Feb 23 [B01a].Provisional designation S/2001 (87) 1.Permanent designation I Romulus, assigned 2005 Aug 11; named for the Roman mythological character [M05h].

Third component discovered2004 Aug 09 by F. Marchis, P. Descamps, D. Hestroffer, and J. Berthierusingadaptive optics telescope observations from Very Large Telescope, ESO, Cerro Paranal, Chile.Announced2005 Aug 11 [M05a].Provisional designation S/2004 (87) 1.Permanent designation II Remus, assigned 2005 Aug 11; named for the Roman mythological character [M05h].

--Links, more technical:

--Links, less technical:

--Links to ADS abstracts:


©2001-2007, 2014by Wm. Robert Johnston.
Last modified21 September 2014.
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