Large asteroid with two moons
87 Sylvia is one of thelargest asteroids (approximately tied for 7th place, to within measurement uncertainties). It is the parent body of theSylvia family and member ofCybele group located beyond themain asteroid belt (seeminor-planet groups ). Sylvia was the first asteroid known to possess more than onemoon .
Discovery and naming [ edit ] Sylvia was discovered byN. R. Pogson on 16 May 1866, fromMadras (Chennai) ,India .[ 8] Antonio Paluzie-Borrell , writing inPaul Herget 'sThe Names of the Minor Planets (1955), mistakenly states that the name honorsSylvie Petiaux-Hugo Flammarion , the first wife of astronomerCamille Flammarion . In fact, in the article announcing the discovery of the asteroid, Pogson explained that he selected the name in reference toRhea Silvia , mother ofRomulus and Remus (MNRAS , 1866).
Physical characteristics [ edit ] Sylvia is very dark in color and probably has a primitive composition, though with some internal differentiation. The discovery of its moons made possible an accurate measurement of the asteroid's mass, density andmass distribution . Its density is low (around 1.4 times the density of water), indicating that the asteroid is porous; best-fit models estimate it had an original composition by volume of 35% rock, 13% ice and 52% internal voids, and that today it consists of a pristine anhydrous outer layer, and a differentiated interior, with meltwater having percolated inward so that the porosity of the rock is filled with ice out to a radius of about 46 km, then ice-free porous rock out to about 104 km.[ 3]
Sylvia is a fairly fast rotator, turning about its axis every 5.2 hours, giving it an equatorial rotation velocity of about 65 m/s, almost half the escape velocity.
Sylvia's shape is flattened and elongated (a/b ≈ 1.45 ; a/c ≈ 1.84) and somewhat irregular. However, its surface has not been imaged well enough for individual features to be resolved.
Adaptive Optics observations of (87) Sylvia, showing its two satellites,Remus andRomulus . Sylvia has two orbiting satellites. They have been named(87) Sylvia I Romulus and(87) Sylvia II Remus , afterRomulus and Remus , the children of the mythologicalRhea Silvia .
Romulus , the first moon, was discovered on 18 February 2001, from theKeck II telescope byMichael E. Brown andJean-Luc Margot .Remus , the second moon, was discovered over three years later on 9 August 2004, byFranck Marchis ofUC Berkeley , andPascal Descamps ,Daniel Hestroffer , andJérôme Berthier of theObservatoire de Paris , France.
The orbital properties of the satellites are listed in this table.[ 3] [ a] The orbital planes of both satellites and the equatorial plane of the primary asteroid are all well-aligned. Diameters are estimates based on the assumption that the moons have the same albedo as their primary.
Name Mass [kg] Diameter [km] Semi-major axis [km] Orbital period [days] Eccentricity Inclination [°] Remus (0.8± 0.2)× 1015 10+17 −6 694.2± 0.1 1.3570± 0.0003 0.005+0.010 −0.002 8.7± 1.8Romulus (1.4± 0.4)× 1015 23.1± 0.7[ 9] 1340 .6± 0.4 3.64126 ± 0.00002 0.000+0.003 −0.000 7.4± 0.5
^ Errors were published as 3 sigma. To maintain consistency with the table for Sylvia, they have here been reduced to 1 sigma. ^ Noah Webster (1884)A Practical Dictionary of the English Language ^ JPL data Retrieved 2021-09-29^a b c Carry, B.; et al. (June 2021)."Evidence for differentiation of the most primitive small bodies" .Astronomy & Astrophysics .650 A129.arXiv :2103.06349 .Bibcode :2021A&A...650A.129C .doi :10.1051/0004-6361/202140342 .ISSN 0004-6361 . ^ 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 . ^ Margot and Brown (2001), fromJim Baer (2008)."Recent Asteroid Mass Determinations" . Personal Website. Archived fromthe original on 2 July 2013. Retrieved5 December 2008 . ^ Supplemental IRAS Minor Planet Survey Archived 2009-08-17 at theWayback Machine ^ PDS spectral class data Archived 2009-08-05 at theWayback Machine ^ Pogson, N. R. (1866),Minor Planet (87) Sylvia ,Monthly Notices of the Royal Astronomical Society , Vol. 26, p. 311 (June 1866) ^ Berthier, Jerome; Vachier, Frédéric; Marchis, Franck; Ďurech, Josef; Carry, Benoît (1 September 2014). "Physical and dynamical properties of the main belt triple asteroid (87) Sylvia".Icarus .239 :118– 130.arXiv :1407.1292 .Bibcode :2014Icar..239..118B .doi :10.1016/j.icarus.2014.05.046 .S2CID 29853731 . Pogson, N. R. (1866),Minor Planet (87) Sylvia , Monthly Notices of the Royal Astronomical Society, Vol. 26, p. 311 (June 1866) Data on (87) Sylvia from Johnston's archive (maintained by W. R. Johnston)Rubble-Pile Minor Planet Sylvia and Her Twins (ESO news release, August 2005) Includes images and artists impressionsAdaptive Optics System Reveals New Asteroidal Satellite (SpaceDaily.com, March 2001) Includes a discovery image.Space.com: First asteroid trio discovered IAUC 7588 , reporting discovery of S/2001 (87) 1IAUC 7590 , confirming the discoveryIAUC 8582 , reporting discovery of S/2004 (87) 1 and naming Romulus and RemusAn animation of (87) Sylvia and its moons (on Vimeo) Shape model derived from lightcurve (on page 19) Instability zones for satellites of asteroids. The example of the (87) Sylvia system (arXiv :1112.5363 / 22 December 2011)Orbits, masses, and evolution of main belt triple (87) Sylvia (arXiv :1206.5755 / 25 June 2012)Occultation of TYC 1856-00745-1 by (87) Sylvia and by its satellite Romulus Archived 30 January 2013 at theWayback Machine (E. Frappa, A. Klotz, P. Dubreuil)87 Sylvia atAstDyS-2, Asteroids—Dynamic Site 87 Sylvia at theJPL Small-Body Database
Mean diameter 900–1000 km Mean diameter 500–600 km Mean diameter 300–500 km Mean diameter 200–300 km