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- Q1385800 subject Q13336749.
- Q1385800 subject Q18698486.
- Q1385800 subject Q8272864.
- Q1385800 absoluteMagnitude "10.7".
- Q1385800 abstract "Romulus is the outer and larger moon of the main-belt asteroid 87 Sylvia, not to be confused with the directly Sun-orbiting asteroid 10386 Romulus. It follows an almost-circular close-to-equatorial orbit around the parent asteroid. In this respect it is similar to the other moon Remus.Romulus was discovered in February 2001 from the Keck II telescope by Michael E. Brown and Jean-Luc Margot. Its full designation is (87) Sylvia I Romulus; before receiving its name, it was known as S/2001 (87) 1.The moon is named after Romulus, the mythological founder of Rome, one of the twins of Rhea Silvia raised by a wolf.87 Sylvia has a low density, which indicates that it is probably a rubble pile formed when debris from a collision between its parent body and another asteroid re-accreted gravitationally. Therefore, it is likely that both Romulus and Remus, the second of Sylvia's moons, are smaller rubble piles which accreted in orbit around the main body from debris of the same collision. In this case their albedo and density are expected to be similar to Sylvia's.Romulus' orbit is expected to be quite stable − it lies far inside Sylvia's Hill sphere (about 1/50 of Sylvia's Hill radius), but also far outside the synchronous orbit.From Romulus' surface, Sylvia takes up an angular region 16°×10° across, while Remus's apparent size varies between 0.62° and 0.19° (for comparison, Earth's Moon has an apparent size of about 0.5°).".
- Q1385800 averageSpeed "97.2".
- Q1385800 discovered "2001-02-18".
- Q1385800 discoverer Q298913.
- Q1385800 discoverer Q4022628.
- Q1385800 escapeVelocity "25.2".
- Q1385800 mass "4000.0".
- Q1385800 orbitalPeriod "60.480000000000004".
- Q1385800 thumbnail CMSylvia.png?width=300.
- Q1385800 wikiPageExternalLink 08582.html.
- Q1385800 wikiPageExternalLink 2005eso..pres...21..
- Q1385800 wikiPageExternalLink 07590.html.
- Q1385800 wikiPageExternalLink am-00087.html.
- Q1385800 wikiPageExternalLink asteroid-01b.html.
- Q1385800 wikiPageWikiLink Q107673.
- Q1385800 wikiPageWikiLink Q13336749.
- Q1385800 wikiPageWikiLink Q1792859.
- Q1385800 wikiPageWikiLink Q18698486.
- Q1385800 wikiPageWikiLink Q210997.
- Q1385800 wikiPageWikiLink Q2179.
- Q1385800 wikiPageWikiLink Q2197.
- Q1385800 wikiPageWikiLink Q219936.
- Q1385800 wikiPageWikiLink Q220.
- Q1385800 wikiPageWikiLink Q2309668.
- Q1385800 wikiPageWikiLink Q298913.
- Q1385800 wikiPageWikiLink Q313521.
- Q1385800 wikiPageWikiLink Q3863.
- Q1385800 wikiPageWikiLink Q4022628.
- Q1385800 wikiPageWikiLink Q405.
- Q1385800 wikiPageWikiLink Q462326.
- Q1385800 wikiPageWikiLink Q498792.
- Q1385800 wikiPageWikiLink Q573.
- Q1385800 wikiPageWikiLink Q8272864.
- Q1385800 wikiPageWikiLink Q828224.
- Q1385800 wikiPageWikiLink Q940979.
- Q1385800 absMagnitude "10.7".
- Q1385800 avgSpeed "27.0".
- Q1385800 discovered "2001-02-18".
- Q1385800 discoverer "Michael E. Brown and Jean-Luc Margot".
- Q1385800 escapeVelocity "~ 7 m/s".
- Q1385800 mass "~ 4 kg".
- Q1385800 name "Romulus".
- Q1385800 period "60.480000000000004".
- Q1385800 type Place.
- Q1385800 type CelestialBody.
- Q1385800 type Location.
- Q1385800 type Place.
- Q1385800 type Planet.
- Q1385800 type Thing.
- Q1385800 type Q634.
- Q1385800 comment "Romulus is the outer and larger moon of the main-belt asteroid 87 Sylvia, not to be confused with the directly Sun-orbiting asteroid 10386 Romulus. It follows an almost-circular close-to-equatorial orbit around the parent asteroid. In this respect it is similar to the other moon Remus.Romulus was discovered in February 2001 from the Keck II telescope by Michael E. Brown and Jean-Luc Margot.".
- Q1385800 label "Romulus (moon)".
- Q1385800 depiction CMSylvia.png.
- Q1385800 name "Romulus".