Romulus (moon)
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| Discovery[1] | |
|---|---|
| Discovered by | Michael E. Brown and Jean-Luc Margot |
| Discovered on | February 18, 2001 |
| Orbital characteristics[2] | |
| Is a satellite of | 87 Sylvia |
| Semimajor axis | 1356 ± 5 km |
| Eccentricity | 0.001 ± 0.001 |
| Orbital period | 3.6496 ± 0.0007 d |
| Orbital speed | 27.0 m/s |
| Inclination | 1.7 ± 1.0° (with respect to Sylvia equator) |
| Physical characteristics | |
| Dimensions | 18 ± 4 km[2][3] |
| Mass | ~ 4×1015 kg (estimate)[4] |
| Escape velocity | ~ 7 m/s (estimate) |
| Rotation period | unknown |
| Axial tilt | unknown |
| Albedo | unknown |
| Absolute magnitude | 10.7[2] |
Romulus is the outer and larger moon of the main belt asteroid 87 Sylvia. It follows an almost-circular close-to-equatorial orbit around the parent asteroid. In this respect it is similar to the other moon Remus. Not to be confused with the directly Sun-orbiting asteroid 10386 Romulus.
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 likely a rubble pile asteroid formed when debris from a collision between its parent body and another asteroid re-accreted gravitationally. It is likely then, 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.[2]
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.[2]
From Romulus' surface, Sylvia takes up an angular region 16°×10° across, while Remus apparent size varies between 0.62° and 0.19°.
[edit] See also
[edit] References
- ^ IAUC 7588, announcing the discovery of S/2001 (87) 1
- ^ a b c d e F. Marchis et al (2005). "Discovery of the triple asteroidal system 87 Sylvia". Nature 436: 822.
- ^ Assuming the same albedo as Sylvia
- ^ Assuming same density and albedo as Sylvia
[edit] External links
- 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 impressions
- Adaptive Optics System Reveals New Asteroidal Satellite (SpaceDaily.com, March 2001) Includes a discovery image.
- IAUC 7590, confirming the discovery of S/2001 (87) 1
- IAUC 8582, reporting discovery of S/2004 (87) 1 and naming Romulus and Remus
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| Vulcanoids | Near-Earth asteroids | Main belt | Jupiter Trojans | Centaurs | Damocloids | Comets | Trans-Neptunians (Kuiper belt · Scattered disc · Oort cloud) |
| For other objects and regions, see: asteroid groups and families, binary asteroids, asteroid moons and the Solar system For a complete listing, see: List of asteroids. See also Pronunciation of asteroid names and Meanings of asteroid names. |
