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Discovery
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|---|---|
| Discovered by | Edward L. G. Bowell |
| Discovery date | January 24, 1982 |
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Designations
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| Named after | David D. Balam |
| Alternate name(s) | 1954 XM; 1962 ED; 1974 YO; 1982 BG1 |
| Minor planet category |
Main belt |
| Epoch November 26, 2005 (JD 2453700.5) | |
| Aphelion | 371.292 Gm (2.482 AU) |
| Perihelion | 297.982 Gm (1.992 AU) |
| Semi-major axis | 334.637 Gm (2.237 AU) |
| Eccentricity | 0.110 |
| Orbital period | 1221.998 d (3.35 a) |
| Average orbital speed | 19.85 km/s |
| Mean anomaly | 67.047° |
| Inclination | 5.382° |
| Longitude of ascending node | 295.903° |
| Argument of perihelion | 173.884° |
| Satellites | 2 (5.2±1 km) (1.5 km) |
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Physical characteristics
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| Dimensions | 7.2 km[1] |
| Mass | 5.09±0.2×1014 kg[1][2] |
| Mean density | 2.61±0.45 g/cm³[1][2] |
| Rotation period | 2.80483 hr[3] |
| Albedo | 0.16 |
| Temperature | ~183 K |
| Spectral type | S[1] |
| Absolute magnitude (H) | 13.4[3] |
3749 Balam is an asteroid orbiting in the asteroid belt. It is named after the Canadian astronomer David D. Balam.
A satellite with a diameter of ~1.5 km, designated S/2002 (3749) 1, was discovered by William J. Merline, Laird M. Close, Nick Siegler, Christophe Dumas, Clark R. Chapman, François J. Rigaut, François Ménard, William M. Owen Jr., and David C. Slater from the Gemini North Telescope, Mauna Kea; this was announced on February 13, 2002.[4] It orbits 289±13 km away in 61±10 days, with an orbital eccentricity of ~0.9.[2]
Being such as small primary body in the inner main belt with a separation of over 100 primary radii, S/2002 (3749) 1 is the most loosely-bound binary known.[5] Balam has a hill sphere with a radius of about 1,500 km.[2]
In March 2008, Franck Marchis discovered a larger (~3 km) inner companion, making this a triple system.[6][7][8]
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