471 Papagena
From Wikipedia, the free encyclopedia
Discovery[1] and designation | |
---|---|
Discovered by | Max Wolf |
Discovery date | June 7, 1901 |
Designations | |
Alternative names | 1901 GN |
Minor planet category | Main belt |
Orbital characteristics[1] | |
Epoch April 10, 2007 (JD 2454200.5) | |
Aphelion | 3.5595 AU (Q) |
Perihelion | 2.2118 AU (q) |
Semi-major axis | 2.8856 AU (a) |
Eccentricity | 0.2335 |
Orbital period | 4.90 a |
Mean anomaly | 83.155° (M) |
Inclination | 14.985° |
Longitude of ascending node | 84.095° |
Physical characteristics | |
Dimensions |
134.19 km[1] 124.55 ± 8.77[2] km |
Mass | (3.05 ± 1.73) × 1018[2] kg |
Mean density | 3.01 ± 1.82[2] g/cm3 |
Geometric albedo | 0.1994[1] |
Spectral type | S[1] |
Apparent magnitude | 9.27 to 13.13 |
Absolute magnitude (H) | 6.72[3] |
Angular diameter | 0.147" to 0.041" |
|
471 Papagena is an asteroid that was discovered by German astronomer Max Wolf on June 7, 1901.[1] Its provisional name was 1901 GN.
Papagena comes to a favorable near-opposition apparent magnitude of better than magnitude 9.8 every five years. On September 30, 2010, it will be magnitude 9.68 and will get brighter every five years until December 12, 2035, when this late-to-be-discovered asteroid will be at magnitude 9.28. It is named for a character in Mozart's opera, The Magic Flute.
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 Yeomans, Donald K., "471 Papagena", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), retrieved 2013-03-25.
- ↑ 2.0 2.1 2.2 Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science 73: 98-118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009. See Table 1.
- ↑ Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers 34: 113–119, Bibcode:2007MPBu...34..113W.
External links
- Orbital simulation from JPL (Java) / Ephemeris
|
This article is issued from Wikipedia. The text is available under the Creative Commons Attribution/Share Alike; additional terms may apply for the media files.