Astronomy:897 Lysistrata
From HandWiki
| Discovery | |
|---|---|
| Discovered by | Max Wolf |
| Discovery site | Heidelberg |
| Discovery date | 3 August 1918 |
| Designations | |
| (897) Lysistrata | |
| Pronunciation | /laɪˈsɪstrətə/[1] |
| 1918 DZ | |
| Orbital characteristics[2] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 97.33 yr (35551 days) |
| |{{{apsis}}}|helion}} | 2.7820 astronomical unit|AU (416.18 Gm) |
| |{{{apsis}}}|helion}} | 2.3016 AU (344.31 Gm) |
| 2.5418 AU (380.25 Gm) | |
| Eccentricity | 0.094510 |
| Orbital period | 4.05 yr (1480.2 d) |
| Mean anomaly | 87.8819° |
| Mean motion | 0° 14m 35.592s / day |
| Inclination | 14.326° |
| Longitude of ascending node | 257.977° |
| 24.460° | |
| Earth MOID | 1.29145 AU (193.198 Gm) |
| Jupiter MOID | 2.32255 AU (347.449 Gm) |
| TJupiter | 3.395 |
| Physical characteristics | |
| Mean radius | 10.955±0.7 km |
| Rotation period | 11.26 h (0.469 d) |
| Geometric albedo | 0.2619±0.036 |
| Absolute magnitude (H) | 10.37 |
897 Lysistrata /laɪˈsɪstrətə/ is a minor planet orbiting the Sun that was discovered by German astronomer Max Wolf on August 3, 1918.
This is a member of the dynamic Maria family of asteroids that most likely formed as the result of a collisional breakup of a parent body.[3]
References
- ↑ 'Lysistrate' in Noah Webster (1884) A Practical Dictionary of the English Language
- ↑ Yeomans, Donald K., "897 Lysistrata", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=897, retrieved 2 May 2016.
- ↑ Veeder, G. J. et al. (March 1995), "Eos, Koronis, and Maria family asteroids: Infrared (JHK) photometry", Icarus 114: pp. 186–196, doi:10.1006/icar.1995.1053, Bibcode: 1995Icar..114..186V, https://trs.jpl.nasa.gov/bitstream/2014/29296/1/95-0212.pdf.
External links
- 897 Lysistrata at AstDyS-2, Asteroids—Dynamic Site
- 897 Lysistrata at the JPL Small-Body Database
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