Astronomy:550 Senta
From HandWiki
.png) A three-dimensional model of 550 Senta based on its light curve | |
| Discovery | |
|---|---|
| Discovered by | Max Wolf |
| Discovery site | Heidelberg |
| Discovery date | 16 November 1904 |
| Designations | |
| (550) Senta | |
| Pronunciation | German: [ˈzɛntaː] |
| 1904 PL | |
| Orbital characteristics[1] | |
| Epoch 31 July 2016 (JD 2457600.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 115.33 yr (42124 d) |
| |{{{apsis}}}|helion}} | 3.1653 astronomical unit|AU (473.52 Gm) |
| |{{{apsis}}}|helion}} | 2.0115 AU (300.92 Gm) |
| 2.5884 AU (387.22 Gm) | |
| Eccentricity | 0.22287 |
| Orbital period | 4.16 yr (1521.1 d) |
| Mean anomaly | 17.4133° |
| Mean motion | 0° 14m 12.012s / day |
| Inclination | 10.108° |
| Longitude of ascending node | 270.702° |
| 45.342° | |
| Physical characteristics | |
| Mean radius | 18.875±1.9 km |
| Rotation period | 20.555 h (0.8565 d)[1][2] |
| Geometric albedo | 0.2215±0.052 |
| Absolute magnitude (H) | 9.37 |
Senta (minor planet designation: 550 Senta) is a minor planet orbiting the Sun that was discovered by German astronomer Max Wolf on 16 November 1904, from Heidelberg.
Photometric observations of this asteroid made at the Torino Observatory in Italy during 1990–1991 were used to determine a synodic rotation period of 20.555 ± 0.01 hours.[2]
In light of Max Wolf's propensity around the time of discovery to name asteroids after operatic heroines, it is likely that the asteroid is named after Senta, the heroine of Richard Wagner's opera The Flying Dutchman.[citation needed]
References
- ↑ 1.0 1.1 Yeomans, Donald K., "550 Senta", JPL Small-Body Database Browser (NASA Jet Propulsion Laboratory), https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=550, retrieved 5 May 2016.
- ↑ 2.0 2.1 di Martino, M. et al. (February 1994), "Lightcurves and rotational periods of nine main belt asteroids", Icarus 107 (2): 269–275, doi:10.1006/icar.1994.1022, Bibcode: 1994Icar..107..269D.
External links
- 550 Senta at AstDyS-2, Asteroids—Dynamic Site
- 550 Senta at the JPL Small-Body Database
 |  |
