A 3D lightcurve model of 131 Vala | |
| Discovery | |
|---|---|
| Discovered by | Christian Heinrich Friedrich Peters |
| Discovery site | Litchfield Observatory |
| Discovery date | 24 May 1873 |
| Designations | |
| Pronunciation | /ˈvɑːlə/ |
Named after | vǫlva |
| A873 KA; 1945 KA; 1952 DS3; 1953 QE | |
| Main belt | |
| Orbital characteristics | |
| Epoch 21 November 2025 (JD 2461000.5) | |
| Uncertainty parameter 0 | |
| Observation arc | 152.54 yr |
| Aphelion | 2.60 AU (389.00 Gm) |
| Perihelion | 2.26 AU (338.50 Gm) |
| 2.43 AU (363.75 Gm) | |
| Eccentricity | 0.069427 |
| 3.79 yr (1,384.89 d) | |
Average orbital speed | 19.08 km/s |
| 92.165° | |
| 0° 15m 35.784s / day | |
| Inclination | 4.9632° |
| 65.556° | |
| 161.388° | |
| Earth MOID | 1.26 AU (187.95 Gm) |
| Jupiter MOID | 2.38 AU (355.52 Gm) |
| TJupiter | 3.499 |
| Physical characteristics | |
| Dimensions | 40.44±1.8 km |
| Mass | 6.9×1016 kg |
Equatorial surface gravity | 0.0113 m/s² |
Equatorial escape velocity | 0.0214 km/s |
| 5.1812 h (0.21588 d) | |
| 0.1051±0.010 | |
| Temperature | ~178 K |
| K (Bus) | |
| 10.03 | |
131 Vala is an asteroid located in the main asteroid belt. It was discovered by C. H. F. Peters on 24 May 1873, and derives its name from völva (vǫlva, lit. 'staff bearer'), a prophetess in Norse paganism. One observation of an occultation of a star by Vala is from Italy (26 May 2002). 10-μm radiometric data collected from Kitt Peak in 1975 gave a diameter estimate of 34 km.
Vala was discovered on 24 May 1873 by German-American astronomer Christian Heinrich Friedrich Peters at Litchfield Observatory in New York State, United States. Peters announced the asteroid's discovery on 3 June in the journal Astronomische Nachrichten. The asteroid was given the name Vala, after the prophetesses (Old Norse: vǫlva) from Norse paganism.: 25 : 72ff
Vala orbits the Sun at an average distance of 2.43 astronomical units (AU), taking 3.79 Earth years to complete one orbit. This places it in the main asteroid belt, where it is classified as a background asteroid since it does not have any known relationship to an asteroid family. Its orbit has an inclination of 4.96° with respect to the ecliptic and an eccentricity of 0.07. Its distance from the Sun ranges from 2.26 AU at perihelion to 2.60 AU at aphelion.
In the Tholen classification system, it is categorized as an SU-type asteroid, while the Bus asteroid taxonomy system lists it as a K-type asteroid. Photometric observations of this asteroid during 2007 at the Organ Mesa Observatory in Las Cruces, New Mexico were used to create a "nearly symmetric bimodal" light curve plot. This showed a rotation period of 10.359 ± 0.001 hours and a brightness variation of 0.09 ± 0.02 magnitude during each cycle. The result is double the 5.18-hour period reported in the JPL Small-Body Database.