131 Vala

Vala (minor planet designation: 131 Vala) is an inner main-belt asteroid. 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.[4] 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.[5]

131 Vala
Orbital diagram
Discovery[1]
Discovered byChristian Heinrich Friedrich Peters
Discovery date24 May 1873
Designations
(131) Vala
Pronunciation/ˈvɑːlə/[2]
Named after
vǫlva
A873 KA; 1945 KA;
1952 DS3; 1953 QE
Main belt[1]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc142.88 yr (52187 d)
Aphelion2.60 AU (388.64 Gm)
Perihelion2.27 AU (338.99 Gm)
2.43 AU (363.82 Gm)
Eccentricity0.068233
3.79 yr (1,385.3 d)
19.08 km/s
289.275°
0° 15m 35.532s / day
Inclination4.9602°
65.682°
160.641°
Earth MOID1.26 AU (187.95 Gm)
Jupiter MOID2.38 AU (355.52 Gm)
TJupiter3.499
Physical characteristics
Dimensions40.44±1.8 km[1]
Mass6.9×1016 kg
Equatorial surface gravity
0.0113 m/s²
Equatorial escape velocity
0.0214 km/s
5.1812 h (0.21588 d)[1]
0.1051±0.010
Temperature~178 K
K[3] (Bus)
10.03[1]

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.[3] 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.[6] The result is double the 5.18-hour period reported in the JPL Small-Body Database.[1]

On 2028-Apr-05, Vala will pass 0.0276 AU (4,130,000 km; 2,570,000 mi) from asteroid 2 Pallas.[7]

References

Further reading

  • Franco, Lorenzo; et al. (October 2019), "Spin-Shape Model for 131 Vala", Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers, 46 (4): 392–394, Bibcode:2019MPBu...46..392F


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