Astronomy:131 Vala

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Short description: Main-belt asteroid
131 Vala
Орбита астероида 131.png
Orbital diagram
Discovery[1]
Discovered byChristian Heinrich Friedrich Peters
Discovery date24 May 1873
Designations
(131) Vala
Pronunciation/ˈvɑːlə/[2]
Named aftervǫlva
A873 KA; 1945 KA;
1952 DS3; 1953 QE
Minor planet categoryMain belt[1]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc142.88 yr (52187 d)
|{{{apsis}}}|helion}}2.60 astronomical unit|AU (388.64 Gm)
|{{{apsis}}}|helion}}2.27 AU (338.99 Gm)
2.43 AU (363.82 Gm)
Eccentricity0.068233
Orbital period3.79 yr (1,385.3 d)
Average Orbital speed19.08 km/s
Mean anomaly289.275°
Mean motion0° 15m 35.532s / day
Inclination4.9602°
Longitude of ascending node65.682°
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
Rotation period5.1812 h (0.21588 d)[1]
Geometric albedo0.1051±0.010
Physics~178 K
K[3] (Bus)
Absolute magnitude (H)10.03[1]


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]

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 astronomical unit|AU (4,130,000 km; 2,570,000 mi) from asteroid 2 Pallas.[7]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 1.6 "JPL Small-Body Database Browser: 131 Vala". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=131. Retrieved 12 May 2016. 
  2. "Vala". Dictionary.com Unabridged. Random House. https://www.dictionary.com/browse/Vala. 
  3. 3.0 3.1 DeMeo, Francesca E. et al. (July 2009), "An extension of the Bus asteroid taxonomy into the near-infrared", Icarus 202 (1): pp. 160–180, doi:10.1016/j.icarus.2009.02.005, Bibcode2009Icar..202..160D, archived from the original on 2014-03-17, https://web.archive.org/web/20140317200310/https://www.tara.tcd.ie/bitstream/2262/43276/1/PEER_stage2_10.1016/j.icarus.2009.02.005.pdf, retrieved 2013-04-08.  See appendix A.
  4. Schmadel, Lutz D.; International Astronomical Union (2003). Dictionary of minor planet names. Berlin; New York: Springer-Verlag. p. 27. ISBN 978-3-540-00238-3. https://books.google.com/books?id=KWrB1jPCa8AC&pg=PA27. 
  5. Morrison, D.; Chapman, C. R. (March 1976), "Radiometric diameters for an additional 22 asteroids", Astrophysical Journal 204: pp. 934–939, doi:10.1142/9789812834300_0469, Bibcode2008mgm..conf.2594S. 
  6. Pilcher, Frederick (June 2008), "Period Determination for 84 Klio, 98 Ianthe, 102 Miriam 112 Iphigenia, 131 Vala, and 650 Amalasuntha", The Minor Planet Bulletin 35 (2): pp. 71–72, doi:10.1016/j.pss.2012.03.009, Bibcode2008MPBu...35...71P. 
  7. "JPL Close-Approach Data: 131 Vala". https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=131;cad=1#cad. Retrieved 2011-12-07. 

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, Bibcode2019MPBu...46..392F 

External links