Astronomy:245 Vera

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Short description: Asteroid
245 Vera
000245-asteroid shape model (245) Vera.png
3D model based on lightcurve data
Discovery
Discovered byN. R. Pogson
Discovery date6 February 1885
Designations
(245) Vera
Pronunciation/ˈvɪərə/
A885 CA, 1919 HB
Minor planet categoryMain belt
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc131.06 yr (47,869 d)
|{{{apsis}}}|helion}}3.70600 astronomical unit|AU (554.410 Gm)
|{{{apsis}}}|helion}}2.50409 AU (374.607 Gm)
3.10504 AU (464.507 Gm)
Eccentricity0.19354
Orbital period5.47 yr (1,998.5 d)
Average Orbital speed16.93 km/s
Mean anomaly120.926°
Mean motion0° 10m 48.493s / day
Inclination5.15859°
Longitude of ascending node61.2968°
329.674°
Physical characteristics
Dimensions79.50±3.2 km
Rotation period14.38 h (0.599 d)
Geometric albedo0.2082±0.018
Physicsunknown
S[2]
Absolute magnitude (H)7.82


Vera (minor planet designation: 245 Vera) is a large Main belt asteroid. It was discovered by N. R. Pogson on February 6, 1885, in Madras,[3] and was named at the suggestion of his wife.[4] The asteroid is orbiting the Sun at a distance of 3.11 astronomical unit|AU with a period of 5.47 years and an eccentricity (ovalness) of 0.19. The orbital plane is tilted at an angle of 5.16° to the plane of the ecliptic.[1] In 1890, Daniel Kirkwood noted that this asteroid shares similar orbital elements with 86 Semele and 106 Dione.[5]

Photometric measurements of this asteroid made during 1980–1981 were used to produce a light curve that demonstrated a rotation period of 14.38±0.03 h with a brightness variation of 0.26±0.01 in magnitude.[6] It is classified as a stony S-type asteroid in the Tholen system.[2] The asteroid has an estimated diameter of 75.95±2.63 km based on near infrared observations.[7]

References

  1. 1.0 1.1 "245 Vera". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=245. 
  2. 2.0 2.1 Xu, Shui et al. (May 1995), "Small Main-belt Asteroid Spectroscopic Survey: initial results", Icarus 115 (1): 1–35, doi:10.1006/icar.1995.1075, Bibcode1995Icar..115....1X. 
  3. Discovery Circumstances: Numbered Minor Planets (1)-(5000), IAU: Minor Planet Center, http://cfa-www.harvard.edu/iau/lists/NumberedMPs000001.html, retrieved 2021-09-12. 
  4. Schmadel, Lutz D. (2013), Dictionary of Minor Planet Names, Springer Berlin Heidelberg, ISBN 9783662028049, https://books.google.com/books?id=2lzoCAAAQBAJ&pg=PA53. 
  5. "On the similarity of certain orbits in the zone of asteroids", Publications of the Astronomical Society of the Pacific 2 (7): 95–97, 1890, doi:10.1086/120087. 
  6. Debehogne, H. et al. (November 1982), "Physical studies of asteroids. VIII - Photoelectric photometry of the asteroids 42, 48, 93, 105, 145 and 245", Astronomy and Astrophysics Supplement Series 50: 277–281, Bibcode1982A&AS...50..277D. 
  7. Masiero, Joseph R. et al. (August 2014), "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos", The Astrophysical Journal 791 (2): 11, doi:10.1088/0004-637X/791/2/121, 121, Bibcode2014ApJ...791..121M. 

Further reading

External links