7341 1991VK
Last update: 2021-09-17 23:50 UTC
Physical properties
  • Rotation Period
  • Quality
  • Amplitude
  • Rotation Direction
  • Spinvector L
  • Spinvector B
Rotational properties
Value
Unit
Source
Rotation Period
Value
4.2096
Unit
h
Source
[3]
Quality
Value
3
Unit
-
Source
[3]
Amplitude
Value
0.28-0.7
Unit
mag
Source
[3]
Rotation Direction
Value
-
Unit
-
Source
[-]
Spinvector L
Value
-
Unit
Source
[-]
Spinvector B
Value
-
Unit
Source
[-]
  • Taxonomy
  • Taxonomy (all)
Taxononomy
Value
Unit
Source
Taxonomy
Value
Q
Unit
-
Source
[1]
Taxonomy (all)
Value
S,Sq,Sr
Unit
-
Source
[2]
  • Absolute Magnitude (H)
  • Slope Parameter (G)
H / G
Value
Unit
Source
Absolute Magnitude (H)
Value
16.849
Unit
mag
Source
[4]
Slope Parameter (G)
Value
0.26
Unit
mag
Source
[5]
  • Albedo
  • Diameter
Size and albedo
Value
Unit
Source
Albedo
Value
0.2355
Unit
-
Source
[7]
Diameter
Value
900
*Estimated from the absolute magnitude using
Unit
Source
[7]
  • Color Index Information
Color Index Information
Value
Unit
Source
Color Index Information
Value
-
Unit
mag
Source
[-]
  • Sightings
Sightings
Value
Unit
Source
Sightings
Value
Visual S
Unit
-
Source
[8]

Sources

No.NameAdditional
[1]EARN1.) DeMeo, F.E. et al. (2014) Icarus 227, 112-122. (Mars
encounters cause fresh surfaces on some near-Earth
asteroids) (contains taxonomic classification of 249 NEAs)
[2]EARN1.) Binzel, R.P. & S. Xu (1992) I.A.U. Circ. HREF="http://www.cbat.eps.harvard.edu/iauc/05400/05422.html">
5422.
(1991 VK, 1991 VL, 1991 WA and 1991 XB)
2.) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds.
W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp.
255-271. (Physical Properties of NEOs)
3.) Lazzarin, M. et al. (2004) Icarus 169, 373-384. (Visible
and near-infrared spectroscopic investigation of near-Earth
objects at ESO: first results)
4.) Bus, S.J. & Binzel, R.P. (2002) Icarus 158,106-145. (Phase
II of the Small Main-Belt Asteroid Spectrographic Survey: A
Feature-Based Taxonomy.)
5.) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed
spectral properties of near-Earth objects: results for
population distribution, source regions, and space
weathering processes.)
6.) Lazzarin, M., Marchi,S. & Magrin, S. (2010) href="http://www.astro.unipd.it/planets/sineo/data.html">
SINEO Database
(Spectroscopic Investiation of
Near-Earth Objects)
7.) DeMeo, F.E. et al. (2014) Icarus 227, 112-122. (Mars
encounters cause fresh surfaces on some near-Earth
asteroids) (contains taxonomic classification of 249 NEAs)
[3]EARN1.) Pravec, P. et al. (1998) Icarus 136, 124-153. (Lightcurves
of 26 Near-Earth Asteroids)(1943,2063,2100,3103,3122,3200,
3691,3752,4341,4957,5143,5587,7025,7341,7480,7482,7822,8034,
1989UQ,1992CC1,1992QN,1995FX,1997BR,1997GH3,1997GL3,1997SE5)
2.) Warner, B.D. (2017) MPB 44, 22-36. (NEAR-EARTH ASTEROID
LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2016
JULY-SEPTEMBER) (46 NEAs)
[4]ESA ODIMESA orbit determination and impact monitoring system
[5]EARN1.) Pravec, P. et al. (2012) Icarus 221, 365-387 (Absolute
magnitudes of asteroids and a revision of asteroid albedo
estimates from WISE thermal observations)
2.) Pravec, P. et al. (1998) Icarus 136, 124-153. (Lightcurves
of 26 Near-Earth Asteroids)(1943,2063,2100,3103,3122,3200,
3691,3752,4341,4957,5143,5587,7025,7341,7480,7482,7822,8034,
1989UQ,1992CC1,1992QN,1995FX,1997BR,1997GH3,1997GL3,1997SE5)
[6]NEODySNEO Dynamic Site: https://newton.spacedys.com/neodys2
[7]EARN1.) Masiero, J.R. et al. (2018) Astron. J. 154_168(10pp).
(NEOWISE Reactivation Mission Year Three: Asteroid
Diameters and Albedos) (170NEOs, 6110MBAs)
2.) Usui, F. et al. (2011) Pub. Astron. Soc. Japan 63,
1117-1138. (Asteroid Catalog Using AKARI: AKARI/IRC
Mid-Infrared Asteroid Survey)
3.) Binzel, R.P. et al. (2002) in "Asteroids III" (Eds.
W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp.
255-271. (Physical Properties of NEOs)
[8]EARN1.) Lazzarin, M. et al. (2004) Icarus 169, 373-384. (Visible
and near-infrared spectroscopic investigation of near-Earth
objects at ESO: first results)
2.) Binzel, R.P. et al. (2004) Icarus 170, 259-294. (Observed
spectral properties of near-Earth objects: results for
population distribution, source regions, and space
weathering processes.)
3.) Lazzarin, M., Marchi,S. & Magrin, S. (2010) href="http://www.astro.unipd.it/planets/sineo/data.html">
SINEO Database
(Spectroscopic Investiation of
Near-Earth Objects)
4.) deLeon, J. et al. (2010) Astron. Astrophys 517, A23.
(Observations, compositional, and physical characterization
of near-Earth and Mars-crosser asteroids from a
spectroscopic survey)
[9]EARN1.) Ostro, S.J. et al. (1998) B.A.A.S 30, 1036.
(Near-Earth-Asteroid Radar at Goldstone, Aug 1996 - Jun
1998) [7822(1991CS),4197(1982TA),4179Toutatis,7341(1991VK),
7482(1994PC1),1997BR,1998BY7,6037(1988EG),1998KY26]
2.) href="http://echo.jpl.nasa.gov/asteroids/index.html">JPL's
NEO Radar Detection Program Webpage
**Estimated value