3551 Verenia help
Last update: 2025-05-29 13:38 UTC
Physical properties
  • Rotation Period
  • Quality
  • Amplitude
  • Rotation Direction
  • Spinvector L
  • Spinvector B
Rotational properties
Value
Unit
Source
Rotation Period
Value
4.930
Unit
h
Source
[4]
Quality
Value
2
Unit
-
Source
[4]
Amplitude
Value
0.11-0.15
Unit
mag
Source
[4]
Rotation Direction
Value
-
Unit
-
Source
[-]
Spinvector L
Value
-
Unit
Source
[-]
Spinvector B
Value
-
Unit
Source
[-]
  • Taxonomy
  • Taxonomy (all)
Taxonomy
Value
Unit
Source
Taxonomy
Value
U
V
Unit
-
-
Source
[1]
[2]
Taxonomy (all)
Value
-
V
Unit
-
-
Source
[3]
[2]
  • Absolute Magnitude (H)
  • Slope Parameter (G)
H / G
Value
Unit
Source
Absolute Magnitude (H)
Value
16.719
Unit
mag
Source
[5]
Slope Parameter (G)
Value
0.15**
Unit
mag
Source
[5]
  • Albedo
  • Diameter
Size and albedo
Value
Unit
Source
Albedo
Value
0.28
Unit
-
Source
[7]
Diameter
Value
870
Unit
Source
[6]
  • Color Index Information
Color Index Information
Value
Unit
Source
Color Index Information
Value
0.39
0.13
Unit
U-B
B-V
Source
[2]
[2]
  • Sightings
Sightings
Value
Unit
Source
Sightings
Value
-
Unit
-
Source
[-]

Sources

No.NameAdditional
No.[1]NameEARNAdditional1.) Alexey V. Sergeyev and Benoit Carry A&A, 652 (2021) A59
No.[2]NameEARNAdditional1.) Cruikshank, D.P. et al. (1991) Icarus 89, 1-13. (Three
basaltic earth-approaching asteroids and the source of the
basaltic meteorites)
No.[3]NameEARNAdditionalEarth Asteroids Research Node: https://earn.dlr.de
No.[4]NameEARNAdditional1.) Harris, A.W. & J.W. Young (1985) B.A.A.S. 17, 726.
(Photometric Results for Earth Approaching Asteroids.)
(1627,1036,1862,1982RA,1982XB,1983RD,1984KD)
2.) Binzel, R.P. (1987) Icarus 72, 135-208. (A photoelectric
survey of 130 asteroids)
3.) Wisniewski, W.Z. (1987) Icarus 70, 566-572. (Photometry of
six radar target asteroids)1986 DA, 3199, 3103, and 1983
RD. 1986 JK and 1986 RA
4.) Harris, A.W. (DLR) (1998) Icarus 131, 291-301. (A Thermal
Model for Near-Earth Asteroids)
No.[5]NameESA AegisAdditionalESA orbit determination and impact monitoring system
No.[6]NameEARNAdditional1.) Harris, A.W. (DLR) & J.S.V Lagerros (2002) in "Asteroids
III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA,
pp. 205-218. (Asteroids in the thermal infrared)
2.) Veeder, G.J. et al. (1989) Astron. J. 97, 1211-1219.
(Radiometry of near-earth asteroids)
3.) Cruikshank, D.P. et al. (1991) Icarus 89, 1-13. (Three
basaltic earth-approaching asteroids and the source of the
basaltic meteorites)
No.[7]NameEARNAdditional1.) Thomas, C.A. et al. (2011) Astron. J. 142, 85.
(ExploreNEOs. V. AVERAGE ALBEDO BY TAXONOMIC COMPLEX IN THE
NEAR-EARTH ASTEROID POPULATION) (new albedos data for 118
NEOs)
2.) Harris, A.W. (DLR) & J.S.V Lagerros (2002) in "Asteroids
III" (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA,
pp. 205-218. (Asteroids in the thermal infrared)
3.) Veeder, G.J. et al. (1989) Astron. J. 97, 1211-1219.
(Radiometry of near-earth asteroids)