2008 SV11

(2008 SV11 )

Discovery Circumstances:

Mt. Lemmon Survey - Mt. Lemmon Survey

25 Sep 2008

(1)

Orbital Type:

AP

(*)( 2)

Taxonomic Type:

CX

( 3)

Albedo:

-

-

Diameter:(km)

629 - 1407 m

($)

H:(mag)

18.40

(#)

G:

0.15

(#)

U-B:(mag)

-

-

B-V:(mag)

-

-

V-R:(mag)

-

-

R-I:(mag)

-

-

Rotation Period:(hrs)

32.4

( 4)

Quality:

2- !

( 4)

Lightcurve Amplitude:(mag)

0.5

( 4)

Spin Vector:

-

-

Sense of Rotation:

-

-

Radar Observations:

Y

( 5)

Spectral Observations:

-

-

IR Observations:

-

-

Remarks

* - orbital type derived from osculating orbital elements

$ - diameter range derived from H and assumed albedo for C and S type - 0.04 and 0.20 respectively

# - absolute magnitude H derived from astrometric observation via orbit determination - G value assumed to be 0.15

! - quality code according to Lagerkvist et al. (1989) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1162-1179.

References

( 1) M.P.E.C. 2008-S65

(002) Taylor, P.A. et al. (2009) DPS 41, 3201. (Variability of Thermal Infrared Emission from Near-Earth Asteroids) (2005GN59,1996HW1,2008SV11)

(003) Somers, J.M. et al. (2010) DPS 42, 1316. (abstract) (Optical Characterization Of Planetary Radar Targets, Low-deltaV, And Potentially Hazardous Asteroids: Results From 2009-2010)

(004) Warner, B.D. & R.D. Stephens (2009) MPB 36, 164-165. (ANALYSIS OF THE LIGHTCURVES OF 198 AMPELLA AND 2008 SV11)

(005) JPL's NEO Radar Detection Program Webpage


NEODyS Page of 2008 SV11