2000 DO8

(2000 DO8 )

Discovery Circumstances:

LINEAR - Lincoln Laboratory ETS, New Mexico

28 Feb 2000

(1)

Orbital Type:

AP

(*)

Taxonomic Type:

S:

( 2)

Albedo:

m

( 3)

Diameter:

0.04 km

( 4)

H:(mag)

24.5

( 5)

G:

0.15

(#)

U-B:(mag)

-

-

B-V:(mag)

-

-

Rotation Period:(hrs)

0.0217

( 6)( 7)( 8)

Quality:

3 !

( 6)( 7)( 8)

Lightcurve Amplitude:(mag)

1.39

( 6)( 7)( 8)

Spin Vector:

-

-

Radar Observations:

-

-

Spectral Observations:

Y

( 9)

IR Observations:

-

-

Remarks

* - orbital type derived from osculating orbital elements

# - 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)

References

( 1) M.P.E.C. 2000-E14

( 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) 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)

( 4) 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)

( 5) Whiteley, R.J. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 473-480. (Monolithic fast-rotating asteroids) (H-values and rotation properties of 36 NEAs)

( 6) Whiteley, R.J. et al. (2000) B.A.A.S. 32, 1003. (Lightcurve analysis of 4 monolithic fast-rotating asteroids.) (2000 AG6, 2000 DO8, 2000 EB14, 2000 HB24)

( 7) Whiteley, R.J. et al. (2002) Icarus 157, 139-154. (Lightcurve Analysis of Four New Monolithic Fast-Rotating Asteroids) (2000 AG6,2000 DO8, 2000 EB14,2000 HB24)

( 8) Whiteley, R.J. et al. (2002) Proceedings of ACM2002, ESA-SP500, pp. 473-480. (Monolithic fast-rotating asteroids) (H-values and rotation properties of 36 NEAs)

( 9) 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.)

NEODyS Page of 2000 DO8