(184266) 2004 VW14

(2004 VW14 )

Discovery Circumstances:

LONEOS - Lowell Observatory-LONEOS

3 Nov 2004

(1)

Orbital Type:

AP

(*)

Taxonomic Type:

Q,Sq

( 2)( 3)

Albedo:

-

-

Diameter:(km)

397 - 888 m

($)

H:(mag)

19.40

(#)

G:

0.15

(#)

U-B:(mag)

-

-

B-V:(mag)

-

-

V-R:(mag)

-

-

R-I:(mag)

-

-

Rotation Period:(hrs)

2.5009

( 4)

Quality:

3 !

( 4)

Lightcurve Amplitude:(mag)

0.14

( 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. 2004-V28

(002) Thomas, C.A. et al. (2014) Icarus 228, 217-246. (Physical characterization of Warm Spitzer-observed near-Earth objects)

(003) 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)

(004) Petr Pravec's Ondrejov NEO Photometric Program Webpage "Prepublished Periods"

(005) JPL's NEO Radar Detection Program Webpage


NEODyS Page of (184266) 2004 VW14