(363599) 2004 FG11

(2004 FG11 )

Discovery Circumstances:

LINEAR - Lincoln Laboratory ETS, New Mexico

23 Mar 2004

(1)

Orbital Type:

AP

(*)

Taxonomic Type:

V

( 2)( 3)

Albedo:

0.306

( 4)

Diameter:(km)

0.152 km

( 5)

H:(mag)

21.00

(#)

G:

0.15

(#)

U-B:(mag)

-

-

B-V:(mag)

-

-

V-R:(mag)

-

-

R-I:(mag)

-

-

Rotation Period:(hrs)

20.

( 6)

Quality:

2BR !

( 6)

Lightcurve Amplitude:(mag)

-

( 6)

Spin Vector:

-

-

Sense of Rotation:

-

-

Radar Observations:

Y

( 7)

Spectral Observations:

Y

( 8)

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) in "Asteroids II" (Eds. R.P.Binzel et al.), Univ.Ariz.Press, Tucson, USA, pp. 1162-1179.

B - in rotation quality code means Binary asteroid

R - as rotation quality code means Radar observations

References

( 1) M.P.E.C. 2004-F60

(002) Hicks, M. et al. (2010) ATel#2571 (Palomar Spectroscopy of 2001 FM129, 2004 FG11, and 2005 YU55)

(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) Mainzer, A. et al. (2014) Astrophys. J. 784, 110. (The Population of Tiny Near-Earth Objects Observed by NEOWISE)

(005) Mainzer, A. et al. (2014) Astrophys. J. 784, 110. (The Population of Tiny Near-Earth Objects Observed by NEOWISE)

(006) Taylor, P.A. et al. (2012) CBET 3091. (2004 FG11) (radar detection of a binary system)

(007) JPL's NEO Radar Detection Program Webpage

(008) Hicks, M. et al. (2010) ATel#2571 (Palomar Spectroscopy of 2001 FM129, 2004 FG11, and 2005 YU55)


NEODyS Page of (363599) 2004 FG11