2014 UV210

(2014 UV210)

Discovery Circumstances:

Pan-STARRS 1 - Pan-STARRS 1, Haleakala

25 Oct 2014

(1)

Orbital Type:

AM

(*)( 2)

Taxonomic Type:

-

-

Albedo:

-

-

Diameter:(km)

12 - 28 m

($)

H:(mag)

26.90

(#)

G:

0.15

(#)

U-B:(mag)

-

-

B-V:(mag)

-

-

V-R:(mag)

-

-

R-I:(mag)

-

-

V-I:(mag)

-

-

B-R:(mag)

-

-

Rotation Period:(hrs)

0.5559

( 3)

Quality:

3- !

( 3)

Lightcurve Amplitude:(mag)

0.91

( 3)

Spin Vector:

-

-

Sense of Rotation:

-

-

Radar Observations:

Y

( 4)

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

(001) M.P.E.C. 2014-X25

(002) Reddy, V. et al. (2015) LPSC 46, 1289. (PHYSICAL CHARACTERIZATION OF CHELYABINSK-SIZED (~20 METER) NEAR-EARTH ASTEROIDS: IMPLICATIONS FOR IMPACT HAZARD, METEORITE SOURCE BODIES, AND HUMAN EXPLORATION)(2009KW2,2014WY119,2014WC201,2014UV210,2014XB6)

(003) Thirouin, A.; Moskovitz, N.; Binzel, R.P.; Christensen, E.; et al. (2016) Astron. J. 152, A163.

(004) JPL's NEO Radar Detection Program Webpage


NEODyS Page of 2014 UV210