Discovery [1] | |
---|---|
Discovered by | D. D. Balam |
Discovery site | Climenhaga Obs. |
Discovery date | 20 October 1987 |
Designations | |
(4789) Sprattia | |
Named after | Christopher E. Spratt [1] (Canadian astronomer) |
1987 UU2 · 1976 HE1 | |
main-belt [1][2] · (inner)[3] background [4] | |
Orbital characteristics [2] | |
Epoch 23 March 2018 (JD 2458200.5) | |
Uncertainty parameter 0 | |
Observation arc | 41.82 yr (15,276 d) |
Aphelion | 2.5176 AU |
Perihelion | 1.9596 AU |
2.2386 AU | |
Eccentricity | 0.1246 |
3.35 yr (1,223 d) | |
45.388° | |
0° 17m 39.48s / day | |
Inclination | 1.2760° |
209.73° | |
152.92° | |
Physical characteristics | |
3.54±0.42 km[5] 4.172±0.232 km[6][7] 4.22 km (calculated)[3] | |
3.136±0.0005 h[8] | |
0.20 (assumed)[3] 0.279±0.070[6][7] 0.44±0.13[5] | |
S (Pan-STARRS)[3][9] S (SDSS-MOC)[10] | |
13.789±0.002 (R)[8] 13.80[5] 13.9[2][7] 14.24[3] 14.24±0.22[9] | |
4789 Sprattia, provisional designation 1987 UU2, is a stony background asteroid from the inner regions of the asteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 20 October 1987, by Canadian astronomer David Balam at the Climenhaga Observatory (657) in Victoria, Canada. The S-type asteroid has a rotation period of 3.1 hours and was named after Canadian amateur astronomer Christopher E. Spratt.[1][3]
MPC-object
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).lcdb
was invoked but never defined (see the help page).AstDys-object
was invoked but never defined (see the help page).Nugent-2015
was invoked but never defined (see the help page).Masiero-2011
was invoked but never defined (see the help page).WISE
was invoked but never defined (see the help page).Waszczak-2015
was invoked but never defined (see the help page).Veres-2015
was invoked but never defined (see the help page).SDSS-Taxonomy
was invoked but never defined (see the help page).