Discovery[1] | |
---|---|
Discovered by | Y. Kushida O. Muramatsu |
Discovery site | Yatsugatake Obs. |
Discovery date | 3 November 1994 |
Designations | |
(15350) Naganuma | |
Named after | Naganuma[1] (Japanese town) |
1994 VB2 · 1998 WQ19 | |
main-belt[1][2] · (inner) background[3][4] | |
Orbital characteristics[2] | |
Epoch 27 April 2019 (JD 2458600.5) | |
Uncertainty parameter 0 | |
Observation arc | 23.69 yr (8,652 d) |
Aphelion | 3.0346 AU |
Perihelion | 1.7301 AU |
2.3823 AU | |
Eccentricity | 0.2738 |
3.68 yr (1,343 d) | |
240.74° | |
0° 16m 4.8s / day | |
Inclination | 4.6159° |
197.86° | |
204.64° | |
Physical characteristics | |
4.357±0.070 km[5][6][7] | |
2.5835±0.0001 h[8][a] | |
0.256[5][6][7] | |
S (assumed)[9] | |
13.90[5][7] 14.1[1][2] | |
15350 Naganuma, provisional designation 1994 VB2, is a stony background asteroid from the inner regions of the asteroid belt, approximately 4.3 kilometers (2.7 miles) in diameter. It was discovered on 3 November 1994, by Japanese astronomers Yoshio Kushida and Osamu Muramatsu at the Yatsugatake South Base Observatory. The likely S-type asteroid has a rotation period of 2.5 hours.[9] It was named for the town of Naganuma in northern Japan.[1]
MPC-object
was invoked but never defined (see the help page).jpldata
was invoked but never defined (see the help page).Ferret
was invoked but never defined (see the help page).AstDys-object
was invoked but never defined (see the help page).Mainzer-2016
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).Pray-2006f
was invoked but never defined (see the help page).lcdb
was invoked but never defined (see the help page).
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