Discovery | |
---|---|
Discovered by | George Henry Peters |
Discovery site | Washington, D.C. |
Discovery date | 11 May 1904 |
Designations | |
(536) Merapi | |
Pronunciation | /məˈrɑːpi/ |
Named after | Mount Mĕrapi, West Sumatera[1] |
1904 OF | |
Adjectives | Merapian |
Orbital characteristics[2] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 111.94 yr (40885 d) |
Aphelion | 3.7977 AU (568.13 Gm) |
Perihelion | 3.1992 AU (478.59 Gm) |
3.4984 AU (523.35 Gm) | |
Eccentricity | 0.085546 |
6.54 yr (2390.1 d) | |
302.40° | |
0° 9m 2.232s / day | |
Inclination | 19.425° |
59.239° | |
295.862° | |
Physical characteristics | |
75.71±4.5 km[2] 77.585 ± 1.765 km[3] | |
Mass | (2.61 ± 0.47) × 1019 kg[3] |
Mean density | 13.36 ± 2.59 g/cm3[3] |
8.78 h (0.366 d) | |
0.0452±0.006 | |
8.2 | |
536 Merapi is a main belt asteroid orbiting the Sun. It was discovered by American astronomer George Henry Peters on May 11, 1904, from Washington, D.C.[4]
Photometric observations of this asteroid at the Oakley Observatory in Terre Haute, Indiana, during 2006 gave a light curve with a period of 8.809 ± 0.008 hours and a brightness variation of 0.23 ± 0.05 in magnitude.[5]
JPL
was invoked but never defined (see the help page).Carry2012
was invoked but never defined (see the help page).IAU_MPC
was invoked but never defined (see the help page).Warner2008
was invoked but never defined (see the help page).