723 Hammonia is a minor planet orbiting the Sun. It was discovered in 1911 and is named after the city of Hamburg.[2] Although the name alludes to Hamburg it was discovered in Vienna.[3] (Vienna is the capital of Austria)
Discovery | |
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Discovered by | J. Palisa |
Discovery site | Vienna Observatory |
Discovery date | 21 October 1911 |
Designations | |
MPC designation | (723) Hammonia |
Pronunciation | /hæˈmoʊniə/ |
Named after | Hamburg |
Alternative designations | 1911 NB |
Orbital characteristics[1] | |
Epoch 31 July 2016 (JD 2457600.5) | |
Uncertainty parameter 0 | |
Observation arc | 113.17 yr (41337 d) |
Aphelion | 3.1540 AU (471.83 Gm) |
Perihelion | 2.8324 AU (423.72 Gm) |
Semi-major axis | 2.9932 AU (447.78 Gm) |
Eccentricity | 0.053719 |
Orbital period (sidereal) | 5.18 yr (1891.5 d) |
Mean anomaly | 71.167° |
Mean motion | 0° 11m 25.188s / day |
Inclination | 4.9954° |
Longitude of ascending node | 163.351° |
Argument of perihelion | 246.398° |
Physical characteristics | |
Mean radius | 17.84±0.7 km |
Synodic rotation period | 5.436 h (0.2265 d) |
Geometric albedo | 0.1829±0.015 |
Absolute magnitude (H) | 10.0 |
The asteroid was discovered by the noted and prolific astronomer Johann Palisa.[4] He worked from Pola early in his career and later from Vienna observatories.[5] The same night he discovered Hammonia, he also discovered 724 Hapag and 725 Amanda.[6] He discovered dozens and dozens of asteroids between 1874 and 1923, ranging from 136 Austria to 1073 Gellivara.[7]
As seen from a certain area on Earth, 723 Hammonia occulted the star 3UC149-190572 on June 3, 2013.[8]
In 2014 it was noted to have a high-albedo and amorphous Mg pyroxenes was suggested as a possible reason for this.[9]
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