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723 Hammonia

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Minor planet orbiting the Sun

723 Hammonia
Discovery
Discovered byJ. Palisa
Discovery siteVienna Observatory
Discovery date21 October 1911
Designations
MPC designation(723) Hammonia
Pronunciation/hæˈmoʊniə/
Named afterHamburg
Alternative designations1911 NB
Orbital characteristics
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc113.17 yr (41337 d)
Aphelion3.1540 AU (471.83 Gm)
Perihelion2.8324 AU (423.72 Gm)
Semi-major axis2.9932 AU (447.78 Gm)
Eccentricity0.053719
Orbital period (sidereal)5.18 yr (1891.5 d)
Mean anomaly71.167°
Mean motion0° 11 25.188 / day
Inclination4.9954°
Longitude of ascending node163.351°
Argument of perihelion246.398°
Physical characteristics
Mean radius17.84±0.7 km
Synodic rotation period5.436 h (0.2265 d)
Geometric albedo0.1829±0.015
Absolute magnitude (H)10.0

723 Hammonia is a minor planet orbiting the Sun. It was discovered in 1911 and is named after the city of Hamburg. Although the name alludes to Hamburg it was discovered in Vienna.

The asteroid was discovered by the noted and prolific astronomer Johann Palisa. He worked from Pola early in his career and later from Vienna observatories. The same night he discovered Hammonia, he also discovered 724 Hapag and 725 Amanda. He discovered dozens and dozens of asteroids between 1874 and 1923, ranging from 136 Austria to 1073 Gellivara.

As seen from a certain area on Earth, 723 Hammonia occulted the star 3UC149-190572 on June 3, 2013.

In 2014 it was noted to have a high-albedo and amorphous Mg pyroxenes was suggested as a possible reason for this.

See also

References

  1. "723 Hammonia (1911 NB)". JPL Small-Body Database. NASA/Jet Propulsion Laboratory. Retrieved 5 May 2016.
  2. ^ "(723) Hammonia". Dictionary of Minor Planet Names. Springer. 2007. pp. 69–70. doi:10.1007/978-3-540-29925-7_724. ISBN 978-3-540-00238-3.
  3. ^ "Johann Palisa, the most successful visual discoverer of asteroids" (PDF). Archived from the original (PDF) on 28 September 2007. Retrieved 31 August 2015.
  4. OCULTACION 3UC149-190572 POR 723 HAMMONIA 2013-06-03
  5. Kasuga, T.; Usui, F.; Ootsubo, T.; Hasegawa, S.; Kuroda, D.; Shirahata, M.; Okamura, N. (2014). "High-albedo C-complex outer-belt asteroids: The near-infrared spectra". Asteroids: 254. Bibcode:2014acm..conf..254K.

External links

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