From Wikipedia, the free encyclopedia

723 Hammonia
Discovery
Discovered by J. Palisa
Discovery site Vienna Observatory
Discovery date21 October 1911
Designations
(723) Hammonia
Pronunciation /hæˈmniə/
Named after
Hamburg
1911 NB
Orbital characteristics [1]
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)
2.9932 AU (447.78 Gm)
Eccentricity0.053719
5.18 yr (1891.5 d)
71.167 °
0° 11m 25.188s / day
Inclination4.9954°
163.351°
246.398°
Physical characteristics
17.84±0.7 km
5.436  h (0.2265  d)
0.1829±0.015
10.0

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. [2] (Vienna is the capital of Austria)

The asteroid was discovered by the noted and prolific astronomer Johann Palisa. [3] He worked from Pola early in his career and later from Vienna observatories. [3] The same night he discovered Hammonia, he also discovered 724 Hapag and 725 Amanda. [3] He discovered dozens and dozens of asteroids between 1874 and 1923, ranging from 136 Austria to 1073 Gellivara. [3]

As seen from a certain area on Earth, 723 Hammonia occulted the star 3UC149-190572 on June 3, 2013. [4]

In 2014 it was noted to have a high-albedo and amorphous Mg pyroxenes was suggested as a possible reason for this. [5]

See also

References

  1. ^ "723 Hammonia (1911 NB)". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 5 May 2016.
  2. ^ a b "(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. ^ a b c d "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.


From Wikipedia, the free encyclopedia

723 Hammonia
Discovery
Discovered by J. Palisa
Discovery site Vienna Observatory
Discovery date21 October 1911
Designations
(723) Hammonia
Pronunciation /hæˈmniə/
Named after
Hamburg
1911 NB
Orbital characteristics [1]
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)
2.9932 AU (447.78 Gm)
Eccentricity0.053719
5.18 yr (1891.5 d)
71.167 °
0° 11m 25.188s / day
Inclination4.9954°
163.351°
246.398°
Physical characteristics
17.84±0.7 km
5.436  h (0.2265  d)
0.1829±0.015
10.0

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. [2] (Vienna is the capital of Austria)

The asteroid was discovered by the noted and prolific astronomer Johann Palisa. [3] He worked from Pola early in his career and later from Vienna observatories. [3] The same night he discovered Hammonia, he also discovered 724 Hapag and 725 Amanda. [3] He discovered dozens and dozens of asteroids between 1874 and 1923, ranging from 136 Austria to 1073 Gellivara. [3]

As seen from a certain area on Earth, 723 Hammonia occulted the star 3UC149-190572 on June 3, 2013. [4]

In 2014 it was noted to have a high-albedo and amorphous Mg pyroxenes was suggested as a possible reason for this. [5]

See also

References

  1. ^ "723 Hammonia (1911 NB)". JPL Small-Body Database. NASA/ Jet Propulsion Laboratory. Retrieved 5 May 2016.
  2. ^ a b "(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. ^ a b c d "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.



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