Discovery [2] [3] | |
---|---|
Discovered by | J. Helffrich |
Discovery site | Heidelberg Obs. |
Discovery date | 1910 |
Designations | |
(702) Alauda | |
Pronunciation | /əˈlɔːdə/ [4] [5] |
Named after | Alauda (genus of Birds) [6] |
1910 KQ | |
main-belt · (outer)
[7] Alauda [8] | |
Adjectives | Alaudian |
Orbital characteristics [2] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 106.89 yr (39,040 days) |
Aphelion | 3.2533 AU |
Perihelion | 3.1372 AU |
3.1953 AU | |
Eccentricity | 0.0182 |
5.71 yr (2,086 days) | |
311.58 ° | |
0° 10m 21.36s / day | |
Inclination | 20.589° |
289.77° | |
349.49° | |
Known satellites | 1 (Pichi üñëm) [9] [10] |
Physical characteristics | |
Dimensions | 163.98±57.99 km
[11] 172.29±55.38 km [12] 175 km [13] 190.58±2.65 km [14] 190.980±1.973 km [15] 194.73±3.2 km [16] 201.961±4.642 km [17] 202±20 km [18] |
Mass | (6.057±0.36)×1018 kg [19] |
Mean
density | 1.57±0.5 g/cm3 [19] |
8.3531 h (0.34805 d) [7] | |
0.0587±0.002 [2] | |
C (
Tholen)
[2] B ( SMASSII) [2] | |
11.42 to 13.57 [20] | |
7.25 [2] | |
702 Alauda /əˈlɔːdə/, provisional designation 1910 KQ, is a carbonaceous asteroid and binary system from the outer asteroid belt, approximately 190 kilometers in diameter. [2] It is the parent body of the Alauda family. Discovered in 1910 by German astronomer Joseph Helffrich at Heidelberg Observatory, it was named after the lark (alauda). [3] [6] Its small moon, named Pichi üñëm, was discovered in 2007. [10] [21]
Alauda's satellite Pichi üñëm provisionally known as S/2007 (702) 1, was discovered on 26 July 2007 from observations using adaptive-optics imaging with the European Southern Observatory (ESO) 8-m Very Large Telescope (VLT) on Cerro Paranal, Chile. [10] It is about 3.5 km in diameter (assuming it has the same albedo as the primary) and orbits Alauda in a nearly circular orbit at a distance of 1226.5±24 km. Pichi üñëm takes 4.91 days to complete one orbit. [19] [21] [22] It was named Pichi üñëm (Mapuche pronunciation: [ˈpɪtʃi ɨˈɲɘm], approximately /ˈpɪtʃi ɪˈnjʌm/), meaning "little bird" in the Mapuche language of Chile, the country from which the moon was discovered. [23]
Alauda has been identified as the largest member of the Alauda family, a dynamical family of bright carbonaceous asteroids with more than a thousand known members. [24]: 23 Other members of this family include: 581 Tauntonia, 1101 Clematis, 1838 Ursa, 3139 Shantou, 3325 TARDIS, 4368 Pillmore, 5360 Rozhdestvenskij, 5815 Shinsengumi, and many others. [25] Alauda's moon may be a result of the collision that created the asteroid family. [10]
The discovery and tracking of Alauda's moon enabled Alauda's mass to be determined. The discoverers of the moon, Patricio Rojo and Jean-Luc Margot, estimated Alauda's mass to be (6.057±0.36)×1018 kg and its density to be 1.57±0.5 g/cm3. [19]
Alauda has been observed to occult stars on several occasions, providing important information on its size and shape. It produced occultations on 2001-07-12 and 2004-04-21. [26] It may have occulted an apparent magnitude 9.5 star in the constellation of Gemini on 2009-10-17 at 08:18 UT. [1] This event should have been visible from Uruguay, Argentina, and Chile. [1]
Discovery [2] [3] | |
---|---|
Discovered by | J. Helffrich |
Discovery site | Heidelberg Obs. |
Discovery date | 1910 |
Designations | |
(702) Alauda | |
Pronunciation | /əˈlɔːdə/ [4] [5] |
Named after | Alauda (genus of Birds) [6] |
1910 KQ | |
main-belt · (outer)
[7] Alauda [8] | |
Adjectives | Alaudian |
Orbital characteristics [2] | |
Epoch 4 September 2017 ( JD 2458000.5) | |
Uncertainty parameter 0 | |
Observation arc | 106.89 yr (39,040 days) |
Aphelion | 3.2533 AU |
Perihelion | 3.1372 AU |
3.1953 AU | |
Eccentricity | 0.0182 |
5.71 yr (2,086 days) | |
311.58 ° | |
0° 10m 21.36s / day | |
Inclination | 20.589° |
289.77° | |
349.49° | |
Known satellites | 1 (Pichi üñëm) [9] [10] |
Physical characteristics | |
Dimensions | 163.98±57.99 km
[11] 172.29±55.38 km [12] 175 km [13] 190.58±2.65 km [14] 190.980±1.973 km [15] 194.73±3.2 km [16] 201.961±4.642 km [17] 202±20 km [18] |
Mass | (6.057±0.36)×1018 kg [19] |
Mean
density | 1.57±0.5 g/cm3 [19] |
8.3531 h (0.34805 d) [7] | |
0.0587±0.002 [2] | |
C (
Tholen)
[2] B ( SMASSII) [2] | |
11.42 to 13.57 [20] | |
7.25 [2] | |
702 Alauda /əˈlɔːdə/, provisional designation 1910 KQ, is a carbonaceous asteroid and binary system from the outer asteroid belt, approximately 190 kilometers in diameter. [2] It is the parent body of the Alauda family. Discovered in 1910 by German astronomer Joseph Helffrich at Heidelberg Observatory, it was named after the lark (alauda). [3] [6] Its small moon, named Pichi üñëm, was discovered in 2007. [10] [21]
Alauda's satellite Pichi üñëm provisionally known as S/2007 (702) 1, was discovered on 26 July 2007 from observations using adaptive-optics imaging with the European Southern Observatory (ESO) 8-m Very Large Telescope (VLT) on Cerro Paranal, Chile. [10] It is about 3.5 km in diameter (assuming it has the same albedo as the primary) and orbits Alauda in a nearly circular orbit at a distance of 1226.5±24 km. Pichi üñëm takes 4.91 days to complete one orbit. [19] [21] [22] It was named Pichi üñëm (Mapuche pronunciation: [ˈpɪtʃi ɨˈɲɘm], approximately /ˈpɪtʃi ɪˈnjʌm/), meaning "little bird" in the Mapuche language of Chile, the country from which the moon was discovered. [23]
Alauda has been identified as the largest member of the Alauda family, a dynamical family of bright carbonaceous asteroids with more than a thousand known members. [24]: 23 Other members of this family include: 581 Tauntonia, 1101 Clematis, 1838 Ursa, 3139 Shantou, 3325 TARDIS, 4368 Pillmore, 5360 Rozhdestvenskij, 5815 Shinsengumi, and many others. [25] Alauda's moon may be a result of the collision that created the asteroid family. [10]
The discovery and tracking of Alauda's moon enabled Alauda's mass to be determined. The discoverers of the moon, Patricio Rojo and Jean-Luc Margot, estimated Alauda's mass to be (6.057±0.36)×1018 kg and its density to be 1.57±0.5 g/cm3. [19]
Alauda has been observed to occult stars on several occasions, providing important information on its size and shape. It produced occultations on 2001-07-12 and 2004-04-21. [26] It may have occulted an apparent magnitude 9.5 star in the constellation of Gemini on 2009-10-17 at 08:18 UT. [1] This event should have been visible from Uruguay, Argentina, and Chile. [1]