1076 Viola

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1076 Viola
Discovery [1]
Discovered by K. Reinmuth
Discovery site Heidelberg Obs.
Discovery date5 October 1926
Designations
(1076) Viola
Pronunciation /ˈv.ələ/ [2]
Named after
Viola (flowering plant) [3]
1926 TE
main-belt  ·(inner)
Nysa [4]  · background [5]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc 90.48 yr (33,048 days)
Aphelion 2.8323 AU
Perihelion 2.1164 AU
2.4744 AU
Eccentricity 0.1447
3.89 yr (1,422 days)
70.608°
0° 15m 11.52s / day
Inclination 3.3195°
143.71°
304.08°
Physical characteristics
Dimensions 21.412±7.130 km [6]
21.43±6.81 km [7]
22.0±2.2 km [8]
22.273±0.069 km [9]
22.298±0.117 km [10]
22.63±2.7 km [11]
23.57±7.70 km [12]
24±2 km [13]
26.39±0.61 km [14]
7.336 h [15]
0.032±0.002 [14]
0.0375±0.0535 [6]
0.04±0.01 [8] [13]
0.04±0.02 [12]
0.04±0.05 [7]
0.041±0.004 [10]
0.0415±0.012 [11]
0.0428±0.0046 [9]
Tholen = F [1]
SMASS = C [1] [4]
B–V = 0.629 [1]
U–B = 0.250 [1]
12.21 [12]  ·12.30 [1] [4] [6] [7] [8] [9] [11] [13] [14]

    1076 Viola /ˈv.ələ/ , [16] provisional designation 1926 TE, is a Nysian asteroid from the inner regions of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 5 October 1926, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. [17] The asteroid was named after the flowering plant Viola . [3]

    Contents

    Orbit and classification

    Viola is a non-family asteroid of the main belt's background population when applying the Hierarchical Clustering Method to its proper orbital elements. [5] The asteroid has also been classified as a member of the Nysa family ( 405 ), [4] the largest asteroid family of the main belt, consisting of stony and carbonaceous subfamilies. The family, named after 44 Nysa, is located near the Kirkwood gap (3:1 orbital resonance with Jupiter), a depleted zone that separates the central main belt.

    Viola orbits the Sun in the inner asteroid belt at a distance of 2.1–2.8  AU once every 3 years and 11 months (1,422 days; semi-major axis of 2.47 AU). Its orbit has an eccentricity of 0.14 and an inclination of 3° with respect to the ecliptic. [1] The body's observation arc begins at Heidelberg in January 1951, or more than 24 years after its official discovery observation. [17]

    Physical characteristics

    In the Tholen classification, Viola is a rare F-type asteroid, while in the SMASS taxonomy, it is classified as a common, carbonaceous C-type. [1] [4]

    Rotation period

    In the 1980s, a rotational lightcurve of Viola was obtained from photometric observations by American astronomer Richard Binzel. Lightcurve analysis gave a well-defined rotation period of 7.336 hours with a brightness amplitude of 0.12 magnitude ( U=3 ). [15] A tentative period of 14.4 hours was measured by French amateur astronomer René Roy in January 2009, but later retracted from the LCDB ( U=n.a. ). [4] [18]

    Diameter and albedo

    According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Viola measures between 21.412 and 26.39 kilometers in diameter and its surface has an albedo between 0.032 and 0.0428. [6] [7] [8] [9] [10] [11] [12] [13] [14]

    The Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0415 and a diameter of 22.63 kilometers based on an absolute magnitude of 12.30. [4] [11]

    Naming

    This minor planet was named after Viola , a genus of flowering plants within the violet family. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 ( H 102 ). [3]

    Reinmuth's flowers

    Due to his many discoveries, Karl Reinmuth submitted a large list of 66 newly named asteroids in the early 1930s. The list covered his discoveries with numbers between (1009) and (1200). This list also contained a sequence of 28 asteroids, starting with 1054 Forsytia, that were all named after plants, in particular flowering plants (also see list of minor planets named after animals and plants). [19]

    References

    1. 1 2 3 4 5 6 7 8 9 "JPL Small-Body Database Browser: 1076 Viola (1926 TE)" (2017-03-29 last obs.). Jet Propulsion Laboratory . Retrieved 6 December 2017.
    2. "viola" . Oxford English Dictionary (Online ed.). Oxford University Press.(Subscription or participating institution membership required.)
    3. 1 2 3 Schmadel, Lutz D. (2007). "(1076) Viola". Dictionary of Minor Planet Names – (1076) Viola. Springer Berlin Heidelberg. p. 92. doi:10.1007/978-3-540-29925-7_1077. ISBN   978-3-540-00238-3.
    4. 1 2 3 4 5 6 7 "LCDB Data for (1076) Viola". Asteroid Lightcurve Database (LCDB). Retrieved 6 December 2017.
    5. 1 2 "Asteroid 1076 Viola – Nesvorny HCM Asteroid Families V3.0". Small Bodies Data Ferret. Retrieved 26 October 2019.
    6. 1 2 3 4 Masiero, Joseph R.; Nugent, C.; Mainzer, A. K.; Wright, E. L.; Bauer, J. M.; Cutri, R. M.; et al. (October 2017). "NEOWISE Reactivation Mission Year Three: Asteroid Diameters and Albedos". The Astronomical Journal. 154 (4): 10. arXiv: 1708.09504 . Bibcode:2017AJ....154..168M. doi: 10.3847/1538-3881/aa89ec .
    7. 1 2 3 4 Nugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015). "NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos". The Astrophysical Journal. 814 (2): 13. arXiv: 1509.02522 . Bibcode:2015ApJ...814..117N. doi:10.1088/0004-637X/814/2/117. S2CID   9341381 . Retrieved 6 December 2017.
    8. 1 2 3 4 Alí-Lagoa, V.; Licandro, J.; Gil-Hutton, R.; Cañ; ada-Assandri, M.; Delbo', M.; et al. (June 2016). "Differences between the Pallas collisional family and similarly sized B-type asteroids". Astronomy and Astrophysics. 591: 11. Bibcode:2016A&A...591A..14A. doi: 10.1051/0004-6361/201527660 . hdl: 11336/63614 .
    9. 1 2 3 4 Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv: 1109.6407 . Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. S2CID   35447010.
    10. 1 2 3 Masiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos". The Astrophysical Journal. 791 (2): 11. arXiv: 1406.6645 . Bibcode:2014ApJ...791..121M. doi:10.1088/0004-637X/791/2/121. S2CID   119293330.
    11. 1 2 3 4 5 Tedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0". NASA Planetary Data System. 12: IRAS-A-FPA-3-RDR-IMPS-V6.0. Bibcode:2004PDSS...12.....T . Retrieved 22 October 2019.
    12. 1 2 3 4 Nugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016). "NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos". The Astronomical Journal. 152 (3): 12. arXiv: 1606.08923 . Bibcode:2016AJ....152...63N. doi: 10.3847/0004-6256/152/3/63 .
    13. 1 2 3 4 Alí-Lagoa, V.; de León, J.; Licandro, J.; Delbó, M.; Campins, H.; Pinilla-Alonso, N.; et al. (June 2013). "Physical properties of B-type asteroids from WISE data". Astronomy and Astrophysics. 554: 16. arXiv: 1303.5487 . Bibcode:2013A&A...554A..71A. doi:10.1051/0004-6361/201220680. S2CID   119214002 . Retrieved 6 December 2017.
    14. 1 2 3 4 Usui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey". Publications of the Astronomical Society of Japan. 63 (5): 1117–1138. Bibcode:2011PASJ...63.1117U. doi:10.1093/pasj/63.5.1117. (online, AcuA catalog p. 153)
    15. 1 2 Binzel, R. P.; Mulholland, J. D. (December 1983). "A photoelectric lightcurve survey of small main belt asteroids". Icarus. 56 (3): 519–533. Bibcode:1983Icar...56..519B. doi:10.1016/0019-1035(83)90170-7. ISSN   0019-1035 . Retrieved 6 December 2017.
    16. /vˈlə/ is the pronunciation of the musical instrument, rather than the flower that this asteroid is named after.
    17. 1 2 "1076 Viola (1926 TE)". Minor Planet Center. Retrieved 6 December 2017.
    18. Behrend, Raoul. "Asteroids and comets rotation curves – (1076) Viola". Geneva Observatory. Retrieved 6 December 2017.
    19. Schmadel, Lutz D. (2007). "(1054) Forsytia". Dictionary of Minor Planet Names – (1054) Forsytia. Springer Berlin Heidelberg. p. 90. doi:10.1007/978-3-540-29925-7_1055. ISBN   978-3-540-00238-3.