Carbonaceous Meliboean asteroid
1165 Imprinetta , provisional designation 1930 HM , is a carbonaceous Meliboean asteroid from the outer regions of the asteroid belt , approximately 49 kilometers (30 mi) in diameter. It was discovered on 24 April 1930 by Dutch astronomer Hendrik van Gent at the Union Observatory in Johannesburg, South Africa.[ 15] The asteroid was named after Imprinetta Gent, wife of the discoverer.[ 2]
Orbit and classification
Imprinetta is a member of the Meliboea family , a smaller asteroid family of carbonaceous outer-belt asteroids with a few hundred members, named after 137 Meliboea .[ 4] [ 16] : 23
This asteroid orbits the Sun in the outer main-belt at a distance of 2.5–3.8 AU once every 5 years and 6 months (2,017 days). Its orbit has an eccentricity of 0.21 and an inclination of 13° with respect to the ecliptic .[ 1]
The body's observation arc begins with its first identification as A909 TA at Heidelberg Observatory in October 1909, more than 20 years prior to its official discovery observation at Johannesburg.[ 15]
Physical characteristics
Imprinetta has been characterized as a carbonaceous C-type asteroid by PanSTARRS photometric survey,[ 3] [ 14] which corresponds with the overall spectral type of the Meliboea family.[ 16] : 23
Rotation period
In October 2003, a rotational lightcurve of Imprinetta was obtained from photometric observations by American John Menke at his observatory in Barnesville, Maryland. Lightcurve analysis gave a well-defined rotation period of 8.107 hours with a brightness variation of 0.20 magnitude (U=3 ).[ 13] An alternative observation gave a lightcurve with period of 7.9374 hours and an amplitude of 0.20 magnitude (U=2 ).[ 12]
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 , Imprinetta measures between 47.14 and 59.378 kilometers (29.291 and 36.896 mi) in diameter and its surface has an albedo between 0.029 and 0.0562.[ 5] [ 6] [ 7] [ 8] [ 9] [ 10] [ 11]
The Collaborative Asteroid Lightcurve Link derives an albedo of 0.0392 and a diameter of 48.65 kilometers (30.23 mi) based on an absolute magnitude of 10.7.[ 3]
Naming
This minor planet was named after Imprinetta Gent, wife of the discoverer. The naming was proposed by the discoverer and by Gerrit Pels , who computed its orbit. The official naming citation was mentioned in The Names of the Minor Planets by Paul Herget in 1955 (H 108 ).[ 2]
References
^ a b c d "JPL Small-Body Database Browser: 1165 Imprinetta (1930 HM)" (2017-03-30 last obs.). Jet Propulsion Laboratory . Retrieved 6 September 2017 .
^ a b c Schmadel, Lutz D. (2007). "(1165) Imprinetta". Dictionary of Minor Planet Names . Springer Berlin Heidelberg . p. 98. doi :10.1007/978-3-540-29925-7_1166 . ISBN 978-3-540-00238-3 .
^ a b c d e f g "LCDB Data for (1165) Imprinetta" . Asteroid Lightcurve Database (LCDB). Retrieved 6 September 2017 .
^ a b "Asteroid 1165 Imprinetta – Nesvorny HCM Asteroid Families V3.0" . Small Bodies Data Ferret . Retrieved 31 October 2019 .
^ a b c d 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 . Retrieved 6 September 2017 .
^ a b c d 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 .
^ a b c d 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 .
^ a b c 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 . Retrieved 6 September 2017 .
^ a b c d 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 )
^ a b c d Masiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012). "Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids" . The Astrophysical Journal Letters . 759 (1): 5. arXiv :1209.5794 . Bibcode :2012ApJ...759L...8M . doi :10.1088/2041-8205/759/1/L8 . Retrieved 6 September 2017 .
^ a b c d 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 .
^ a b Monson, Andy; Kipp, Steven (December 2004). "Corrigendum: Rotational periods of asteroids 1165 Imprinetta, 1299 Mertona 1645 Waterfield, 1833 Shmakova, 2313 Aruna, and (13856) 1999 XZ105" . The Minor Planet Bulletin . 31 (4): 97. Bibcode :2004MPBu...31...97M . ISSN 1052-8091 . Retrieved 6 September 2017 .
^ a b Menke, John L. (September 2005). "Lightcurves and periods for asteroids 471 Papagena, 675 Ludmilla, 1016 Anitra, 1127 Mimi, 1165 Imprinetta, 1171 Rustahawelia, and 2283 Bunke" . The Minor Planet Bulletin . 32 (3): 64– 66. Bibcode :2005MPBu...32...64M . ISSN 1052-8091 . Retrieved 6 September 2017 .
^ a b c Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015). "Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results" . Icarus . 261 : 34– 47. arXiv :1506.00762 . Bibcode :2015Icar..261...34V . doi :10.1016/j.icarus.2015.08.007 . Retrieved 6 September 2017 .
^ a b "1165 Imprinetta (1930 HM)" . Minor Planet Center . Retrieved 6 September 2017 .
^ a b Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families". Asteroids IV . pp. 297– 321. arXiv :1502.01628 . Bibcode :2015aste.book..297N . doi :10.2458/azu_uapress_9780816532131-ch016 . ISBN 9780816532131 .
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