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173 Ino

Ino (minor planet designation: 173 Ino) is a large asteroid and the parent body of the Ino family, located in the central regions of the asteroid belt, approximately 150 kilometers (93 miles) in diameter. It was discovered on 1 August 1877, by French astronomer Alphonse Borrelly at Marseille Observatory in southern France, and named after the queen Ino from Greek mythology.[1][2] The dark Xk-type asteroid has a rotation period of 6.15 hours.[21]

173 Ino
Discovery[1]
Discovered byA. Borrelly
Discovery siteMarseille
Discovery date1 August 1877
Designations
(173) Ino
Pronunciation/ˈn/ EYE-noh[5]
Named after
Ἰνώ Īnṓ[2] (Greek mythology)
A877 PA; 1922 SB
main-belt[1][3] · (middle)
Ino[4]
AdjectivesInoan (/ˈnən/ eye-NOH-ən)[6]
Orbital characteristics[3]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc138.75 yr (50,678 d)
Aphelion3.3142 AU
Perihelion2.1708 AU
2.7425 AU
Eccentricity0.2085
4.54 yr (1,659 d)
307.27°
0° 13m 1.2s / day
Inclination14.197°
148.18°
228.89°
Physical characteristics
Dimensionsc/a = 0.76±0.06[7]
Mean diameter
145±3 km[7]
119±27 km[8]
125.8±1.5 km[9]
148±42 km[10]
154.1±3.5 km[11]
160.6 km[12]
Mass(2.2±1.3)×1018 kg[7]
(4.79±3.11)×1018 kg[13]
Mean density
1.4±0.8 g/cm3[7]
2.23±1.47 g/cm3[13]
5.93 h[14]
6.1±0.2 h[15]
6.106±0.001 h[15]
6.1088±0.0007 h[15]
6.11 h[16]
6.113±0.002 h[17]
6.11651 h[18]
6.15 h[19]
6.163 h[20]
0.061 (calculated)[7]
0.059[12]
0.06±0.02[10]
0.0642±0.003[11]
0.07±0.05[8]
0.096±0.018[9]
Tholen = C[3]
SMASS = Xk[3]
B–V = 0.705[3]
U–B = 0.305[3]
7.66[3][9][10][11][12][21]
7.80±0.05[22]
7.90[8][23]

Orbit and classification

Ino is the parent body and namesake of the Ino family (522),[4] an asteroid family in the intermediate main belt with nearly 500 known members.[24]: 23  The adjectival form of the asteroid name is "Inoan".

It orbits the Sun in the central main-belt at a distance of 2.2–3.3 AU once every 4 years and 6 months (1,659 days; semi-major axis of 2.74 AU). Its orbit has an eccentricity of 0.21 and an inclination of 14° with respect to the ecliptic.[3] The body's observation arc begins at Düsseldorf-Bilk Observatory in January 1879, five months after its official discovery observation at Marseilles.[1]

Physical characteristics

In the Tholen classification, Ino is a common carbonaceous C-type, while in the SMASS classification it is a Xk-subtype that transitions between the X-type and uncommon K-type asteroids.[3]

Multiple photometric studies of this asteroid were performed between 1978 and 2002. The combined data gave an irregular, asymmetrical light curve with a period of 6.163 ± 0.005 hours and a brightness variation of 0.10–0.15 in magnitude. The asteroid is rotating in a retrograde direction.[18]

References

  1. ^ a b c d "173 Ino". Minor Planet Center. Retrieved 18 April 2018.
  2. ^ a b Schmadel, Lutz D. (2007). "(173) Ino". Dictionary of Minor Planet Names – (173) Ino. Springer Berlin Heidelberg. p. 30. doi:10.1007/978-3-540-29925-7_174. ISBN 978-3-540-00238-3.
  3. ^ a b c d e f g h i "JPL Small-Body Database Browser: 173 Ino" (2017-10-21 last obs.). Jet Propulsion Laboratory. Retrieved 18 April 2018.
  4. ^ a b "Asteroid 173 Ino". Small Bodies Data Ferret. Retrieved 24 October 2019.
  5. ^ Noah Webster (1884) A Practical Dictionary of the English Language
  6. ^ George Stuart (1882) The Eclogues, Georgics, and Moretum of Virgil, p. 271
  7. ^ a b c d e P. Vernazza et al. (2021) VLT/SPHERE imaging survey of the largest main-belt asteroids: Final results and synthesis. Astronomy & Astrophysics 54, A56
  8. ^ a b c 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.
  9. ^ a b c 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.
  10. ^ a b c 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.
  11. ^ a b c 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. ^ a b c 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)
  13. ^ a b Carry, B. (December 2012), "Density of asteroids", Planetary and Space Science, 73 (1): 98–118, arXiv:1203.4336, Bibcode:2012P&SS...73...98C, doi:10.1016/j.pss.2012.03.009 See Table 1.
  14. ^ Schober, H. J. (December 1978). "Photometric Variations of the Minor Planets 55 Pandora and 173 Ino during the Opposition in 1977: Light Curves and Rotation Periods". Astronomy and Astrophysics Supplement. 34: 377. Bibcode:1978A&AS...34..377S. Retrieved 18 April 2018.
  15. ^ a b c Behrend, Raoul. "Asteroids and comets rotation curves – (173) Ino". Geneva Observatory. Retrieved 18 April 2018.
  16. ^ Erikson, A. (December 1989). "Improvement of Rotation Periods for the Asteroids 12 Victoria, 173 Ino and 1245 Calvinia". Asteroids: 55. Bibcode:1990acm..proc...55E. Retrieved 18 April 2018.
  17. ^ Gandolfi, D.; Cigna, M.; Fulvio, D.; Blanco, C. (January 2009). "CCD and photon-counting photometric observations of asteroids carried out at Padova and Catania observatories". Planetary and Space Science. 57 (1): 1–9. arXiv:0810.1560. Bibcode:2009P&SS...57....1G. doi:10.1016/j.pss.2008.09.014.
  18. ^ a b Michalowski, T.; Kaasalainen, M.; Marciniak, A.; Denchev, P.; Kwiatkowski, T.; Kryszczynska, A.; et al. (November 2005). "Photometry and models of selected main belt asteroids. II. 173 Ino, 376 Geometria, and 451 Patientia". Astronomy and Astrophysics. 443 (1): 329–335. Bibcode:2005A&A...443..329M. doi:10.1051/0004-6361:20053656. Retrieved 18 April 2018.
  19. ^ Debehogne, H.; Lagerkvist, C.-I.; Magnusson, P.; Hahn, G. (December 1989). "Physical studies of asteroids XX - Photoelectric photometry of asteroids". Asteroids: 45. Bibcode:1990acm..proc...45D. Retrieved 18 April 2018.
  20. ^ Michalowski, Tadeusz (December 1993). "Poles, shapes, senses of rotation, and sidereal periods of asteroids". Icarus. 106 (2): 563. Bibcode:1993Icar..106..563M. doi:10.1006/icar.1993.1193. Retrieved 18 April 2018.
  21. ^ a b "LCDB Data for (173) Ino". Asteroid Lightcurve Database (LCDB). Retrieved 18 April 2018.
  22. ^ Warner, Brian D. (December 2007). "Initial Results of a Dedicated H-G Project". The Minor Planet Bulletin. 34 (4): 113–119. Bibcode:2007MPBu...34..113W. ISSN 1052-8091. Retrieved 18 April 2018.
  23. ^ 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.
  24. ^ 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.

External links

  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
  • 173 Ino at AstDyS-2, Asteroids—Dynamic Site
    • Ephemeris · Observation prediction · Orbital info · Proper elements · Observational info
  • 173 Ino at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

minor, planet, designation, large, asteroid, parent, body, family, located, central, regions, asteroid, belt, approximately, kilometers, miles, diameter, discovered, august, 1877, french, astronomer, alphonse, borrelly, marseille, observatory, southern, france. Ino minor planet designation 173 Ino is a large asteroid and the parent body of the Ino family located in the central regions of the asteroid belt approximately 150 kilometers 93 miles in diameter It was discovered on 1 August 1877 by French astronomer Alphonse Borrelly at Marseille Observatory in southern France and named after the queen Ino from Greek mythology 1 2 The dark Xk type asteroid has a rotation period of 6 15 hours 21 173 InoDiscovery 1 Discovered byA BorrellyDiscovery siteMarseilleDiscovery date1 August 1877DesignationsMPC designation 173 InoPronunciation ˈ aɪ n oʊ EYE noh 5 Named afterἸnw inṓ 2 Greek mythology Alternative designationsA877 PA 1922 SBMinor planet categorymain belt 1 3 middle Ino 4 AdjectivesInoan aɪ ˈ n oʊ e n eye NOH en 6 Orbital characteristics 3 Epoch 23 March 2018 JD 2458200 5 Uncertainty parameter 0Observation arc138 75 yr 50 678 d Aphelion3 3142 AUPerihelion2 1708 AUSemi major axis2 7425 AUEccentricity0 2085Orbital period sidereal 4 54 yr 1 659 d Mean anomaly307 27 Mean motion0 13m 1 2s dayInclination14 197 Longitude of ascending node148 18 Argument of perihelion228 89 Physical characteristicsDimensionsc a 0 76 0 06 7 Mean diameter145 3 km 7 119 27 km 8 125 8 1 5 km 9 148 42 km 10 154 1 3 5 km 11 160 6 km 12 Mass 2 2 1 3 1018 kg 7 4 79 3 11 1018 kg 13 Mean density1 4 0 8 g cm3 7 2 23 1 47 g cm3 13 Synodic rotation period5 93 h 14 6 1 0 2 h 15 6 106 0 001 h 15 6 1088 0 0007 h 15 6 11 h 16 6 113 0 002 h 17 6 11651 h 18 6 15 h 19 6 163 h 20 Geometric albedo0 061 calculated 7 0 059 12 0 06 0 02 10 0 0642 0 003 11 0 07 0 05 8 0 096 0 018 9 Spectral typeTholen C 3 SMASS Xk 3 B V 0 705 3 U B 0 305 3 Absolute magnitude H 7 66 3 9 10 11 12 21 7 80 0 05 22 7 90 8 23 Contents 1 Orbit and classification 2 Physical characteristics 3 References 4 External linksOrbit and classification EditIno is the parent body and namesake of the Ino family 522 4 an asteroid family in the intermediate main belt with nearly 500 known members 24 23 The adjectival form of the asteroid name is Inoan It orbits the Sun in the central main belt at a distance of 2 2 3 3 AU once every 4 years and 6 months 1 659 days semi major axis of 2 74 AU Its orbit has an eccentricity of 0 21 and an inclination of 14 with respect to the ecliptic 3 The body s observation arc begins at Dusseldorf Bilk Observatory in January 1879 five months after its official discovery observation at Marseilles 1 Physical characteristics EditIn the Tholen classification Ino is a common carbonaceous C type while in the SMASS classification it is a Xk subtype that transitions between the X type and uncommon K type asteroids 3 Multiple photometric studies of this asteroid were performed between 1978 and 2002 The combined data gave an irregular asymmetrical light curve with a period of 6 163 0 005 hours and a brightness variation of 0 10 0 15 in magnitude The asteroid is rotating in a retrograde direction 18 References Edit a b c d 173 Ino Minor Planet Center Retrieved 18 April 2018 a b Schmadel Lutz D 2007 173 Ino Dictionary of Minor Planet Names 173 Ino Springer Berlin Heidelberg p 30 doi 10 1007 978 3 540 29925 7 174 ISBN 978 3 540 00238 3 a b c d e f g h i JPL Small Body Database Browser 173 Ino 2017 10 21 last obs Jet Propulsion Laboratory Retrieved 18 April 2018 a b Asteroid 173 Ino Small Bodies Data Ferret Retrieved 24 October 2019 Noah Webster 1884 A Practical Dictionary of the English Language George Stuart 1882 The Eclogues Georgics and Moretum of Virgil p 271 a b c d e P Vernazza et al 2021 VLT SPHERE imaging survey of the largest main belt asteroids Final results and synthesis Astronomy amp Astrophysics 54 A56 a b c 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 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 a b c 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 a b c 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 Usui Fumihiko Kuroda Daisuke Muller 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 Carry B December 2012 Density of asteroids Planetary and Space Science 73 1 98 118 arXiv 1203 4336 Bibcode 2012P amp SS 73 98C doi 10 1016 j pss 2012 03 009 See Table 1 Schober H J December 1978 Photometric Variations of the Minor Planets 55 Pandora and 173 Ino during the Opposition in 1977 Light Curves and Rotation Periods Astronomy and Astrophysics Supplement 34 377 Bibcode 1978A amp AS 34 377S Retrieved 18 April 2018 a b c Behrend Raoul Asteroids and comets rotation curves 173 Ino Geneva Observatory Retrieved 18 April 2018 Erikson A December 1989 Improvement of Rotation Periods for the Asteroids 12 Victoria 173 Ino and 1245 Calvinia Asteroids 55 Bibcode 1990acm proc 55E Retrieved 18 April 2018 Gandolfi D Cigna M Fulvio D Blanco C January 2009 CCD and photon counting photometric observations of asteroids carried out at Padova and Catania observatories Planetary and Space Science 57 1 1 9 arXiv 0810 1560 Bibcode 2009P amp SS 57 1G doi 10 1016 j pss 2008 09 014 a b Michalowski T Kaasalainen M Marciniak A Denchev P Kwiatkowski T Kryszczynska A et al November 2005 Photometry and models of selected main belt asteroids II 173 Ino 376 Geometria and 451 Patientia Astronomy and Astrophysics 443 1 329 335 Bibcode 2005A amp A 443 329M doi 10 1051 0004 6361 20053656 Retrieved 18 April 2018 Debehogne H Lagerkvist C I Magnusson P Hahn G December 1989 Physical studies of asteroids XX Photoelectric photometry of asteroids Asteroids 45 Bibcode 1990acm proc 45D Retrieved 18 April 2018 Michalowski Tadeusz December 1993 Poles shapes senses of rotation and sidereal periods of asteroids Icarus 106 2 563 Bibcode 1993Icar 106 563M doi 10 1006 icar 1993 1193 Retrieved 18 April 2018 a b LCDB Data for 173 Ino Asteroid Lightcurve Database LCDB Retrieved 18 April 2018 Warner Brian D December 2007 Initial Results of a Dedicated H G Project The Minor Planet Bulletin 34 4 113 119 Bibcode 2007MPBu 34 113W ISSN 1052 8091 Retrieved 18 April 2018 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 Nesvorny 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 External links EditAsteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend Discovery Circumstances Numbered Minor Planets 1 5000 Minor Planet Center 173 Ino at AstDyS 2 Asteroids Dynamic Site Ephemeris Observation prediction Orbital info Proper elements Observational info 173 Ino at the JPL Small Body Database Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 173 Ino amp oldid 1126710617, wikipedia, wiki, book, books, library,

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