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1864 Daedalus

1864 Daedalus, provisional designation 1971 FA, is a stony asteroid and near-Earth object of the Apollo group, approximately 3 kilometers in diameter. It was discovered on 24 March 1971, by Dutch–American astronomer Tom Gehrels at Palomar Observatory, California, and named after Daedalus from Greek mythology.[4]

1864 Daedalus
Discovery[1]
Discovered byT. Gehrels
Discovery sitePalomar Obs.
Discovery date24 March 1971
Designations
(1864) Daedalus
Pronunciation/ˈdɛdələs/[2]
Named after
Daedalus (Greek mythology)[3]
1971 FA
Apollo · NEO[1][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc46.14 yr (16,854 days)
Aphelion2.3586 AU
Perihelion0.5634 AU
1.4610 AU
Eccentricity0.6144
1.77 yr (645 days)
23.049°
0° 33m 29.16s / day
Inclination22.211°
6.6379°
325.64°
Earth MOID0.2693 AU
Physical characteristics
Dimensions2.722±0.114 km[5]
3.00 km (derived)[6]
3.7 km[7]
8.57 h[8]
8.572 h[9]
8.575±0.002 h[10]
0.20 (assumed)[6]
0.273±0.055[5][7]
SQ (Tholen)[1] · Sr (SMASS)[1]
Sq[11] · S[6]
B–V = 0.830[1]
U–B = 0.500[1]
14.85[1][5] · 14.98[6][9]

Orbit and classification edit

Daedalus is a member of the Apollo asteroids, a group of near-Earth object with an Earth-crossing orbit. It orbits the Sun in the inner main-belt at a distance of 0.6–2.4 AU once every 1 years and 9 months (645 days). Its orbit has an eccentricity of 0.61 and an inclination of 22° with respect to the ecliptic.[1] It has an Earth Minimum orbit intersection distance (MOID) of 0.2693 AU.[1]

Physical characteristics edit

Daedalus is a stony asteroid, characterized as an SQ and Sr spectral type in the Tholen and SMASS taxonomy.[1]

Diameter and albedo edit

According to the survey carried out by NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, it measures 2.7 and 3.7 kilometers in diameter, respectively, and its surface has an albedo of 0.273.[5][7] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and derives a diameter of 3.0 kilometers based on an absolute magnitude of 14.98.[6]

Rotation period edit

Several rotational lightcurves of Daedalus were obtained by astronomers Tom Gehrels, Petr Pravec and Brian Warner. Lightcurve analysis gave a concurring rotation period of 8.572 hours with a high brightness variation of 0.85–1.04 magnitude, indicating a non-spheroidal shape (U=3/3/3).[8][9][10]

Naming edit

This minor planet was named after the Greek mythological figure Daedalus, the builder of King Minos' labyrinth, who was subsequently imprisoned there with his son Icarus. They escaped on wings of feathers and wax, but whereas Icarus was drowned when the wax in his wings melted, Daedalus went on to Sicily and built there a temple to Apollo. There is also a lunar crater called Daedalus.[3] The official naming citation was published by the Minor Planet Center on 20 December 1974 (M.P.C. 3758).[12]

References edit

  1. ^ a b c d e f g h i j k (2017-05-15 last obs.). Jet Propulsion Laboratory. Archived from the original on 20 December 2016. Retrieved 9 June 2017.
  2. ^ "Daedalus". Merriam-Webster.com Dictionary.
  3. ^ a b Schmadel, Lutz D. (2007). "(1864) Daedalus". Dictionary of Minor Planet Names – (1864) Daedalus. Springer Berlin Heidelberg. p. 149. doi:10.1007/978-3-540-29925-7_1865. ISBN 978-3-540-00238-3.
  4. ^ a b "1864 Daedalus (1971 FA)". Minor Planet Center. Retrieved 12 December 2016.
  5. ^ 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.
  6. ^ a b c d e "LCDB Data for (1864) Daedalus". Asteroid Lightcurve Database (LCDB). Retrieved 12 December 2016.
  7. ^ a b c Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results". The Astrophysical Journal. 743 (2): 17. arXiv:1109.6400. Bibcode:2011ApJ...743..156M. doi:10.1088/0004-637X/743/2/156. Retrieved 12 December 2016.
  8. ^ a b Gehrels, T.; Roemer, E.; Marsden, B. G. (September 1971). "Minor Planets and Related Objects. VIL Asteroid 1971 FA". Astronomical Journal. 76: 607. Bibcode:1971AJ.....76..607G. doi:10.1086/111169. Retrieved 12 December 2016.
  9. ^ a b c Pravec, P.; Wolf, M.; Varady, M.; Bárta, P. (December 1995). "CCD Photometry of 6 Near-Earth Asteroids". Earth. 71 (3): 177–187. Bibcode:1995EM&P...71..177P. doi:10.1007/BF00612955. Retrieved 12 December 2016.
  10. ^ a b Warner, Brian D. (July 2015). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2015 January - March". The Minor Planet Bulletin. 42 (3): 172–183. Bibcode:2015MPBu...42..172W. ISSN 1052-8091. Retrieved 12 December 2016.
  11. ^ Thomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014). "Physical characterization of Warm Spitzer-observed near-Earth objects". Icarus. 228: 217–246. arXiv:1310.2000. Bibcode:2014Icar..228..217T. doi:10.1016/j.icarus.2013.10.004. Retrieved 12 December 2016.
  12. ^ Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs". Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221. doi:10.1007/978-3-642-01965-4. ISBN 978-3-642-01964-7.

External links edit

  • 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
  • 1864 Daedalus at NeoDyS-2, Near Earth Objects—Dynamic Site
    • Ephemerides · Observation prediction · Orbital info · MOID · Proper elements · Observational info · Close approaches · Physical info · Orbit animation
  • 1864 Daedalus at ESA–space situational awareness
    • Ephemerides · Observations · Orbit · Physical properties · Summary
  • 1864 Daedalus at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

1864, daedalus, provisional, designation, 1971, stony, asteroid, near, earth, object, apollo, group, approximately, kilometers, diameter, discovered, march, 1971, dutch, american, astronomer, gehrels, palomar, observatory, california, named, after, daedalus, f. 1864 Daedalus provisional designation 1971 FA is a stony asteroid and near Earth object of the Apollo group approximately 3 kilometers in diameter It was discovered on 24 March 1971 by Dutch American astronomer Tom Gehrels at Palomar Observatory California and named after Daedalus from Greek mythology 4 1864 DaedalusDiscovery 1 Discovered byT GehrelsDiscovery sitePalomar Obs Discovery date24 March 1971DesignationsMPC designation 1864 DaedalusPronunciation ˈ d ɛ d e l e s 2 Named afterDaedalus Greek mythology 3 Alternative designations1971 FAMinor planet categoryApollo NEO 1 4 Orbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc46 14 yr 16 854 days Aphelion2 3586 AUPerihelion0 5634 AUSemi major axis1 4610 AUEccentricity0 6144Orbital period sidereal 1 77 yr 645 days Mean anomaly23 049 Mean motion0 33m 29 16s dayInclination22 211 Longitude of ascending node6 6379 Argument of perihelion325 64 Earth MOID0 2693 AUPhysical characteristicsDimensions2 722 0 114 km 5 3 00 km derived 6 3 7 km 7 Synodic rotation period8 57 h 8 8 572 h 9 8 575 0 002 h 10 Geometric albedo0 20 assumed 6 0 273 0 055 5 7 Spectral typeSQ Tholen 1 Sr SMASS 1 Sq 11 S 6 B V 0 830 1 U B 0 500 1 Absolute magnitude H 14 85 1 5 14 98 6 9 Contents 1 Orbit and classification 2 Physical characteristics 2 1 Diameter and albedo 2 2 Rotation period 3 Naming 4 References 5 External linksOrbit and classification editDaedalus is a member of the Apollo asteroids a group of near Earth object with an Earth crossing orbit It orbits the Sun in the inner main belt at a distance of 0 6 2 4 AU once every 1 years and 9 months 645 days Its orbit has an eccentricity of 0 61 and an inclination of 22 with respect to the ecliptic 1 It has an Earth Minimum orbit intersection distance MOID of 0 2693 AU 1 Physical characteristics editDaedalus is a stony asteroid characterized as an SQ and Sr spectral type in the Tholen and SMASS taxonomy 1 Diameter and albedo edit According to the survey carried out by NASA s Wide field Infrared Survey Explorer with its subsequent NEOWISE mission it measures 2 7 and 3 7 kilometers in diameter respectively and its surface has an albedo of 0 273 5 7 The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0 20 and derives a diameter of 3 0 kilometers based on an absolute magnitude of 14 98 6 Rotation period edit Several rotational lightcurves of Daedalus were obtained by astronomers Tom Gehrels Petr Pravec and Brian Warner Lightcurve analysis gave a concurring rotation period of 8 572 hours with a high brightness variation of 0 85 1 04 magnitude indicating a non spheroidal shape U 3 3 3 8 9 10 Naming editThis minor planet was named after the Greek mythological figure Daedalus the builder of King Minos labyrinth who was subsequently imprisoned there with his son Icarus They escaped on wings of feathers and wax but whereas Icarus was drowned when the wax in his wings melted Daedalus went on to Sicily and built there a temple to Apollo There is also a lunar crater called Daedalus 3 The official naming citation was published by the Minor Planet Center on 20 December 1974 M P C 3758 12 References edit a b c d e f g h i j k JPL Small Body Database Browser 1864 Daedalus 1971 FA 2017 05 15 last obs Jet Propulsion Laboratory Archived from the original on 20 December 2016 Retrieved 9 June 2017 Daedalus Merriam Webster com Dictionary a b Schmadel Lutz D 2007 1864 Daedalus Dictionary of Minor Planet Names 1864 Daedalus Springer Berlin Heidelberg p 149 doi 10 1007 978 3 540 29925 7 1865 ISBN 978 3 540 00238 3 a b 1864 Daedalus 1971 FA Minor Planet Center Retrieved 12 December 2016 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 c d e LCDB Data for 1864 Daedalus Asteroid Lightcurve Database LCDB Retrieved 12 December 2016 a b c Mainzer A Grav T Bauer J Masiero J McMillan R S Cutri R M et al December 2011 NEOWISE Observations of Near Earth Objects Preliminary Results The Astrophysical Journal 743 2 17 arXiv 1109 6400 Bibcode 2011ApJ 743 156M doi 10 1088 0004 637X 743 2 156 Retrieved 12 December 2016 a b Gehrels T Roemer E Marsden B G September 1971 Minor Planets and Related Objects VIL Asteroid 1971 FA Astronomical Journal 76 607 Bibcode 1971AJ 76 607G doi 10 1086 111169 Retrieved 12 December 2016 a b c Pravec P Wolf M Varady M Barta P December 1995 CCD Photometry of 6 Near Earth Asteroids Earth 71 3 177 187 Bibcode 1995EM amp P 71 177P doi 10 1007 BF00612955 Retrieved 12 December 2016 a b Warner Brian D July 2015 Near Earth Asteroid Lightcurve Analysis at CS3 Palmer Divide Station 2015 January March The Minor Planet Bulletin 42 3 172 183 Bibcode 2015MPBu 42 172W ISSN 1052 8091 Retrieved 12 December 2016 Thomas Cristina A Emery Joshua P Trilling David E Delbo Marco Hora Joseph L Mueller Michael January 2014 Physical characterization of Warm Spitzer observed near Earth objects Icarus 228 217 246 arXiv 1310 2000 Bibcode 2014Icar 228 217T doi 10 1016 j icarus 2013 10 004 Retrieved 12 December 2016 Schmadel Lutz D 2009 Appendix Publication Dates of the MPCs Dictionary of Minor Planet Names Addendum to Fifth Edition 2006 2008 Springer Berlin Heidelberg p 221 doi 10 1007 978 3 642 01965 4 ISBN 978 3 642 01964 7 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 1864 Daedalus at NeoDyS 2 Near Earth Objects Dynamic Site Ephemerides Observation prediction Orbital info MOID Proper elements Observational info Close approaches Physical info Orbit animation 1864 Daedalus at ESA space situational awareness Ephemerides Observations Orbit Physical properties Summary 1864 Daedalus at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 1864 Daedalus amp oldid 1190801918, wikipedia, wiki, book, books, library,

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