 Orbital diagram (top view) | |
| Discovery [1] | |
|---|---|
| Discovered by | NEAT |
| Discovery site | Palomar |
| Discovery date | 8 April 2002 |
| Designations | |
| (55576) Amycus | |
| Pronunciation | /ˈæmɪkəs/ [2] |
Named after | Amycus |
| 2002 GB10 | |
| Centaur [1] [3] | |
| Adjectives | Amycian /əˈmɪsiən/ |
| Symbol |
.svg){kind=small} (astrological) |
| Orbital characteristics [1] | |
| Epoch 13 January 2016 ( JD 2457400.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 7204 days (19.72 yr) |
| Aphelion | 35.019 AU (5.2388 Tm) (Q) |
| Perihelion | 15.178 AU (2.2706 Tm) (q) |
| 25.098 AU (3.7546 Tm) (a) | |
| Eccentricity | 0.39526 (e) |
| 125.74 yr (45926.7 d) | |
| 37.041 ° (M) | |
| 0° 0m 28.219s / day (n) | |
| Inclination | 13.352° (i) |
| 315.45° (Ω) | |
| 239.17° (ω) | |
| Jupiter MOID | 9.92261 AU (1.484401 Tm) |
| TJupiter | 4.133 |
| Physical characteristics | |
| Dimensions | 76.3±12.5 km [4] [5] |
| 9.76 h (0.407 d) | |
| ~ 0.18 [4] | |
| ~ 20 [7] | |
| 7.8 [1] | |
55576 Amycus /ˈæmɪkəs/ is a centaur discovered on 8 April 2002 by the NEAT at Palomar. [1]
The minor planet was named for Amycus, a male centaur in Greek mythology.
It came to perihelion in February 2003. [1] Data from the Spitzer Space Telescope gave a diameter of 76.3±12.5 km. [4] [5]
A low probability asteroid occultation of star UCAC2 17967364 with an apparent magnitude of +13.8 was possible on 11 February 2009. [8] Another such event involving a star with an apparent magnitude of +12.9 occurred on 10 April 2014 at about 10:46 Universal Time, visible for observers in the southwest US and western Mexico. [9]
Near 3:4 resonance of Uranus
Amycus (2002 GB10) lies within 0.009 AU of the 3:4 resonance of Uranus and is estimated to have a long orbital half-life of about 11.1 Myr. [10] [11]
See also
References
- ^ a b c d e f "JPL Small-Body Database Browser: 55576 Amycus (2002 GB10)" (2007-08-15 last obs). Retrieved 12 April 2016.
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ Marc W. Buie. "Orbit Fit and Astrometric record for 55576" (2003-06-22 using 73 of 81 observations). SwRI (Space Science Department). Archived from the original on 4 June 2011. Retrieved 28 February 2009.
- ^ a b c John Stansberry; Will Grundy; Mike Brown; Dale Cruikshank; John Spencer; David Trilling; Jean-Luc Margot (20 February 2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". arXiv: astro-ph/0702538.
- ^ a b Wm. Robert Johnston (22 August 2008). "List of Known Trans-Neptunian Objects". Johnston's Archive. Archived from the original on 13 February 2009. Retrieved 28 February 2009.
- ^ a b Hainaut, O. R.; Boehnhardt, H.; Protopapa, S. (October 2012). "Colours of minor bodies in the outer solar system. II. A statistical analysis revisited". Astronomy and Astrophysics. 546: 20. arXiv: 1209.1896. Bibcode: 2012A&A...546A.115H. doi: 10.1051/0004-6361/201219566. S2CID 54776793. Retrieved 26 September 2019.
- ^ "AstDys (55576) Amycus Ephemerides". Department of Mathematics, University of Pisa, Italy. Archived from the original on 26 May 2011. Retrieved 15 March 2009.
- ^ Steve Preston (8 January 2009). "Star occultation by asteroid 55576 Amycus". IOTA (International Occultation Timing Association). Retrieved 28 December 2009.[ dead link]
-
^ Hans-J. Bode; Filipe Braga Ribas; B. Sicardy (2013). "Bright Star Occultations by TNOs in 2014. J. Occultation Astronomy 2014-1". IOTA (International Occultation Timing Association).
{{ cite journal}}: Cite journal requires|journal=( help) - ^ Horner, J.; Evans, N.W.; Bailey, M. E. (2004). "Simulations of the Population of Centaurs I: The Bulk Statistics". Monthly Notices of the Royal Astronomical Society. 354 (3): 798–810. arXiv: astro-ph/0407400. Bibcode: 2004MNRAS.354..798H. doi: 10.1111/j.1365-2966.2004.08240.x. S2CID 16002759.
- ^ Showalter, Mark R.; Benecchi, Susan D.; Buie, Marc W.; Grundy, William M.; Keane, James T.; Lisse, Carey M.; Olkin, Cathy B.; Porter, Simon B.; Robbins, Stuart J.; Singer, Kelsi N.; Verbiscer, Anne J.; Weaver, Harold A.; Zangari, Amanda M.; Hamilton, Douglas P.; Kaufmann, David E. (2021). "A statistical review of light curves and the prevalence of contact binaries in the Kuiper Belt". Icarus. 356: 114098. arXiv: 2105.03543. doi: 10.1016/j.icarus.2020.114098. S2CID 225284888.
External links
|
Orbital diagram (top view) | |
| Discovery [1] | |
|---|---|
| Discovered by | NEAT |
| Discovery site | Palomar |
| Discovery date | 8 April 2002 |
| Designations | |
| (55576) Amycus | |
| Pronunciation | /ˈæmɪkəs/ [2] |
Named after | Amycus |
| 2002 GB10 | |
| Centaur [1] [3] | |
| Adjectives | Amycian /əˈmɪsiən/ |
| Symbol |
(astrological) |
| Orbital characteristics [1] | |
| Epoch 13 January 2016 ( JD 2457400.5) | |
| Uncertainty parameter 2 | |
| Observation arc | 7204 days (19.72 yr) |
| Aphelion | 35.019 AU (5.2388 Tm) (Q) |
| Perihelion | 15.178 AU (2.2706 Tm) (q) |
| 25.098 AU (3.7546 Tm) (a) | |
| Eccentricity | 0.39526 (e) |
| 125.74 yr (45926.7 d) | |
| 37.041 ° (M) | |
| 0° 0m 28.219s / day (n) | |
| Inclination | 13.352° (i) |
| 315.45° (Ω) | |
| 239.17° (ω) | |
| Jupiter MOID | 9.92261 AU (1.484401 Tm) |
| TJupiter | 4.133 |
| Physical characteristics | |
| Dimensions | 76.3±12.5 km [4] [5] |
| 9.76 h (0.407 d) | |
| ~ 0.18 [4] | |
| ~ 20 [7] | |
| 7.8 [1] | |
55576 Amycus /ˈæmɪkəs/ is a centaur discovered on 8 April 2002 by the NEAT at Palomar. [1]
The minor planet was named for Amycus, a male centaur in Greek mythology.
It came to perihelion in February 2003. [1] Data from the Spitzer Space Telescope gave a diameter of 76.3±12.5 km. [4] [5]
A low probability asteroid occultation of star UCAC2 17967364 with an apparent magnitude of +13.8 was possible on 11 February 2009. [8] Another such event involving a star with an apparent magnitude of +12.9 occurred on 10 April 2014 at about 10:46 Universal Time, visible for observers in the southwest US and western Mexico. [9]
Near 3:4 resonance of Uranus
Amycus (2002 GB10) lies within 0.009 AU of the 3:4 resonance of Uranus and is estimated to have a long orbital half-life of about 11.1 Myr. [10] [11]
See also
References
- ^ a b c d e f "JPL Small-Body Database Browser: 55576 Amycus (2002 GB10)" (2007-08-15 last obs). Retrieved 12 April 2016.
- ^ Noah Webster (1884) A Practical Dictionary of the English Language
- ^ Marc W. Buie. "Orbit Fit and Astrometric record for 55576" (2003-06-22 using 73 of 81 observations). SwRI (Space Science Department). Archived from the original on 4 June 2011. Retrieved 28 February 2009.
- ^ a b c John Stansberry; Will Grundy; Mike Brown; Dale Cruikshank; John Spencer; David Trilling; Jean-Luc Margot (20 February 2007). "Physical Properties of Kuiper Belt and Centaur Objects: Constraints from Spitzer Space Telescope". arXiv: astro-ph/0702538.
- ^ a b Wm. Robert Johnston (22 August 2008). "List of Known Trans-Neptunian Objects". Johnston's Archive. Archived from the original on 13 February 2009. Retrieved 28 February 2009.
- ^ a b Hainaut, O. R.; Boehnhardt, H.; Protopapa, S. (October 2012). "Colours of minor bodies in the outer solar system. II. A statistical analysis revisited". Astronomy and Astrophysics. 546: 20. arXiv: 1209.1896. Bibcode: 2012A&A...546A.115H. doi: 10.1051/0004-6361/201219566. S2CID 54776793. Retrieved 26 September 2019.
- ^ "AstDys (55576) Amycus Ephemerides". Department of Mathematics, University of Pisa, Italy. Archived from the original on 26 May 2011. Retrieved 15 March 2009.
- ^ Steve Preston (8 January 2009). "Star occultation by asteroid 55576 Amycus". IOTA (International Occultation Timing Association). Retrieved 28 December 2009.[ dead link]
-
^ Hans-J. Bode; Filipe Braga Ribas; B. Sicardy (2013). "Bright Star Occultations by TNOs in 2014. J. Occultation Astronomy 2014-1". IOTA (International Occultation Timing Association).
{{ cite journal}}: Cite journal requires|journal=( help) - ^ Horner, J.; Evans, N.W.; Bailey, M. E. (2004). "Simulations of the Population of Centaurs I: The Bulk Statistics". Monthly Notices of the Royal Astronomical Society. 354 (3): 798–810. arXiv: astro-ph/0407400. Bibcode: 2004MNRAS.354..798H. doi: 10.1111/j.1365-2966.2004.08240.x. S2CID 16002759.
- ^ Showalter, Mark R.; Benecchi, Susan D.; Buie, Marc W.; Grundy, William M.; Keane, James T.; Lisse, Carey M.; Olkin, Cathy B.; Porter, Simon B.; Robbins, Stuart J.; Singer, Kelsi N.; Verbiscer, Anne J.; Weaver, Harold A.; Zangari, Amanda M.; Hamilton, Douglas P.; Kaufmann, David E. (2021). "A statistical review of light curves and the prevalence of contact binaries in the Kuiper Belt". Icarus. 356: 114098. arXiv: 2105.03543. doi: 10.1016/j.icarus.2020.114098. S2CID 225284888.