Hubble Space Telescope image of Typhon and its moon Echidna, taken in 2006 | |
Discovery | |
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Discovered by | NEAT |
Discovery date | 5 February 2002 |
Designations | |
MPC designation | (42355) Typhon |
Pronunciation | /ˈtaɪfɒn/ |
Named after | Τυφών Typhōn |
Alternative designations | 2002 CR46 |
Minor planet category | SDO Centaur |
Adjectives | Typhonian /taɪˈfoʊniən/ |
Orbital characteristics | |
Epoch 13 January 2016 (JD 2457400.5) | |
Uncertainty parameter 2 | |
Observation arc | 9563 days (26.18 yr) |
Aphelion | 58.982252 AU (8.8236193 Tm) |
Perihelion | 17.545721 AU (2.6248025 Tm) |
Semi-major axis | 38.263987 AU (5.7242110 Tm) |
Eccentricity | 0.5414560 |
Orbital period (sidereal) | 236.70 yr (86453.7 d) |
Mean anomaly | 14.61898075° |
Mean motion | 0° 0 14.991 / day |
Inclination | 2.4252078° |
Longitude of ascending node | 351.9098598° |
Argument of perihelion | 159.3215723° |
Known satellites | 1 (Echidna) |
TJupiter | 4.692 |
Physical characteristics | |
Mean diameter | 138±9 km 162±7 km |
Mass | ≈9.082×10 kg |
Mean density | 0.66+0.09 −0.08 g/cm |
Synodic rotation period | 9.67 h (0.403 d) |
Geometric albedo | 0.044±0.003 0.10±0.02 |
Spectral type | B−V=0.74±0.02 V−R=0.52±0.01 |
Absolute magnitude (H) | 7.5 |
42355 Typhon (/ˈtaɪfɒn/; provisional designation 2002 CR46) is a scattered disc object that was discovered on February 5, 2002, by the NEAT program. It measures 162±7 km in diameter, and is named after Typhon, a monster in Greek mythology.
Typhon is the first known binary centaur, using an extended definition of a centaur as an object on a non-resonant (unstable) orbit with the perihelion inside the orbit of Neptune.
Physical properties
Typhon has a BR taxonomic class, with a blue surface. It has a resulting B–R magnitude of 1.274.
Based on a conventional magnitude-to-diameter conversion, the body measures 162 km in diameter, with an albedo of 0.044 and a magnitude of 7.5. Mike Brown gives it a diameter of 192 km with a magnitude of 7.5. Due to its small size, it is unlikely to be classified as a dwarf planet. As of 2021, no rotational lightcurve has been analyzed. The body's rotational period, pole, and actual shape remain unknown.
Moon
Discovery | |
---|---|
Discovery date | 2006 |
Designations | |
MPC designation | (42355) Typhon I Echidna |
Pronunciation | /ɪˈkɪdnə/ |
Named after | Έχιδνα |
Adjectives | Echidnian Echidnean (rarely) (both /ɪˈkɪdniən/) |
Orbital characteristics | |
Semi-major axis | ~1300 km |
Orbital period (sidereal) | 11 d |
Satellite of | Typhon |
Physical characteristics | |
Dimensions | 89±6 km |
A large moon was identified in 2006. It is named Echidna (formal designation (42355) Typhon I Echidna), after the monstrous mate of Typhon. It orbits Typhon at ~1300 km, completing one orbit in about 11 days. Its diameter is estimated to be 89±6 km.
References
- "Typhon". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ "JPL Small-Body Database Browser: (42355 Typhon)" (2008-03-14 last obs). Retrieved 12 April 2016.
- "List Of Centaurs and Scattered-Disk Objects". Minor Planet Center. Retrieved 2008-09-21.
- (42355) Typhon and Echidna
- "Typhonian". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- ^ Duffard, R.; Pinilla-Alonso, N.; Santos-Sanz, P.; Vilenius, E.; Ortiz, J. L.; Mueller, T.; et al. (April 2014). ""TNOs are Cool": A survey of the trans-Neptunian region. XI. A Herschel-PACS view of 16 Centaurs". Astronomy and Astrophysics. 564: 17. arXiv:1309.0946. Bibcode:2014A&A...564A..92D. doi:10.1051/0004-6361/201322377. S2CID 119177446.
- ^ Santos-Sanz, P., Lellouch, E., Fornasier, S., Kiss, C., Pal, A., Müller, T. G., Vilenius, E., Stansberry, J., Mommert, M., Delsanti, A., Mueller, M., Peixinho, N., Henry, F., Ortiz, J. L., Thirouin, A., Protopapa, S., Duffard, R., Szalai, N., Lim, T., Ejeta, C., Hartogh, P., Harris, A. W., & Rengel, M. (2012). “TNOs are Cool”: A Survey of the Transneptunian Region IV - Size/albedo characterization of 15 scattered disk and detached objects observed with Herschel Space Observatory-PACS
- K. Noll; H. Levison; W. Grundy; D. Stephens (October 2006). "Discovery of a binary Centaur". Icarus. 184 (2): 611. arXiv:astro-ph/0605606. Bibcode:2006Icar..184..611N. doi:10.1016/j.icarus.2006.05.010. S2CID 18927838.
- J. L. Elliot; S. D. Kern; K. B. Clancy; A. A. S. Gulbis; R. L. Millis; M. W. Buie; et al. (February 2005). "The Deep Ecliptic Survey: A Search for Kuiper Belt Objects and Centaurs. II. Dynamical Classification, the Kuiper Belt Plane, and the Core Population" (PDF). The Astronomical Journal. 129 (2): 1117. Bibcode:2005AJ....129.1117E. doi:10.1086/427395.
- "Echidna". Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription or participating institution membership required.)
- François Hartog (Janet Lloyd, trans., 1988) The Mirror of Herodotus, p. 25
- J. A. Weinstock (2014) The Ashgate Encyclopedia of Literary and Cinematic Monsters, p. 79
- George Sandys (1669) Ovid's Metamorphosis Englished, 6th ed., p. 134.
External links
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