16 Psyche
 NAHHHH BLUD THIS PAGE IS FROM OHIO 💀💀💀😭 |
16 Psyche is a very big Main belt asteroid, well over 200 kilometers in diameter, and likely the biggest of the metallic M-type asteroids. It is estimated to have 0.6 percent of the mass of the entire asteroid belt.[1]
This asteroid was found by Annibale de Gasparis on March 17, 1852 from Naples and named after the Greek nymph Psyche. The first fifteen asteroids to be found were given symbols by astronomers as a type of short-hand notation. In 1851, however, J. F. Encke suggested using a circled number. 16 Psyche was the first new asteroid to be found that was designated with this scheme (in 1852 by J. Ferguson).[2]
Characteristics change
Radar[3][4] observations indicate that it is made of iron-nickel. Psyche appears to be a case of an exposed metallic core from a bigger differentiated parent body. Unlike some other M-type asteroids, Psyche shows no sign of the presence of water or water-bearing minerals on its surface, consistent with its interpretation as a metallic body.[5] Small amounts of pyroxene appear to be present.[6]
If Psyche is the core remnant of a bigger parent body, we might expect other asteroids on similar orbits. Psyche does not belong to any asteroid family.[7] One theory is that the collision occurred very early in the solar system's history, and all the other remnants have since been ground into fragments by subsequent collisions or had their orbits perturbed beyond recognition.
Psyche is massive enough that its perturbations on other asteroids can be measured, which enables a mass measurement. Its density is fairly low for metal (although fairly common for asteroids as such), indicating a fairly high porosity of 30–40%.[8]
Psyche appears to have a fairly round surface and is approximately ellipsoidal in shape. Recent lightcurve analysis indicates that its pole points towards either ecliptic coordinates (β, λ) = (-9°, 35°) or (β, λ) = (-2°, 215°) with a 10° uncertainty.[9] This gives an axial tilt of 95°.
Two stellar occultations by Psyche have been seen (from Mexico on March 22, 2002, and another on May 16, 2002). Lightcurve changes indicate a non-spherical body, consistent with the lightcurve and radar results.
References change
- ↑ B. Vitaeau (2000). "Mass and density of asteroids (16) Psyche and (121) Hermione" (PDF). Astronomy & Astrophysics. 354: 725. Bibcode:2000A&A...354..725V. Archived from the original (PDF) on 2007-09-29. Retrieved 2007-12-18.
- ↑ Hilton, J. (September 17, 2001). "When Did the Asteroids Become Minor Planets?". U.S. Naval Observatory. Archived from the original on 2007-06-24. Retrieved 2007-04-03.
- ↑ S.J. Ostro (1985). "Radar observations of asteroids and comets" (PDF). Astronomical Society of the Pacific, Publications. 97: 877. Bibcode:1985PASP...97..877O. doi:10.1086/131619. S2CID 120491725.
- ↑ C. Magri; et al. (1999). "Mainbelt Asteroids: Results of Arecibo and Goldstone Radar Observations of 37 Objects during 1980-1995". Icarus. 140 (2): 379. Bibcode:1999Icar..140..379M. doi:10.1006/icar.1999.6130.
- ↑ E. Merényi; et al. (1997). "Prediction of Water in Asteroids from Spectral Data Shortward of 3 µm". Icarus. 129 (2): 421. Bibcode:1997Icar..129..421M. doi:10.1006/icar.1997.5796.
- ↑ P.S. Hardersen, M.J. Gaffey, and P.A. Abell (2005). "Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids". Icarus. 175 (1): 141. Bibcode:2005Icar..175..141H. doi:10.1016/j.icarus.2004.10.017.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ↑ D.R. Davis, P. Farinella, & M. Francesco (1999). "The Missing Psyche Family: Collisionally Eroded or Never Formed?". Icarus. 137 (1): 140. Bibcode:1999Icar..137..140D. doi:10.1006/icar.1998.6037.
{{cite journal}}: CS1 maint: multiple names: authors list (link) - ↑ Cite error: The named reference
Lupishko1999was used but no text was provided for refs named (see the help page). - ↑ Cite error: The named reference
Kaasalainen02was used but no text was provided for refs named (see the help page).
Other websites change
- Shape model deduced from lightcurve Archived 2008-02-16 at the Wayback Machine (PDF)
- Occultation of TYC 5783-1228 by 16 Psyche Archived 2007-12-27 at the Wayback Machine (Video)
- Orbital simulation from JPL (Java) / Ephemeris