Detection of water and/or hydroxyl on asteroid (16) Psyche

NASA [NNH14CK55B]; Eugene M. Shoemaker Postdoctoral Fellowship (NASA Planetary Geology and Geophysics Program); NASA Planetary Geology and Geophysics grants [NNX14AN05G, NNX14AN35G]; NASA Solar System Observing grant [NNX16AE91G]

[1]  Lance A. M. Benner,et al.  A radar survey of M- and X-class asteroids , 2008 .

[2]  B. Clark,et al.  Spectroscopic survey of M-type asteroids , 2010, 1007.2582.

[3]  Driss Takir,et al.  Outer Main Belt asteroids: Identification and distribution of four 3-μm spectral groups , 2011 .

[4]  Alessandro Morbidelli,et al.  Iron meteorites as remnants of planetesimals formed in the terrestrial planet region , 2006, Nature.

[5]  Alan W. Harris,et al.  A Thermal Model for Near-Earth Asteroids , 1998 .

[6]  E. Cloutis,et al.  The M‐/X‐asteroid menagerie: Results of an NIR spectral survey of 45 main‐belt asteroids , 2011 .

[7]  Daniel J. Scheeres,et al.  Radar observations and a physical model of Asteroid 1580 Betulia , 2007 .

[8]  M. Shepard,et al.  Radar observations of Asteroids 64 Angelina and 69 Hesperia , 2011 .

[9]  L. Lebofsky Asteroid 1 Ceres - Evidence for water of hydration , 1978 .

[10]  Lori M. Feaga,et al.  Temporal and Spatial Variability of Lunar Hydration As Observed by the Deep Impact Spacecraft , 2009, Science.

[11]  David E. Trilling,et al.  Online multi-parameter phase-curve fitting and application to a large corpus of asteroid photometric data , 2011 .

[12]  Francesco Marzari,et al.  The Missing Psyche Family: Collisionally Eroded or Never Formed? , 1999 .

[13]  Larry A. Lebofsky,et al.  The composition and origin of the C, P, and D asteroids: Water as a tracer of thermal evolution in the outer belt , 1990 .

[14]  Richard P. Binzel,et al.  An extension of the Bus asteroid taxonomy into the near-infrared , 2009 .

[15]  Roger N. Clark,et al.  Detection of Adsorbed Water and Hydroxyl on the Moon , 2009, Science.

[16]  The composition of M-type asteroids: Synthesis of spectroscopic and radar observations , 2010 .

[17]  D. Lupishko,et al.  On the bulk density of the M-type asteroid 16 Psyche , 2006 .

[18]  N. Pinilla-Alonso,et al.  A new investigation of hydration in the M-type asteroids , 2015 .

[19]  H. McSween,et al.  Toward an understanding of phyllosilicate mineralogy in the outer main asteroid belt , 2015 .

[20]  J. Conklin,et al.  The composition of M-type asteroids II: Synthesis of spectroscopic and radar observations , 2010 .

[21]  John T. Rayner,et al.  SpeX: A Medium‐Resolution 0.8–5.5 Micron Spectrograph and Imager for the NASA Infrared Telescope Facility , 2003 .

[22]  A. Kovačević,et al.  Motion of the asteroid (13206) 1997GC22 and the mass of (16) Psyche , 2002 .

[23]  Paul A. Abell,et al.  Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids , 2005 .

[24]  V. Reddy,et al.  PHASE ANGLE EFFECTS ON 3 μm ABSORPTION BAND ON CERES: IMPLICATIONS FOR DAWN MISSION , 2015, 1504.02678.

[25]  John T. Rayner,et al.  Four years of good SpeX , 2004, SPIE Astronomical Telescopes + Instrumentation.

[26]  Karri Muinonen,et al.  A three-parameter magnitude phase function for asteroids , 2010 .

[27]  J. Taylor An Introduction to Error Analysis , 1982 .

[28]  C. Russell,et al.  Delivery of dark material to Vesta via carbonaceous chondritic impacts , 2012, 1208.2833.

[29]  M. Shepard,et al.  Compositional characterization of asteroid (16) Psyche , 2016 .

[30]  Richard P. Binzel,et al.  Phase II of the Small Main-Belt Asteroid Spectroscopic Survey: A Feature-Based Taxonomy , 2002 .

[31]  Erik Asphaug,et al.  Hit-and-run planetary collisions , 2006, Nature.

[32]  Harry Y. McSween,et al.  Nature and degree of aqueous alteration in CM and CI carbonaceous chondrites , 2013 .

[33]  Sebastiano Ligori,et al.  Evidence of a metal-rich surface for the asteroid (16) Psyche from interferometric observations in the thermal infrared , 2013, 1306.2455.

[34]  Andrew Scott Rivkin,et al.  Brucite and carbonate assemblages from altered olivine-rich materials on Ceres , 2009 .

[35]  W. Hartmann,et al.  Asteroids - The big picture , 1989 .

[36]  John T. Rayner,et al.  Spextool: A Spectral Extraction Package for SpeX, a 0.8–5.5 Micron Cross‐Dispersed Spectrograph , 2004 .

[37]  R. Jaumann,et al.  Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres , 2015, Nature.

[38]  Andrew Scott Rivkin,et al.  The Nature of M-Class Asteroids from 3-μm Observations☆ , 2000 .

[39]  D. Tholen,et al.  Asteroid Taxonomy from Cluster Analysis of Photometry. , 1984 .

[40]  Richard J. Rudy,et al.  A refined “standard” thermal model for asteroids based on observations of 1 Ceres and 2 Pallas , 1986 .

[41]  M. D. Dyar,et al.  Character and Spatial Distribution of OH/H2O on the Surface of the Moon Seen by M3 on Chandrayaan-1 , 2009, Science.