DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE

The asteroid (16) Psyche is of scientific interest because it contains similar to 1% of the total mass of the asteroid belt and is thought to be the remnant metallic core of a protoplanet. Radar observations have indicated the significant presence of metal on the surface with a small percentage of s...

Full description

Bibliographic Details
Main Authors: Sanchez, Juan A., Reddy, Vishnu, Shepard, Michael K., Thomas, Cristina, Cloutis, Edward A., Takir, Driss, Conrad, Albert, Kiddell, Cain, Applin, Daniel
Other Authors: Univ Arizona, LBT Observ
Language:en
Published: IOP PUBLISHING LTD 2016
Subjects:
Online Access:http://hdl.handle.net/10150/622750
http://arizona.openrepository.com/arizona/handle/10150/622750
id ndltd-arizona.edu-oai-arizona.openrepository.com-10150-622750
record_format oai_dc
spelling ndltd-arizona.edu-oai-arizona.openrepository.com-10150-6227502017-03-04T03:00:46Z DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE Sanchez, Juan A. Reddy, Vishnu Shepard, Michael K. Thomas, Cristina Cloutis, Edward A. Takir, Driss Conrad, Albert Kiddell, Cain Applin, Daniel Univ Arizona, LBT Observ Univ Arizona, Lunar & Planetary Lab minor planets asteroids: general techniques: spectroscopic The asteroid (16) Psyche is of scientific interest because it contains similar to 1% of the total mass of the asteroid belt and is thought to be the remnant metallic core of a protoplanet. Radar observations have indicated the significant presence of metal on the surface with a small percentage of silicates. Prior ground-based observations showed rotational variations in the near-infrared (NIR) spectra and radar albedo of this asteroid. However, no comprehensive study that combines multi-wavelength data has been conducted so far. Here we present rotationally resolved NIR spectra (0.7-2.5 mu m) of (16) Psyche obtained with the NASA Infrared Telescope Facility. These data have been combined with shape models of the asteroid for each rotation phase. Spectral band parameters extracted from the NIR spectra show that the pyroxene band center varies from similar to 0.92 to 0.94 mu m. Band center values were used to calculate the pyroxene chemistry of the asteroid, whose average value was found to be Fs(30)En(65)Wo(5). Variations in the band depth (BD) were also observed, with values ranging from 1.0% to 1.5%. Using a new laboratory spectral calibration method, we estimated an average orthopyroxene content of 6% +/- 1%. The mass-deficit region of Psyche, which exhibits the highest radar albedo, also shows the highest value for the spectral slope and the minimum BD. The spectral characteristics of Psyche suggest that its parent body did not have the typical structure expected for a differentiated body or that the sequence of events that led to its current state was more complex than previously thought. 2016-12-28 Article DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE 2016, 153 (1):29 The Astronomical Journal 1538-3881 10.3847/1538-3881/153/1/29 http://hdl.handle.net/10150/622750 http://arizona.openrepository.com/arizona/handle/10150/622750 The Astronomical Journal en http://stacks.iop.org/1538-3881/153/i=1/a=29?key=crossref.26de63d3d798b379b85ded354bf80521 © 2016. The American Astronomical Society. All rights reserved. IOP PUBLISHING LTD
collection NDLTD
language en
sources NDLTD
topic minor planets
asteroids: general
techniques: spectroscopic
spellingShingle minor planets
asteroids: general
techniques: spectroscopic
Sanchez, Juan A.
Reddy, Vishnu
Shepard, Michael K.
Thomas, Cristina
Cloutis, Edward A.
Takir, Driss
Conrad, Albert
Kiddell, Cain
Applin, Daniel
DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE
description The asteroid (16) Psyche is of scientific interest because it contains similar to 1% of the total mass of the asteroid belt and is thought to be the remnant metallic core of a protoplanet. Radar observations have indicated the significant presence of metal on the surface with a small percentage of silicates. Prior ground-based observations showed rotational variations in the near-infrared (NIR) spectra and radar albedo of this asteroid. However, no comprehensive study that combines multi-wavelength data has been conducted so far. Here we present rotationally resolved NIR spectra (0.7-2.5 mu m) of (16) Psyche obtained with the NASA Infrared Telescope Facility. These data have been combined with shape models of the asteroid for each rotation phase. Spectral band parameters extracted from the NIR spectra show that the pyroxene band center varies from similar to 0.92 to 0.94 mu m. Band center values were used to calculate the pyroxene chemistry of the asteroid, whose average value was found to be Fs(30)En(65)Wo(5). Variations in the band depth (BD) were also observed, with values ranging from 1.0% to 1.5%. Using a new laboratory spectral calibration method, we estimated an average orthopyroxene content of 6% +/- 1%. The mass-deficit region of Psyche, which exhibits the highest radar albedo, also shows the highest value for the spectral slope and the minimum BD. The spectral characteristics of Psyche suggest that its parent body did not have the typical structure expected for a differentiated body or that the sequence of events that led to its current state was more complex than previously thought.
author2 Univ Arizona, LBT Observ
author_facet Univ Arizona, LBT Observ
Sanchez, Juan A.
Reddy, Vishnu
Shepard, Michael K.
Thomas, Cristina
Cloutis, Edward A.
Takir, Driss
Conrad, Albert
Kiddell, Cain
Applin, Daniel
author Sanchez, Juan A.
Reddy, Vishnu
Shepard, Michael K.
Thomas, Cristina
Cloutis, Edward A.
Takir, Driss
Conrad, Albert
Kiddell, Cain
Applin, Daniel
author_sort Sanchez, Juan A.
title DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE
title_short DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE
title_full DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE
title_fullStr DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE
title_full_unstemmed DETECTION OF ROTATIONAL SPECTRAL VARIATION ON THE M-TYPE ASTEROID (16) PSYCHE
title_sort detection of rotational spectral variation on the m-type asteroid (16) psyche
publisher IOP PUBLISHING LTD
publishDate 2016
url http://hdl.handle.net/10150/622750
http://arizona.openrepository.com/arizona/handle/10150/622750
work_keys_str_mv AT sanchezjuana detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT reddyvishnu detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT shepardmichaelk detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT thomascristina detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT cloutisedwarda detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT takirdriss detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT conradalbert detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT kiddellcain detectionofrotationalspectralvariationonthemtypeasteroid16psyche
AT applindaniel detectionofrotationalspectralvariationonthemtypeasteroid16psyche
_version_ 1718419337869524992