The steep red spectrum of 1992 AD

An asteroid covered with organic material?

Uwe - Fink, Martin Hoffmann, William Grundy, Michael Hicks, William Sears

Research output: Contribution to journalArticle

37 Citations (Scopus)

Abstract

A spectrum of the newly discovered asteroid 1992 AD (now numbered 5145) was obtained by us with our CCD camera and spectrometer 1992 February 01.23. The reflection spectrum of 1992 AD displays a very steep and constant red slope between 0.5 and 1.0 μm and exhibits no absorption nor emission features. The red slope is steeper than that of any presently known Solar System object. The reflectivity ratio between 1.0 and 0.55 μm is a factor of 3.5 (1.36 magnitudes), or using a slight extrapolation, a factor of 4.90 (1.72 magnitudes) for the wavelength octave 1.0 to 0.5 μm. The steep red slope is difficult to match with conventional silicate or meteoritic materials. While allotropes of sulfur may give a partial match, the best match is provided by the steep red spectra of mixtures of tholins, the residues left after subjecting organic molecules to an energetic radiation environment.

Original languageEnglish (US)
Pages (from-to)145-149
Number of pages5
JournalIcarus
Volume97
Issue number1
DOIs
StatePublished - 1992

Fingerprint

organic materials
asteroids
asteroid
slopes
octaves
CCD cameras
solar system
reflectivity
extrapolation
silicates
spectrometer
sulfur
energetics
silicate
spectrometers
wavelength
reflectance
radiation
wavelengths
material

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

The steep red spectrum of 1992 AD : An asteroid covered with organic material? / Fink, Uwe -; Hoffmann, Martin; Grundy, William; Hicks, Michael; Sears, William.

In: Icarus, Vol. 97, No. 1, 1992, p. 145-149.

Research output: Contribution to journalArticle

Fink, Uwe - ; Hoffmann, Martin ; Grundy, William ; Hicks, Michael ; Sears, William. / The steep red spectrum of 1992 AD : An asteroid covered with organic material?. In: Icarus. 1992 ; Vol. 97, No. 1. pp. 145-149.
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abstract = "A spectrum of the newly discovered asteroid 1992 AD (now numbered 5145) was obtained by us with our CCD camera and spectrometer 1992 February 01.23. The reflection spectrum of 1992 AD displays a very steep and constant red slope between 0.5 and 1.0 μm and exhibits no absorption nor emission features. The red slope is steeper than that of any presently known Solar System object. The reflectivity ratio between 1.0 and 0.55 μm is a factor of 3.5 (1.36 magnitudes), or using a slight extrapolation, a factor of 4.90 (1.72 magnitudes) for the wavelength octave 1.0 to 0.5 μm. The steep red slope is difficult to match with conventional silicate or meteoritic materials. While allotropes of sulfur may give a partial match, the best match is provided by the steep red spectra of mixtures of tholins, the residues left after subjecting organic molecules to an energetic radiation environment.",
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AU - Sears, William

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AB - A spectrum of the newly discovered asteroid 1992 AD (now numbered 5145) was obtained by us with our CCD camera and spectrometer 1992 February 01.23. The reflection spectrum of 1992 AD displays a very steep and constant red slope between 0.5 and 1.0 μm and exhibits no absorption nor emission features. The red slope is steeper than that of any presently known Solar System object. The reflectivity ratio between 1.0 and 0.55 μm is a factor of 3.5 (1.36 magnitudes), or using a slight extrapolation, a factor of 4.90 (1.72 magnitudes) for the wavelength octave 1.0 to 0.5 μm. The steep red slope is difficult to match with conventional silicate or meteoritic materials. While allotropes of sulfur may give a partial match, the best match is provided by the steep red spectra of mixtures of tholins, the residues left after subjecting organic molecules to an energetic radiation environment.

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