Mirages and the Nature of Pluto's Atmosphere

J. A. Stansberry, J. I. Lunine, William B. Hubbard, Roger Yelle, D. M. Hunten

Research output: Contribution to journalArticle

48 Citations (Scopus)

Abstract

We present model occultation lightcurves demonstrating that a strong thermal inversion layer at the base of Pluto's stratosphere can reproduce the minimum flux measured by the Kuiper Airborne Observatory (KAO) during the 1988 occultation of a star by Pluto. The inversion layer also forms the occultation equivalent of a mirage at a radius of 1198 km, which is capable of hiding tropospheres of significant depth. Pluto's surface lies below 1198 km, its radius depending on the depth of the troposphere. We begin by computing plausible temperature structures for Pluto's lower atmosphere, constrained by a calculation of the temperature of the atmosphere near the surface. We then trace rays from the occulted star through the model atmosphere, computing the resultant bending of the ray. Model light curves are obtained by summing the contribution of individual rays within the shadow of Pluto on Earth. We find that we can reproduce the KAO lightcurve using model atmospheres with a temperature inversion and no haze. We have explored models with tropospheres as deep as 40 km (implying a Pluto radius of 1158 km) that reproduce the suite of occultation data. Deeper tropospheres can be fitted to the data, but the mutual event radius of 1150 km probably provides a lower bound. If Pluto has a shallow or nonexistent troposphere, its density is consistent with formation in the solar nebula with modest water loss due to impact ejection. If the troposphere is relatively deep, implying a smaller radius and larger density, signficant amounts of water loss are required.

Original languageEnglish (US)
Pages (from-to)503-513
Number of pages11
JournalIcarus
Volume111
Issue number2
DOIs
StatePublished - Oct 1994

Fingerprint

Pluto atmosphere
mirage
Pluto (planet)
Pluto
troposphere
occultation
atmosphere
Kuiper Airborne Observatory
radii
water loss
inversion layer
rays
atmospheres
observatory
inversions
temperature inversions
stars
solar nebula
lower atmosphere
temperature inversion

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Cite this

Stansberry, J. A., Lunine, J. I., Hubbard, W. B., Yelle, R., & Hunten, D. M. (1994). Mirages and the Nature of Pluto's Atmosphere. Icarus, 111(2), 503-513. https://doi.org/10.1006/icar.1994.1160

Mirages and the Nature of Pluto's Atmosphere. / Stansberry, J. A.; Lunine, J. I.; Hubbard, William B.; Yelle, Roger; Hunten, D. M.

In: Icarus, Vol. 111, No. 2, 10.1994, p. 503-513.

Research output: Contribution to journalArticle

Stansberry, JA, Lunine, JI, Hubbard, WB, Yelle, R & Hunten, DM 1994, 'Mirages and the Nature of Pluto's Atmosphere', Icarus, vol. 111, no. 2, pp. 503-513. https://doi.org/10.1006/icar.1994.1160
Stansberry, J. A. ; Lunine, J. I. ; Hubbard, William B. ; Yelle, Roger ; Hunten, D. M. / Mirages and the Nature of Pluto's Atmosphere. In: Icarus. 1994 ; Vol. 111, No. 2. pp. 503-513.
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