Pluto's Atmosphere And A Targeted-Occultation Search For Other Bound Kbo Atmospheres

• Published in: Earth, moon, and planets Vol. 92; no. 1-4; pp. 375 - 393
• Main Authors: Elliot, J L, Kern, S D
• Format: Journal Article
• Language: English
• Published: Dordrecht Springer Nature B.V 01.06.2003
• Subjects: Astronomy; Atmosphere; Kuiper Belt; Occultation; Pluto; Pluto atmosphere; Telescopes; Trans-Neptunian objects
• ISSN: 0167-9295; 1573-0794
• DOI: 10.1023/B:MOON.0000031953.70454.50

Processes relevant to Pluto's atmosphere are discussed,and our current knowledge is summarized, including results of two stellar occultationsby Pluto that were observed in 2002. The question of whether other Kuiper belt objects (KBOs)may have bound atmospheres is considered, and observational indicators for KBO atmospheresare described. The definitive detection of a KBO atmosphere could be established withtargeted stellar-occultation observations. These data can also establish accurate diametersfor these objects and be used to detect possible nearby companions. Strategies for acquiringoccultation data with portable, airborne, and fixed telescopes are evaluated in terms of thenumber of KBO occultations per year that should be observable. For the sample of 29 currentlyknown KBOs with H ≤ 5.2, (radius ≤ 300 km for a geometricalbedo of 0.04), we expect about 4 events per year would yield good results for a (stationary) 6.5-m telescope. A network of portable0.36-m telescopes should be able to observe 6 events per year, and a 2.5-m airborne telescopewould have about 200 annual opportunities to observe KBO occultations.