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Surprisingly Enriched CO and CH4 in Halley-type Comet 13P/Olbers: Clues to Its Interstellar Heritage

  • Authors: Michael A. DiSanti, Mohammad Saki, Erika L. Gibb, Boncho P. Bonev, Neil Dello Russo, Ronald J. Vervack, Karen Willacy, Younas Khan, Sara Faggi, Nathan X. Roth, Geronimo L. Villanueva, Hideyo Kawakita

Michael A. DiSanti et al 2026 The Planetary Science Journal 7 .

  • Provider: AAS Journals

Caption: Figure 5.

Excitation analysis for Comet 13P/Olbers. (a) Line-by-line nucleus-centered CO production rates (Section 4.1). (b) Linear least-squares slope fit as a function of rotational temperature, with the best-fit (optimal) Trot (53 ± 1 K) corresponding to a slope of zero (the horizontal red line). (c) Line-by-line H2O production rates for Trot (opt) = 53 K. (d) Same as panel (c), but for its formal best-fit Trot using the 13 brightest water lines. For both CO and H2O, line numbers correspond to those assigned (arbitrarily) in Figure 2(a). Details are given in Section 3.3.

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