Reconciling results of 2019 and 2020 stellar occultations on Pluto's atmosphere. New constraints from both the 5 September 2019 event and consistency analysis

• Published in: arXiv.org 2023-11
• Main Authors: Ye Yuan, Li, Fan, Fu, Yanning, Chen, Jian, Tan, Wei, Zhang, Shuai, Zhang, Wei, Zhang, Chen, Zhang, Qiang, Ye, Jiahui, Li, Delai, Zhu, Yijing, Fu, Zhensen, Zhu, Ansheng, Chen, Yue, Xu, Jun, Zhang, Yang
• Format: Article
• Language: English
• Subjects: Pluto; Pluto atmosphere; Pressure; Pressure drop; Pressure measurement; Stellar occultation
• ISSN: 2331-8422
• DOI: 10.48550/arxiv.2309.14724

A stellar occultation by Pluto on 5 September 2019 yielded positive detections at two separate stations. Using an approach consistent with comparable studies, we derived a surface pressure of \(11.478 \pm 0.55~\mathrm{\mu bar}\) for Pluto's atmosphere from the observations of this event. In addition, to avoid potential method inconsistancies highlighted by Sicardy et al. when comparing with historical pressure measurements, we reanalyzed the data by 15 August 2018 and 17 July 2019 events, respectively. All the new measurements provide a bridge between the two different perspectives on the pressure variation since 2015: a rapid pressure drop from previous studies of the 15 August 2018 and 17 July 2019 events and a plateau phase from that of the 6 June 2020 event. The pressure measurement from the 5 September 2019 event aligns with those from 2016, 2018, and 2020, supporting the latter perspective. While the measurements from the 4 June 2011 and 17 July 2019 events suggest probable V-shaped pressure variations unaccounted for by the volatile transport model (VTM) from Meza et al., the VTM remains applicable on average. And, the validity of the V-shaped variations is debatable due to the stellar faintness of the 4 June 2011 event and the grazing single-chord geometry of the 17 July 2019 event. To reveal and understand all significant pressure variations of Pluto's atmosphere, it is essential to provide constraints on both short-term and long-term evolutions of the interacting atmosphere and surface by continuous pressure monitoring through occultation observations, whenever possible, complemented by frequent spectroscopy and photometry of the surface.