{"title":"New surface composition and temperature maps of Pluto from New Horizons LEISA data","authors":"Alexey Drozdov, Nikolay Emelyanov","doi":"10.1016/j.icarus.2026.117031","DOIUrl":null,"url":null,"abstract":"<div><div>New Horizons RALPH/LEISA near-infrared spectra allow for regional mapping of Pluto’s surface ices and their physical state; however, scan-to-scan artifacts and variable spatial resolution complicate quantitative interpretation. We extend previous LEISA compositional studies (Protopapa et al., 2017; Schmitt et al., 2017; Emran et al., 2023) by combining five close-approach observations into co-registered equirectangular maps at 7 km/pixel and by jointly retrieving surface temperature, ice abundances, and grain sizes using a Hapke-based mixing model.</div><div>We mitigate bad pixels and edge overexposure linked to flat-field uncertainties and correct for residual scan-to-scan spectral discrepancies using per-observation scale and offset terms. The resulting maps provide distributions of CH<span><math><msub><mrow></mrow><mrow><mn>4</mn></mrow></msub></math></span>-rich ice, N<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span>-rich ice, H<span><math><msub><mrow></mrow><mrow><mn>2</mn></mrow></msub></math></span>O ice, and Titan Tholin, alongside a corresponding temperature map.</div></div>","PeriodicalId":13199,"journal":{"name":"Icarus","volume":"452 ","pages":"Article 117031"},"PeriodicalIF":3.2000,"publicationDate":"2026-07-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Icarus","FirstCategoryId":"101","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S0019103526000977","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"2026/3/6 0:00:00","PubModel":"Epub","JCR":"Q2","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
New Horizons RALPH/LEISA near-infrared spectra allow for regional mapping of Pluto’s surface ices and their physical state; however, scan-to-scan artifacts and variable spatial resolution complicate quantitative interpretation. We extend previous LEISA compositional studies (Protopapa et al., 2017; Schmitt et al., 2017; Emran et al., 2023) by combining five close-approach observations into co-registered equirectangular maps at 7 km/pixel and by jointly retrieving surface temperature, ice abundances, and grain sizes using a Hapke-based mixing model.
We mitigate bad pixels and edge overexposure linked to flat-field uncertainties and correct for residual scan-to-scan spectral discrepancies using per-observation scale and offset terms. The resulting maps provide distributions of CH-rich ice, N-rich ice, HO ice, and Titan Tholin, alongside a corresponding temperature map.
期刊介绍:
Icarus is devoted to the publication of original contributions in the field of Solar System studies. Manuscripts reporting the results of new research - observational, experimental, or theoretical - concerning the astronomy, geology, meteorology, physics, chemistry, biology, and other scientific aspects of our Solar System or extrasolar systems are welcome. The journal generally does not publish papers devoted exclusively to the Sun, the Earth, celestial mechanics, meteoritics, or astrophysics. Icarus does not publish papers that provide "improved" versions of Bode''s law, or other numerical relations, without a sound physical basis. Icarus does not publish meeting announcements or general notices. Reviews, historical papers, and manuscripts describing spacecraft instrumentation may be considered, but only with prior approval of the editor. An entire issue of the journal is occasionally devoted to a single subject, usually arising from a conference on the same topic. The language of publication is English. American or British usage is accepted, but not a mixture of these.