{"id":238152,"date":"2025-09-19T05:19:10","date_gmt":"2025-09-19T05:19:10","guid":{"rendered":"https:\/\/www.europesays.com\/us\/238152\/"},"modified":"2025-09-19T05:19:10","modified_gmt":"2025-09-19T05:19:10","slug":"webb-telescope-detects-gas-on-distant-dwarf-planet-makemake-for-the-first-time","status":"publish","type":"post","link":"https:\/\/www.europesays.com\/us\/238152\/","title":{"rendered":"Webb Telescope Detects Gas on Distant Dwarf Planet Makemake for the First Time"},"content":{"rendered":"

\t\t\"Observed<\/a>An SwRI-led team used Webb telescope observations (white) to detect methane gas on the distant dwarf planet Makemake. Sharp emission peaks near 3.3 microns reveal methane in the gas phase above Makemake\u2019s surface. A continuum model (cyan) is overlaid for comparison; the gas emission peaks are identified where the observed spectrum rises above the continuum. An artistic rendering of Makemake\u2019s surface is shown in the background. Credit: Courtesy of S. Protopapa, I. Wong\/SwRI\/STScI\/NASA\/ESA\/CSA<\/p>\n

Methane gas may signal an atmosphere or geological activity on a distant dwarf planet located at the outer edge of the Solar System.<\/strong><\/p>\n

A research team led by the Southwest Research Institute has detected gas on the distant dwarf planet Makemake using NASA\u2019s James Webb Space Telescope (JWST). With this finding, Makemake becomes only the second trans-Neptunian object, after Pluto, where gas has been confirmed. The gas was identified as methane.<\/p>\n

\u201cMakemake is one of the largest and brightest icy worlds beyond Neptune, and its surface is dominated by frozen methane,\u201d said SwRI\u2019s Dr. Silvia Protopapa, lead author of a new paper recently published in The Astrophysical Journal Letters. \u201cThe Webb telescope has now revealed that methane is also present in the gas phase above the surface, a finding that makes Makemake even more fascinating. It shows that Makemake is not an inactive remnant of the outer Solar System, but a dynamic body where methane ice is still evolving.\u201d<\/p>\n

Surface anomalies and thermal clues<\/p>\n

The methane signal was identified as solar-excited fluorescence, meaning sunlight absorbed by methane molecules is re-emitted as spectral emission. Protopapa and her co-authors note that this could reflect the presence of a thin atmosphere in balance with surface ices \u2014 as seen on Pluto \u2014 or short-lived processes such as comet-like sublimation or cryovolcanic plumes. Both explanations remain possible and are consistent with the current data, though limitations in spectral resolution and background noise prevent a definitive conclusion.<\/p>\n

Measuring about 890 miles (1,430 km) across, or roughly two-thirds the size of Pluto, Makemake has long captivated planetary scientists. Previous stellar occultations suggested the absence of a thick global atmosphere, though the existence of a faint one could not be excluded. In addition, infrared observations \u2014 including those from JWST \u2014 have revealed unusual thermal properties and anomalies in Makemake\u2019s methane ice. These results have led to speculation about localized hot spots and possible outgassing from its surface.<\/p>\n

Future Webb observations needed<\/p>\n

\u201cWhile the temptation to link Makemake\u2019s various spectral and thermal anomalies is strong, establishing the mechanism driving the volatile activity remains a necessary step toward interpreting these observations within a unified framework,\u201d said Dr. Ian Wong, staff scientist at the Space Telescope Science Institute and co-author of the paper. \u201cFuture Webb observations at higher spectral resolution will help determine whether the methane arises from a thin bound atmosphere or from plume-like outgassing.\u201d<\/p>\n

\u201cThis discovery raises the possibility that Makemake has a very tenuous atmosphere sustained by methane sublimation,\u201d said Dr. Emmanuel Lellouch of the Paris Observatory, another co-author of the study. \u201cOur best models point to a gas temperature around 40 Kelvin (-233 degrees Celsius) and a surface pressure of only about 10 picobars \u2014 that is, 100 billion times below Earth\u2019s atmospheric pressure, and a million times more tenuous than Pluto\u2019s. If this scenario is confirmed, Makemake would join the small handful of outer solar system bodies where surface\u2013atmosphere exchanges are still active today.\u201d<\/p>\n

\u201cAnother possibility is that the methane is being released in plume-like outbursts,\u201d added Protopapa. \u201cIn this scenario, our models suggest that methane could be released at a rate of a few hundred kilograms per second, comparable to the vigorous water plumes on Saturn\u2019s moon Enceladus and far greater than the faint vapor seen at Ceres.\u201d<\/p>\n

The team\u2019s research showcases the link between Webb observations and detailed spectral modeling, offering new insights into the behavior of volatile-rich surfaces across the trans-Neptunian region.<\/p>\n

Reference: \u201cRotational Dynamics in Pulsational Pair-instability Supernovae: Implications for Mass Loss and Transient Events\u201d by Trang N. Huynh, Emmanouil Chatzopoulos and Nageeb Zaman, 11 September 2025, The Astrophysical Journal.
DOI: 10.3847\/1538-4357\/adf4e7<\/a><\/p>\n

The data used in this work were acquired with JWST\u2019s Near-Infrared Spectrograph through Program 1254 (PI: A. H. Parker).<\/p>\n

Never miss a breakthrough: Join the SciTechDaily newsletter.<\/a><\/b><\/p>\n","protected":false},"excerpt":{"rendered":"An SwRI-led team used Webb telescope observations (white) to detect methane gas on the distant dwarf planet Makemake.…\n","protected":false},"author":3,"featured_media":238153,"comment_status":"","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[24],"tags":[4514,17301,935,14409,159,161,99044,783,67,132,68],"class_list":{"0":"post-238152","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-space","8":"tag-astronomy","9":"tag-james-webb-space-telescope","10":"tag-methane","11":"tag-planetary-science","12":"tag-science","13":"tag-solar-system","14":"tag-southwest-research-institute","15":"tag-space","16":"tag-united-states","17":"tag-unitedstates","18":"tag-us"},"share_on_mastodon":{"url":"https:\/\/pubeurope.com\/@us\/115229279089812629","error":""},"_links":{"self":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts\/238152","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/comments?post=238152"}],"version-history":[{"count":0,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/posts\/238152\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/media\/238153"}],"wp:attachment":[{"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/media?parent=238152"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/categories?post=238152"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.europesays.com\/us\/wp-json\/wp\/v2\/tags?post=238152"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}