Images of the position of WISE1810 on 21 July 2024 from GTC/EMIR in the J, H and Ks bands. The object is marked with a red circle. The field of view of each image is 45′′×45′′. North is up and East left. Credit: arXiv (2025). DOI: 10.48550/arxiv.2503.22289
Using the 10.4-m Gran Telescopio Canarias (GTC), European astronomers have detected methane in the atmosphere of WISEA J181006.18−101000.5—the closest T dwarf to Earth. The finding was reported in a research paper published March 28 on the arXiv pre-print server.
Brown dwarfs are intermediate objects between planets and stars. Astronomers generally agree that they are substellar objects occupying the mass range between 13 and 80 Jupiter masses. One subclass of brown dwarfs (with effective temperatures between 500 and 1,500 K) is known as T dwarfs, and represents the coolest and least luminous substellar objects so far detected.
Studies of T dwarfs could help astronomers better understand objects near the disputed planet/star boundary, for instance, giant exoplanets. However, although many brown dwarfs have been detected to date, T dwarfs are not so common, as only about 400 such objects have been identified.
WISEA J181006.18−101000.5, or WISE1810 for short, is a metal-poor T dwarf at a distance of just 29 light years from the Earth. It has a radius of about 0.65 Jupiter radii and is some 17 times more massive than Jupiter. The effective temperature of WISE1810 is estimated to be within the range of 800–1,300 K.
Previous low-resolution near-infrared and mid-infrared observations of WISE1810 have suggested that it has a significantly chemically modified atmosphere dominated by hydrogen and water vapor. However, no evidence of methane has been found, which is a defining characteristic molecule of the T-dwarf type.
This has changed with the recent publication of a new study conducted by a team of astronomers led by Jerry Zhang of the University of La Laguna, Spain. They obtained new near-infrared photometry of WISE1810 with GTC’s Espectrografo Multiobjeto Infra-Rojo (EMIR), which resulted in clear detection of methane in the atmosphere of this T dwarf.
The detection of methane further supports the classification of WISE1810 as T-type instead of L-type, which was suggested by some studies. The researchers add that no evidence of carbon monoxide and potassium has been found in the atmosphere of this object.
Based on the collected data, the carbon abundance for WISE1810 was estimated to be -1.5 dex, which inferred a metallicity at a level of -1.7 dex. The effective temperature of the T dwarf was constrained to be about 1,000 K.
The authors of the paper explain that the low metallicity of WISE1810 probably accounts majorly for the non-detection of atomic potassium but a lower temperature could also boost this effect.
The study also found that WISE1810 has a heliocentric velocity of -83 km/s. This finding indicates that the object is more likely associated with the Milky Way’s thick disk rather than the halo, despite its very low metallicity.
More information:
Jerry Jun-Yan Zhang et al, Detection of Methane in the Closest Extreme Metal-poor T Dwarf WISEA J181006.18-101000.5, arXiv (2025). DOI: 10.48550/arxiv.2503.22289
Journal information:
arXiv
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Methane detected in the atmosphere of the nearest T dwarf (2025, April 7)
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