{ "id": "1409.5899", "version": "v1", "published": "2014-09-20T15:29:45.000Z", "updated": "2014-09-20T15:29:45.000Z", "title": "A New Parallax Measurement for the Coldest Known Brown Dwarf", "authors": [ "K. L. Luhman", "T. L. Esplin" ], "comment": "Astrophysical Journal, in press", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "WISE J085510.83-071442.5 was recently discovered as the coldest known brown dwarf based on four epochs of images from the Wide-field Infrared Survey Explorer and the Spitzer Space Telescope. We have improved the accuracy of its parallax measurement by obtaining two additional epochs of Spitzer astrometry. We derive a parallactic distance of 2.31+/-0.08 pc, which continues to support its rank as the fourth closest known system to the Sun when compared to WISE J104915.57-531906.1 AB (2.02+/-0.02 pc) and Wolf 359 (2.386+/-0.012 pc). The new constraint on the absolute magnitude at 4.5um indicates an effective temperature of 235-260 K based on four sets of theoretical models. We also show the updated positions of WISE J085510.83-071442.5 in two color-magnitude diagrams. Whereas Faherty and coworkers cited its location in MW2 versus J-W2 as evidence of water clouds, we find that those data can be explained instead by cloudless models that employ non-equilibrium chemistry.", "revisions": [ { "version": "v1", "updated": "2014-09-20T15:29:45.000Z" } ], "analyses": { "keywords": [ "brown dwarf", "parallax measurement", "employ non-equilibrium chemistry", "spitzer space telescope", "wide-field infrared survey explorer" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/796/1/6", "journal": "The Astrophysical Journal", "year": 2014, "month": "Nov", "volume": 796, "number": 1, "pages": 6 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014ApJ...796....6L" } } }