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November 30, 2017NASA Extends Campaign to Nickname New Horizons' Next Target

NASA is extending the campaign to find a temporary tag for the next flyby target of its New Horizons mission, giving the public until midnight Eastern Time on Dec. 6 to continue to help select a nickname for the Kuiper Belt object known as 2014 MU69.

On New Year's Day 2019, the New Horizons spacecraft will fly past this small, frozen Kuiper Belt world (or pair of worlds, if MU69 is a binary as scientists suspect) near the outer edge of our planetary system. This Kuiper Belt object (KBO) currently goes by the official designation "(486958) 2014 MU69." But earlier this month, NASA and the New Horizons team asked the public for help in giving "MU69" a nickname to use for this exploration target. The public suggested such a wide range of creative and quality nicknames that the mission team wanted to give web visitors additional time to vote.

The public suggested such a wide range of creative and quality nicknames that the mission team wanted to give web visitors additional time to vote. More than 96,000 votes have been cast and 31,000 names nominated, with participation coming from 118 countries.

The campaign website (http://frontierworlds.seti.org) includes nicknames under consideration; site visitors can vote for their favorites or nominate names they think should be added to the ballot. The campaign will close at midnight EST/9 pm PST on Wednesday, Dec. 6. NASA and the New Horizons team will review the top vote-getters and announce a selection in early January.

Learn more about New Horizons, NASA's mission to Pluto and the Kuiper Belt, at http://www.nasa.gov/newhorizons and http://pluto.jhuapl.edu.

Artist's concept of NASA’s New Horizons spacecraft flying by a possible binary 2014 MU69 on Jan. 1, 2019. Early observations of MU69 hint at the Kuiper Belt object being either a binary orbiting pair or a contact (stuck together) pair of nearly like-sized bodies with diameters near 20 and 18 kilometers (12 and 11 miles).

Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute/Carlos Hernandez

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