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The Interstellar Series: LP 944-20 Traditional Cache

This cache has been archived.

Indy-Md: Decided to let this star fade out, and open the area for another to place a cache if they want.

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Hidden : 1/23/2007
Difficulty:
2 out of 5
Terrain:
1.5 out of 5

Size: Size:   micro (micro)

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Geocache Description:

LP 944-20 is a fairly bright and energetic brown dwarf star located 16.3 light years away from our Sun. While bright, you still can't see it with your naked eye.

This extremely dim celestial object is one of the closest known solitary brown dwarfs to Sol at present. It is located about 16.3 light-years away in the eastern part of Constellation Fornax, the Furnace, in the southern hemisphere. Previously thought to be a very dim red dwarf star (M9.0 V) on its detection more than 25 years ago, Luyten Palomar (LP) 944-20 was detemined to be a brown dwarf in 1998 when Chris G. Tinney found that it was too cool to destroy all of the lithium in its atmosphere.

LP 944-20 appears to be only about 475 to 650 million years old but may be around 320 million years old if it is a member of the Castor moving group (an extensive but physically related group of more than 50 stars, including Castor itself, Vega, Formalhaut, Alderamin, and Zubenelgenubi, that has a common motion through space; the properties of the group suggest an age for its members to be on the order of 300 or so million years).

Astronomers did not anticipate that a brown dwarf could flare like a true star that sustains nuclear fusion at its core. That is, until on December 15, 1999, when LP 944-20 was observed -- by the Chandra X-Ray Observatory -- to emit a small solar-sized flare, which lasted for two hours and is thought to be very similar to the flares seen on our Sun. This suggested to astronomers that brown dwarfs have significant magnetic fields in order to generate these flares.

In early 2001, a group of astronomers announced the discovery of quiescent and flaring radio emission from LP 944-20. This first-ever detection of persistent radio emission from a brown dwarf was unexpected, and the astronomers concluded that LP 944-20 may be roiled by storms several times more powerful than the most energetic flares on the Sun. Follow-up observations suggested that the object's magnetic fields were extremely weak, which is a surprise because flares are normally powered by the energy in magnetic fields.

Now go find the cache (and please take care when rehiding it, as it could slip from its position if not replaced properly). No hints for you. Let it be a surprise.

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