|
|
Browse All
:
ANTARES of Johnson Space Center (JSC) and Jet Propulsion Laboratory (JPL)
|
Printer Friendly |
A Close Encounter Of The Ste
…
| Title |
A Close Encounter Of The Stellar Kind |
| Explanation |
The unassuming star centered in this sky view [ http://skyview.gsfc.nasa.gov ] will one day be our next door [ http://www.bigear.org/vol1no2/kraus.htm ] stellar neighbor [ http://www.astro.wisc.edu/~dolan/constellations/extra/nearest.html ]. The faint 9th magnitude red dwarf [ http://antwrp.gsfc.nasa.gov/apod/ap991120.html ], currently 63 light-years away [ http://zebu.uoregon.edu/~soper/Stars/parallax_ly.html ] in the constellation Ophiucus [ http://www.astro.wisc.edu/~dolan/constellations/constellations/ Ophiuchus.html ], was recently discovered to be approaching our Solar System. Known in catalogs of nearby stars [ http://tarkus.pha.jhu.edu/~thenry/RECONS.html ] as Gliese 710 it is predicted to come within 1 light-year of the Sun ... a million years from now. At that distance this star, presently much too faint to be seen [ http://liftoff.msfc.nasa.gov/academy/universe/MAG.HTML ] by the naked eye, will blaze at 0.6 magnitude - rivaling the apparent brightness of the mighty red giant Antares [ http://antwrp.gsfc.nasa.gov/apod/ap970624.html ]. Ultimately Gliese 710 poses no direct collision danger itself although its gravitational influence will likely scatter comets out of the Solar System's reservoir, the Oort cloud [ http://www.windows.umich.edu/cgi-bin/tour_def/comets/ Oort_cloud.html ], sending some inbound. This future stellar encounter [ http://cass.jsc.nasa.gov/meetings/dps97/html/H2501/H2501.html ] was discovered by researchers [ http://www.newscientist.com/ns/970524/doomstar.html ] Joan Garcia-Sanchez and Robert Preston (JPL [ http://www.jpl.nasa.gov ]), and collaborators while studying stars in the solar neighborhood [ http://www.clockwk.com/stars/ ] using data from the Hipparcos Astrometry Satellite [ http://astro.estec.esa.nl/SA-general/Projects/Hipparcos/ hipparcos.html ]. The star field shown is based on the Palomar Digitized Sky Survey [ http://www-gsss.stsci.edu/dss/dss.html ] and is 1/4 degree wide (about half the diameter of the full moon). |
|
|
