Home Contact | About | Friends of McDonald | Sign up for Sky Tips
McDonald Observatory McDonald Observatory
A production of the University of Texas McDonald Observatory
StargazingResourcesRadioMagazineTeachersGift ShopMedia Center

Send to a friend 
Printable version 
En Español
Keywords
Astronomical Distances 
Sun 
Earth 
Extrasolar Planets 
Resources
Brightest stars
Extrasolar planets
Latest news about exoplanets
FAQs about Stars and Nebulae
Astronomy Gift Shop
2009 Sky Almanac
McDonald Observatory logo cap

The one constant in the Universe: StarDate magazine
What is the nearest star? 
Of course, the nearest star to Earth is the one we see every day -- our dear old Sun. At a mere 93 million miles distant, it takes light from the Sun only eight minutes to arrive on Earth, shining through your bedroom window at dawn and on sunbathers on the French Riviera.

Several stars lie within a few light-years of the Sun. At a distance of just over four light-years, the three members of Alpha Centauri, including Proxima Centauri, are the nearest stars to Earth. The next three closest stars are red dwarfs: Barnard's Star is six light-years from Earth. Wolf 359 and Lalande 21185 are about eight light-years distant.

The brightest star in Earth's night sky is Sirius, 8.7 light-years away. The binary system called Procyon is a bit farther at 11.2 light-years.

The search for extrasolar planets might take us to Epsilon Eridani or Tau Ceti, Sun-like stars at 10.8 and 11.8 light-years away. Rounding out the stellar neighborhood at a distance of about 11 light-years are Epsilon Indi and the binary system 61 Cygni.

Other FAQs
» FAQs about StarDate Online

Stars and Nebulae Links
StarDate's Black Hole Encyclopedia
Stars and Constellations
Virtual Trips to Black Holes and Neutron Stars

Copyright ©1995-2006 The University of Texas McDonald Observatory. Material on this site may be linked to, quoted or reproduced for educational or personal purposes without prior permission, provided appropriate credit is given. Teachers, scout leaders, and others may distribute the material for classroom instruction or related educational purposes. The materials may not be sold or published in any other form without written permission from The University of Texas McDonald Observatory.