Barnard's Star | Project Daedalus, List of nearest stars, Stars named after people, Stars and planetary systems in fiction, Stellar kinematics, Red dwarf, Star, Light-year, Constellation

Frederic P. Miller (u. a.)

ISBN 10: 6130215878 / ISBN 13: 9786130215873

Published by OmniScriptum, 2026

About this Item

Barnard's Star | Project Daedalus, List of nearest stars, Stars named after people, Stars and planetary systems in fiction, Stellar kinematics, Red dwarf, Star, Light-year, Constellation | Frederic P. Miller (u. a.) | Taschenbuch | Englisch | 2026 | OmniScriptum | EAN 9786130215873 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu Print on Demand.

Seller Inventory # 101427768

Bibliographic Details

• Title: Barnard's Star | Project Daedalus, List of nearest stars, Stars named after people, Stars and planetary systems in fiction, Stellar kinematics, Red dwarf, Star, Light-year, Constellation
• Publisher: OmniScriptum
• Publication Date: 2026
• Language: English
• ISBN 10: 6130215878
• ISBN 13: 9786130215873
• Binding: Taschenbuch
• Condition: Neu
• Dimensions: 220W x 150H x 8D millimeters 220 millimeters width by 150 millimeters height by 8 millimeters depth
• Weight: 197 grams
• Seller catalogs:
  • Bücher

About this title

Synopsis

Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. Barnard's Star, also known occasionally as Barnard's "Runaway" Star, is a very low-mass red dwarf star approximately 6 light-years away from Earth in the constellation of Ophiuchus. In 1916, American astronomer E. E. Barnard measured its proper motion as 10.3 arcseconds per year, which remains the largest known proper motion of any star relative to the Sun. At a distance of about 1.8 parsecs, or just under six light-years, Barnard's Star is the nearest known star in Ophiuchus, the second-closest known star system to the Sun, and the fourth-closest known individual star to the Sun, after the three components of the Alpha Centauri system. Despite its proximity, Barnard's Star at a dim magnitude 9 is not visible with the unaided eye. It is, however, much brighter in the infrared spectrum. Barnard's Star has been the subject of much study and has probably received more attention from astronomers than any other M dwarf star due to its proximity and favourable location for observation near the celestial equator. Research has focused on stellar characteristics, astrometry, and refining the limits of possible extrasolar planets. Although it is an ancient star, observations suggest that Barnard's Star still experiences flare events.