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Astronomy 2e · Front matter

The Brightest Twenty Stars

CC BY 4.0 · OpenStax · approximately 3 min read

Learning objectives

Note: These are the stars that appear the brightest visually, as seen from our vantage point on Earth. They are not necessarily the stars that are intrinsically the most luminous.

View original figure (external; image not reproduced in this text edition)

Original figure description: A table titled “The Brightest Twenty Stars” with eleven columns and twenty-one rows. The first row is a header row and labels each column: “Traditional Name footnote: The brightest stars typically have names from antiquity. Next to each star’s ancient name, we have added a column with its name in the system originated by Bayer”, “Bayer Name”, “Luminosity (Sun = 1)”, “Distance (light-year) footnote: The distances of the more remote stars are estimated from their spectral types and apparent brightnesses and are only approximate. The luminosities for those stars are approximate to the same degree.”, “Spectral Type”, “Proper Motion: RA (arcsec/y)”, “Proper Motion: Dec (arcsec/y)”, “Right Ascension (h) footnote: Right ascension given for Epoch 2000.0”, “Right Ascension (m) footnote: Right ascension given for Epoch 2000.0”, “Declination (deg) footnote: Declination given for Epoch 2000.0”, “Declination (min) footnote: Declination given for Epoch 2000.0”. The second row reads “Sirius “, “α Canis Majoris”, “22.5”, “8.6”, “A1 V”, “−0.5”, “−1.2”, “06”, “45.2”, “−16”, “43”. The third row reads “Canopus “, “α Carinae”, “13,500”, “309”, “F0 II”, “+0.02”, “+0.02”, “06”, “24.0”, “−52”, “42”. The fourth row reads “Rigil Kentaurus”, “α Centauri”, “1.94”, “4.32”, “G2 V + K IV”, “−3.7”, “+0.5”, “14”, “39.7”, “−60”, “50”. The fifth row reads “Arcturus “, “α Bootis”, “120”, “36.72”, “K1.5 III”, “−1.1”, “−2.0”, “14”, “15.7”, “+19”, “11”. The sixth row reads “Vega “, “α Lyrae”, “49”, “25.04”, “A0 V”, “+0.2”, “+0.3”, “18”, “36.9”, “+38”, “47”. The seventh row reads “Capella “, “α Aurigae”, “140”, “42.80”, “G8 III + G0 III”, “+0.08”, “−0.4”, “05”, “16.7”, “+46”, “00”. The eighth row reads “Rigel “, “β Orionis”, “50,600”, “863”, “B8 I”, “+0.00”, “+0.00”, “05”, “14.5”, “−08”, “12”. The ninth row reads “Procyon”, “α Canis Minoris”, “7.31”, “11.46”, “F5 IV-V”, “−0.7”, “−1.0”, “07”, “39.3”, “+05”, “14”. The tenth row reads “Achernar “, “α Eridani”, “1030”, “139”, “B3 V”, “+0.10”, “−0.04”, “01”, “37.7”, “−57”, “14”. The eleventh row reads “Betelgeuse “, “α Orionis”, “13,200”, “498”, “M2 I”, “+0.02”, “+0.01”, “05”, “55.2”, “+07”, “24”. The twelfth row reads “Hadar”, “β Centauri”, “7050”, “392”, “B1 III”, “−0.03”, “−0.02”, “14”, “03.8”, “−60”, “22”. The thirteenth row reads “Altair “, “α Aquilae”, “11.2”, “16.73”, “A7 V”, “+0.5”, “+0.4”, “19”, “50.8”, “+08”, “52”. The fourteenth row reads “Acrux “, “α Crucis”, “4090”, “322”, “B0.5 IV + B1 V”, “−0.04”, “−0.01”, “12”, “26.6”, “−63”, “06”. The fifteenth row reads “Aldebaran”, “α Tauri”, “160”, “66.64”, “K5 III”, “+0.1”, “−0.2”, “04”, “35.9”, “+16”, “31”. The sixteenth row reads “Spica “, “α Virginis”, “2030”, “250”, “B1 III-IV + B2 V”, “−0.04”, “−0.03”, “13”, “25.2”, “−11”, “10”. The seventeenth row reads “Antares”, “α Scorpii”, “9290”, “554”, “M1.5 I + B2.5 V”, “−0.01”, “−0.02”, “16”, “29.4”, “−26”, “26”. The eighteenth row reads “Pollux “, “β Geminorum”, “31.6”, “33.78”, “K0 III”, “−0.6”, “−0.05”, “07”, “45.3”, “+28”, “02”. The nineteenth row reads “Fomalhaut “, “α Piscis Austrini”, “17.2”, “25.13”, “A3 V”, “+0.03”, “−0.2”, “22”, “57.6”, “−29”, “37”. The twentieth row reads “Mimosa”, “β Crucis”, “1980”, “279”, “B0.5 III”, “−0.04”, “−0.02”, “12”, “47.7”, “−59”, “41”. The twenty-first row reads “Deneb “, “α Cygni”, “50,600”, “1412”, “A2 I”, “+0.00”, “+0.00”, “20”, “41.4”, “+45”, “17”.

The brightest stars typically have names from antiquity. Next to each star's ancient name, we have added a column with its name in the system originated by Bayer (see the Naming Stars feature box.) The distances of the more remote stars are estimated from their spectral types and apparent brightnesses and are only approximate. The luminosities for those stars are approximate to the same degree. Right ascension and declination is given for Epoch 2000.0.
← The Nearest Stars, Brown Dwarfs, and White DwarfsThe Chemical Elements →

Attribution. Astronomy 2e, OpenStax, Rice University, and the contributing authors credited in the book. Licensed under Creative Commons Attribution 4.0 International. Source revision 63157f370b of openstax/osbooks-astronomy (2026-02-02). CC BY 4.0. Original source ↗. Text edition of a pinned CC BY 4.0 source revision of the OpenStax book, converted from CNXML by the EvidenceHelix importer. Original prose, learning objectives, tables, exercises, glossary and captions are preserved; images are not copied (figures link to the original source and keep their credits). No new content was added. Later revisions of this book can carry different licence terms and are not used.

In this chapter Contents

  • Preface
  • How to Study for an Introductory Astronomy Class
  • Astronomy Websites, Images, and Apps
  • Scientific Notation
  • Units Used in Science
  • Some Useful Constants for Astronomy
  • Physical and Orbital Data for the Planets
  • Selected Moons of the Planets
  • Future Total Eclipses
  • The Nearest Stars, Brown Dwarfs, and White Dwarfs
  • The Brightest Twenty Stars
  • The Chemical Elements
  • The Constellations
  • Star Chart and Sky Event Resources

Source

OpenStax source file ↗

Illustrated original ↗

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