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    Past Shows
    • Ep. 166: Multiverses
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    • Ep. 155: Dwarf Stars
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    • Ep. 69: The Large Hadron Collider and the Search for the Higgs-Boson
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    • Ep. 54: Questions Show #6
    • Ep. 53: Astronomy in Science Fiction
    • Special Episode: Panspermia
    • Ep. 52: Mars
    • Ep. 51: Earth
    • Ep. 50: Venus


Ep. 155: Dwarf Stars

  • October 12th, 2009
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Artist illustration of a red dwarf star.

Artist illustration of a red dwarf star.

We think we live near an average star, but that's not the case at all. Compared to most stars in the Universe, the Sun is a giant! Let's look at the small end of the stellar spectrum, to stars with a fraction of the size and mass of our own Sun. There are many ways that a star can get small, and they lead dramatically different lives and deaths.

Ep. 155: Dwarf Stars

  • How big (or little) is our Sun?  Sun's Mass: 1.9891 ×1030 KG
  • A red dwarf is a small, cool, very faint, main sequence star whose surface temperature is under about 4,000 K. Red dwarfs are the most common type of star. Proxima Centauri is a red dwarf. (via Enchanted Learning)
  • Red Dwarf Stars -- Universe Today
  • Red Dwarf Stars — Wiki
  • How long do stars last? — Universe Today
  • Paper:  Habitability of Planets Around Red Dwarf Stars – University of Texas
  • Gliese 581 — Wiki
  • Hydrogen Burning — Cornell
  • Brown Dwarf Stars – Cool Cosmos
  • Research on Brown Dwarfs — UC Berkeley
  • Red Dwarf Stars – Universe Today
  • Red Dwarfs — Wiki
  • Electron Degeneracy Pressure — Wolfram
  • White Dwarf -- GSU
  • White Dwarf – Goddard SFC
  • Background radiation of the Universe (CMB) — UBC
  • Black dwarf stars – Universe Today
  • Black dwarfs – Wiki
  • How are black dwarf stars and neutron stars similar? Goddard SFC
  • Blue stragglers in globular clusters — SolStation
  • Looking for Planets Around White Dwarf Stars -- Professor Astronomy
  • Ep. 86 End of Everything Pt. 1
  • Ep. 87 End of Everything Pt. 2



Comments
  1. Julian Says:
    October 13th, 2009 at 6:58 am

    Sun is actually 10^30 kg not 10^33 kg! You've just fried us all!

  2. David Madison Says:
    October 13th, 2009 at 9:18 am

    The numbers tossed around are astronomical. Putting in perspective the smallest red dwarf fusing hydrogen for twelve trillion years, that is a thousand times as long as the universe has existed. When you say it will take a quadrillion years for it to cool off to just about absolute zero, that is eighty thousand times the current age of the universe.

  3. Jesse Cohen Says:
    October 13th, 2009 at 12:38 pm

    Congrats Dr. Pamela Gay on your appearance on History Channel's 'The Universe'! You were awesome!


       

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