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Brown Dwarfs: Crash Course Astronomy #28
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While Jupiter is nowhere near massive enough to initiate fusion in its core, there are even more massive objects out there that fall just short of that achievement called brown dwarfs. Brown dwarfs have a mass between giant planets and small stars. They were only recently discovered in the 1990s, but thousands are now known. More massive ones can fuse deuterium, and even lithium, but not hydrogen, distinguishing them from “normal” stars. Sort of.
Correction: In the illustration at 9:30, the numbers listed after the star names are the year of discovery, not distance.
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Chapters:
Introduction: Brown Dwarfs 00:00
L Stars & The Lithium Test 2:50
Discovering the First Brown Dwarfs 4:14
What Color Are Brown Dwarfs? 6:24
Physical Characteristics of Brown Dwarfs 7:30
Small Stars vs. Big Planets 8:11
Review 10:17
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Want to find Crash Course elsewhere on the internet?
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PHOTOS/VIDEOS
Gliese 229B Spectrum - image provided by Phil Plait [credit: NASA/ESA/Hubble/Al Schultz et al]
Correction: In the illustration at 9:30, the numbers listed after the star names are the year of discovery, not distance.
--
Chapters:
Introduction: Brown Dwarfs 00:00
L Stars & The Lithium Test 2:50
Discovering the First Brown Dwarfs 4:14
What Color Are Brown Dwarfs? 6:24
Physical Characteristics of Brown Dwarfs 7:30
Small Stars vs. Big Planets 8:11
Review 10:17
--
Want to find Crash Course elsewhere on the internet?
--
PHOTOS/VIDEOS
Gliese 229B Spectrum - image provided by Phil Plait [credit: NASA/ESA/Hubble/Al Schultz et al]
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