Download Page R63 - ClassZone

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Lyra wikipedia , lookup

CoRoT wikipedia , lookup

Hipparcos wikipedia , lookup

Perseus (constellation) wikipedia , lookup

Corvus (constellation) wikipedia , lookup

Star wikipedia , lookup

Timeline of astronomy wikipedia , lookup

Proxima Centauri wikipedia , lookup

Planetary habitability wikipedia , lookup

Stellar kinematics wikipedia , lookup

Brown dwarf wikipedia , lookup

Ursa Minor wikipedia , lookup

Astronomical spectroscopy wikipedia , lookup

Star formation wikipedia , lookup

Future of an expanding universe wikipedia , lookup

Stellar classification wikipedia , lookup

Hayashi track wikipedia , lookup

Stellar evolution wikipedia , lookup

Transcript
s8pe-emapp-ca-R52-R64
12/13/05
3:14 PM
MAZER
Page R63
The Hertzsprung-Russell Diagram
The Hertzsprung-Russell (H-R) Diagram is a graph that shows stars
plotted according to brightness and surface temperature. Most stars
fall within a diagonal band called the main sequence. In the mainsequence stage of a star’s life cycle, brightness is closely related to
surface temperature. Red giant and red supergiant stars appear
above the main sequence on the diagram. These stars are bright in
relation to their surface temperatures because their huge surface
areas give off a lot of light. Dim white dwarfs appear below the
main sequence.
HIGHEST
THE H-R DIAGRAM
BLUE SUPERGIANTS
Rigel
Betelgeuse
Spica
RED
SUPERGIANTS
Polaris
<MA
IN S
EQU
ENC
E>
Arcturus
LUMINOSITY
RED GIANTS
Aldebaran
Sirius
Sun
RED
DWARFS
WHITE
DWARFS
LOWEST
Proxima Centauri
TEMPERATURE
APPENDIX
HOTTEST
COOLEST
Appendix R63
PDF