Ch. 21 Flashcards
Star Birth
From dense, cool clumps or separated hotter clumps
Protostars
Very young stars gathered from dust & gas + contracting under gravity
Orion Nebula
- Can best be seen with infrared images
- 4 bright stars in center: Trapezium stars
Star Formation
(1) Dense cores form within molecular cloud
(2) Protostar forms at center of dense core accumulating add’l material through gravity
(3) Stellar wind breaks out but is confined to flow out along poles
(4) Eventually wind sweeps away cloud material
Evolutionary Tracks for Contracting Prostars
(1) More mass → Shorter time to go through each stage
(2) Lower it is in main sequence, harder it is to form a star
Disk Around Protostars
Disk of gas and dust seems essential to star formation
Exoplanet
Planet outside our solar system
Geneva Observatory (Didier Queloz & Michel Mayor)
First to discover a planet around a regular star
Hot Jupiter
Giant planets really close to stores
Planet Transit
Method for detecting exoplanets as they cross in front of the star causing the star to dim slightly
Kepler
Launched to detect exoplanets