stars
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STARS. Page Keeley Where do Stars Go?. Learning goal: Explain the physical properties of stars. Think About It. When you look at the night time sky, how many stars do you see? Hundreds? Thousands? Millions? - PowerPoint PPT PresentationTRANSCRIPT
Think About It When you look at the night time sky, how many
stars do you see? Hundreds? Thousands? Millions?
• Although there might be too many stars to count, all stars share similar characteristics? Can you come up with four different groups to characterize the stars?
How are stars classified?
• Stars are classified according to their physical properties.
• Color (Temperature)• Size• Distance from the Earth• Brightness – Apparent magnitude - Absolute magnitude
Color and Temperature
• Color reveals a star’s temperature• Hot stars appear blue (short wavelength)• Cool stars appear red (long wavelength)• Other colors in between like orange, yellow
and white
Size of Stars (Mass)
• Many stars come in pairs called “Binary Stars”• Binary stars rotate around each other• Scientists use this property to calculate mass
of stars
Brightness of a star
Apparent magnitude: How bright a star looks/appears from Earth depends on
1. Its size2. Its temperature3. Its distance from EarthAbsolute magnitude : how bright a star actually
is.
Distances of Stars from Earth
• Measured in:1. Light years2. Use Parallax angles (apparent change in
position of an object when you look at it from opposite sides of Earth’s orbit).
3. The nearest stars have a larger parallax angle
How is a star born?
• A star is born when the contracting gas and dust from a nebula become so dense and hot that nuclear fusion starts
• Nuclear fusion takes place when hydrogen atoms fuse forming helium.
• What is a nebula?
What determines how long a star will live?
• A star’s lifespan depends on its mass.• Small mass stars live longer because they use their fuel
more slowly• Large mass stars live shorter• A young star has more hydrogen• An old star has more helium• When a star begins to run out of hydrogen it becomes a
red giant or a supergiant.• When a star runs out of hydrogen it becomes a white
dwarf; a neutron star or a blackhole
H-R Diagram
• A graph that shows relationship between absolute magnitude and temperature of stars.
• About 90% of the stars are in the main sequence stage
• Hottest main sequence stars are the brightest and the coolest stars are the dimmest
• Red Giants and Super Giants brightness is because of massive size, not temperature.
• The Sun is in the main sequence stage
H-R diagram
Galaxies
• A huge group of stars, dust and gas bound together by gravity.
What are the main types of galaxies?• Spiral galaxies (Solar System is in a spiral
galaxy called The Milky Way)• Elliptical galaxies• Irregular galaxies
How can scientists determine whether a star is moving toward or away from the Earth?
• They use Doppler shifts• The light from a star that is moving away from
Earth appears red (its waves become longer)• The light from a star that is moving towards
Earth appears blue (its waves become shorter)
The Expanding Universe
• Most galaxies have Doppler Shifts towards the red end of the spectrum. This shows that the Earth and the source are moving away from each other.
• The red shift of distant galaxies indicate that the universe is expanding.