* Your assessment is very important for improving the work of artificial intelligence, which forms the content of this project
Download Stars Power Point
Constellation wikipedia , lookup
Dyson sphere wikipedia , lookup
Extraterrestrial life wikipedia , lookup
Corona Borealis wikipedia , lookup
Aries (constellation) wikipedia , lookup
Canis Minor wikipedia , lookup
Astronomical unit wikipedia , lookup
Rare Earth hypothesis wikipedia , lookup
Auriga (constellation) wikipedia , lookup
Dialogue Concerning the Two Chief World Systems wikipedia , lookup
International Ultraviolet Explorer wikipedia , lookup
Corona Australis wikipedia , lookup
Cassiopeia (constellation) wikipedia , lookup
Canis Major wikipedia , lookup
Star catalogue wikipedia , lookup
Perseus (constellation) wikipedia , lookup
Cygnus (constellation) wikipedia , lookup
Malmquist bias wikipedia , lookup
Stellar classification wikipedia , lookup
Stellar evolution wikipedia , lookup
H II region wikipedia , lookup
Cosmic distance ladder wikipedia , lookup
Aquarius (constellation) wikipedia , lookup
Stellar kinematics wikipedia , lookup
Corvus (constellation) wikipedia , lookup
Observational astronomy wikipedia , lookup
WHAT ARE STARS? •Huge, hot balls of gas that are trillions of kilometers away from the Earth. • Astronomers study the COLOR of star light • Which color is the hottest? • Red and yellow – cool • Blue - hot • Spectrum – when you look at white light through a glass prism – see a rainbow of colors (ROYGBIV) • Continuous Spectrum – shows all the colors – a hot, solid object, such as the glowing wire inside a light bulb • A Spectrograph is used to break a star’s light into a spectrum • This gives information about COMPOSITION and TEMPERATURE of a star • For example – when look at a neon sign WOULD NOT see a continuous spectrum but would see EMISSION LINES • Emission Lines are lines made when certain wave lengths of light or COLORS are given off by hot gases • Bright Line (Emission)-A spectrum consisting of individual lines at unique spots. CONTINUOUS SPECTRUM BRIGHT EMISSION LINES • Each element has a unique set of bright emission lines. • A Star’s Spectrum is made up of DARK EMISSION LINES Absorption DARK EMISSION LINES • A star’s atmosphere absorbs certain colors of light in the spectrum, which causes black lines to appear! • ABSORPTION SPECTRUM - a star’s atmosphere absorbs colors of light instead of emitting them • An absorption spectrum is produced when light from a hot solid or dense gas passes through a cooler gas. • Absorption spectrum of a star – inside is hotter than it’s atmosphere • Black lines in a spectrum represent where less light gets through • What is this star made of? Hydrogen Helium • Stars are classified by HOW HOT THEY ARE! • Temperature differences between stars result in COLOR DIFFERENCES • Hottest stars are BLUE • TYPES OF STARS Temperature & Color • Stars can be different colors • Reddish stars are coolest (<4000°C) • Orange/Yellow stars are medium (4000°-7000°C) • White & Blue stars are hottest (7000°-30,000°C) • • • • Brightest stars – 1st MAGNITUDE STARS Dimmest stars – 6th MAGNITUDE STARS Positive numbers – dimmer stars Negative numbers – brighter stars Apparent Magnitude • How bright stars look when they’re viewed from Earth • Low numbers are brightest, high are dimmest • Sun = -26.7 • Sirius = -1.45 (Brightest Star) Absolute Magnitude • The ACTUAL BRIGHTNESS OF A STAR • If all stars were the same distance away, their absolute magnitudes would be the same as their apparent magnitudes. Absolute Magnitude • The brightness that a star would have at a distance of 32.6 light years from Earth • Sun = +4.8 (ordinary for a star) • Due to closeness to Earth Sun’s apparent magnitude is -26.8 DISTANCE IN SPACE 1. LIGHT YEARS – distance that light travels in one year – 9.5 trillion kilometers (light moves 300,000 Km/sec) 2. PARALLAX – an apparent shift in the position of an object when viewed from different directions • Notice that the location of the middle star seems to shift in relation to more distant stars – seen through telescopes • Daytime and nighttime are caused by the Earth’s rotation • The apparent motion of the sun and stars in our sky is due too the EARTH’S ROTATION • The Earth’s tilt and revolution around the sun cause the seasons. • During each season the Earth faces a different part of the sky at night. • All stars that we see appear to rotate around POLARIS (the North Star) • Due to the Earth’s rotation all of the stars in the sky appear to make one complete circle around Polaris every 24 hours.