Stars

26
Stars • The apparent twinkling of the stars is a product of the turbulence and motion of the Earth’s atmosphere • Stars have different colors depending on how hot they are. The HOTTEST stars are BLUE, the COLDEST stars are RED. (Note- this is opposite to what we are used to associating with temperature.) • Color is used to determine ages – stages – in life cycle.

description

Stars. The apparent twinkling of the stars is a product of the turbulence and motion of the Earth’s atmosphere - PowerPoint PPT Presentation

Transcript of Stars

Page 1: Stars

Stars• The apparent twinkling of the stars is a

product of the turbulence and motion of the Earth’s atmosphere

• Stars have different colors depending on how hot they are. The HOTTEST stars are BLUE, the COLDEST stars are RED. (Note- this is opposite to what we are used to associating with temperature.)

• Color is used to determine ages – stages – in life cycle.

Page 2: Stars

Spectroscope

• A tool that is used to separate light into the visible spectrum. Used to help determine elements in the stars.

Page 3: Stars

Absorption Spectroscopy

Page 4: Stars
Page 5: Stars
Page 6: Stars
Page 7: Stars
Page 8: Stars

Star Colors

• Blue (HOT) 11-40,000C (young)• Beta Centauri• Blue-White 7.5-11,000C Rigel (supergiant)

• White 6-7,500C Vega• Yellow 5-6,000C _____• Orange 3.5-5,000C Aldebaran• Red (COLD) 3-3,500C (old)

Betelgeuse

Page 9: Stars

Hadar (r) and Alpha Centauri (l)

Vega – upper left

Page 10: Stars

Star Life Cycle• Nebula: a large cloud of gas and dust in space

that is the beginning of a star (PLANETS are also formed this way)

• Dwarf: a main sequence star or, the smallest of stars (up to 20 times larger than our sun and up to 20,000 times brighter. Our sun is a dwarf star.)

• Red Giant: star is dying (red=cold) and energy is expanding outward

• White Dwarf: a dying star that is extremely massive and may soon become a black hole

• Supernova: an exploding star; usually occurring after a dying star becomes too dense to be supported

Page 11: Stars

• Binary star (double star): a stellar system consisting of two stars orbiting around their center of mass

• Our Sun is unusual in that it is NOT part of a binary system

Hubble image of the Sirius binary system, in which Sirius B can be clearly seen (lower left).

Page 12: Stars

Star forming region in the nebula NCG 604, in the nearby spiral galaxy M33,

Page 13: Stars

Diminutive by stellar standards, white dwarf stars are also intensely hot ...but they are cooling. No longer do their interior nuclear fires burn, so they will continue to cool (turn more red) until they fade away

Page 14: Stars

E0102-72 is a supernova remnant in the Small Magellanic Cloud, a satellite galaxy of the Milky Way. This galaxy is 190,000 light years from Earth. E0102 -72, which is approximately a thousand years old, is believed to have resulted from the explosion of a massive star. Stretching across forty light years of space, the multi-million degree source resembles a flaming cosmic wheel.

Page 15: Stars

Star Vocabulary

• Luminosity: the brightness of a star compared to the brightness of the Sun. In other words, the Sun’s luminosity is 1, Sirius is 23, Adhara is 5,000. Luminosity is measured in ergs per second.

– The apparent brightness of the sun is 63 billion times brighter than Arcturus, although intrinsically the Sun is 100 times fainter.

• Apparent Magnitude: stars closer to Earth appear brighter than those that are farther away

• Absolute Magnitude: big stars are brighter than small stars. This is the ACTUAL brightness of the star– If all the stars were lined up equi-distant from Earth, we would be

able to compare their actual brightness

Page 16: Stars

Magnitude

• The SMALLER the magnitude, the BRIGHTER the star– For example, Vega with an apparent

magnitude of +.02 seems about 2 ½ times brighter than Antares whose apparent magnitude is +.98

– Antares is actually almost 100 times as bright as Vega, since Antares has an absolute magnitude of -4.0 and Vega ‘s is +.5

Page 17: Stars

Magnitude cont.

• As a comparison, the Sun has an apparent magnitude of -27, but an absolute magnitude of +5. this is because the Sun is so close to Earth.

Page 18: Stars

Hertzsprung-Russell Diagram

• An American, Henry Russell and a Dutchman, Ejnar Hertzsprung noted a relationship between temperature (color) and luminosity (brightness) of the stars.

• The significance of the discovery of the “main sequence” is that for any given temperature, there is a preferred radius. Therefore, luminosity is related to temperature.

Page 19: Stars

SunPage 714In your book

Hot, dim

Cool, brightHot, bright

_______

Hertzsprung-RussellDiagram

White dwarfs,Very hot,Very dense

Very bigVery brightcool

Page 20: Stars
Page 21: Stars
Page 22: Stars

Our SUN

• Age: approx 4.5 billion years old

• Diameter: 1.4 X 106 km

(medium sized star)

• Temperature: 5,800 Kelvin (10,000°F)

• Distance from Earth: 1.5 X 108 km (150,000,000) (closer than any other star)

• Burns more than 24 billion tons of Hydrogen gas per minute.

Page 23: Stars

Sun Vocab

• Sunspot: an area of the sun that gives off less light, due to a disturbance in the sun’s magnetic field

Page 24: Stars

Sun Vocab

• Solar Flare: an area of the sun that erupts

Page 25: Stars

Sun Vocab

• Corona: the area surrounding the Sun that can be seen during an eclipse

• Core: center of the sun where the thermonuclear transmutation of H to He occurs

• Photosphere: the visible surface of the Sun – several hundred miles thick

Page 26: Stars

(part of the atmosphere)

(Visible surface)