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Stars

Date post: 10-May-2015
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by charem
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Page 2: Stars

Scientists believe that our galaxy is a barred spiral galaxyA barred spiral galaxy is a rotating, flat disk of stars, gas and dust with a bar-shaped center made of stars.

Page 3: Stars

A STAR IS BORN

Protostar Every star starts out in a mass of

clouds and gas called a nebula. causes hydrogen gas in the nebula to

spin. As the hydrogen gas spins, it becomes

hotter. It begins to glow.

Page 4: Stars

Medium and larger protostars spin until they reach extremely hot temperatures.

Through the process of nuclear fusion, hydrogen in the stars begins to turn into helium.This is the same process that goes on in the Sun, and makes it able to give light and heat to Earth.

Page 5: Stars

STAR COLORS

A star’s color comes from its surface temperature.

How does one star come to have a hotter surface temperature than another?

It’s a matter of size. The more mass a star has, the hotter

the surface temperature.

Page 6: Stars

STARS ARE CLASSIFIED BY THEIR SURFACE TEMPERATURE.

that is associated to specific spectral patterns

the spectral classification includes 7 main types: O, B, A, F, G, K, M.

A popular mnemonic for remembering this order is "Oh, Be A Fine Girl, Kiss Me".

Page 7: Stars

MORGAN-KEENAN SPECTRAL CLASSIFICATION

Class Temperature Star Color

O 30,000 - 60,000 °K Blue

B 10,000 - 30,000 °K Blue

A  7,500  - 10,000 °K White

F  6,000  -  7,500 °K White (yellowish)

G  5,000  -  6,000 °K Yellow (like the Sun)

K  3,500  -  5,000 °K Orange

M  2,000  -  3,500 °K Red

Page 8: Stars

WHAT IS A NOVA?  

. A nova is an explosion that happens on a white dwarf, which is a very old star.

Page 9: Stars

This swirl of colors is made of material left from Kepler’s Supernova located in the Milky Way GalaxyKepler’s Supernova was the last supernova seen in our galaxy.

Page 10: Stars

A SUPERNOVA GETS AT THE CORE

A supernova is like a nova, except the explosion takes place at the core of the star, not the surface.

Every supernova and nova is important, because each explosion creates dust

This dust forms the building blocks for nebulae, where new stars are born.

Page 11: Stars

BLACK HOLES

After a supernova, a star may leave behind a burned part

This part can collapse and absorb the light around it.

This is a black hole, the end of a giant star. A star must be 10 to 15 times larger than

the Sun in order to end as a black hole. A smaller star will simply cool rather than

collapsing.

Page 12: Stars

CLUSTERS OF STARS

Open clusters

have mostly young, bright, blue stars that were born together.

They usually have irregular shapes.

At 400 light years away, the Pleiades is Earth’s closest open cluster.

Example is Pleiades

Page 13: Stars

GLOBULAR CLUSTERS

can have as many as a million stars – more than open clusters.

have a sphere-like shape, with many stars at the center.

A globular cluster named M15 is the closest of its kind to Earth.

Page 14: Stars

TYPES OF STARS

Protostar a collection of gas that has collapsed down from a giant molecular cloud.

Over time, gravity and pressure increase, forcing the protostar to collapse down.

All of the energy release by the protostar comes only from the heating caused by the gravitational energy – nuclear fusion reactions haven’t started yet.

Page 15: Stars

T TAURI STAR

stage in a star’s formation and evolution right before it becomes a main sequence star.

T Tauri stars don’t have enough pressure and temperature at their cores to generate nuclear fusion

they do resemble main sequence stars Stars will remain in the T Tauri stage for

about 100 million years.

Page 16: Stars

MAIN SEQUENCE STAR

Our Sun is a main sequence star, and so are our nearest neighbors, Sirius and Alpha Centauri A

converting hydrogen into helium in their cores, releasing a tremendous amount of energy

Page 17: Stars

RED GIANT STAR

A shell of hydrogen around the core ignites continuing the life of the star, but causes it to increase in size dramatically.

star has become a red giant star, and can be 100 times larger than it was in its main sequence phase.

The red giant phase of a star’s life will only last a few hundred million years before it runs out of fuel completely and becomes a white dwarf.

Page 18: Stars

WHITE DWARF STAR

When a star has completely run out of hydrogen fuel in its core and it lacks the mass to force higher elements into fusion reaction, it becomes a white dwarf star

A white dwarf shines because it was a hot star once, but there’s no fusion reactions happening any more

Page 19: Stars

A white dwarf will just cool down until it because the background temperature of the Universe.This process will take hundreds of billions of years, so no white dwarfs have actually cooled down that far yet.

Page 20: Stars

RED DWARF STAR

Red dwarf stars are the most common kind of stars in the Universe.

Red dwarf stars are able to keep the hydrogen fuel mixing into their core, and so they can conserve their fuel for much longer than other stars.

red dwarf stars will burn for up to 10 trillion years.

Page 21: Stars

NEUTRON STARS

If a star has between 1.35 and 2.1 times the mass of the Sun, it doesn’t form a white dwarf when it dies.

Instead, the star dies in a catastrophic supernova explosion, and the remaining core becomes a neutron star.

Page 22: Stars

SUPERGIANT STARS

The largest stars in the Universe are supergiant stars.

supergiants are consuming hydrogen fuel at an enormous rate and will consume all the fuel in their cores within just a few million years.

Supergiant stars live fast and die young


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