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Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino
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Page 1: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

Milky Way GalaxyCierra Yoshikawa

Tomohiro Hoshino

Page 2: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

What is the Milky Way Galaxy?

Spiral galaxy Containing 400 billion stars

including our solar system Plus gas and dust x750 solar mass

Page 3: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

What is the Milky Way Galaxy?

100000 light year in diameter Formed by the collapse of a

large region of gas and dust Part of group of galaxies called

the Local Group Group of 30 galaxies that are

about 5 million light years across

Page 4: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

Other Info

Page 5: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

Milky Way Arms

Perseus Arm

Saittarius Arm

Cygnu Arm

Orion Arm (our solar system)

Norma Arm

Sctum-Crux Arm

Page 6: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.
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3 General Components

The halo Nuclear bulge The disk

Page 8: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

The Halo

Consists of the oldest stars and dark matter, absence of gas or dust 146 Globular Clusters

Spherical shape Believed to be formed 10-15 billion

yrs ago Produces hot gas called gamma-ray

halo

Page 9: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

The Disk

Contains the sun and other intermediate-to young stars (million –ten billion years old), gas and dust

Approximately 300pc (1,000 light years) thick and 30kpc (100,000 light years) in diameter

Page 10: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

The Disk Cont.

Sun sits about 2/3 of the way from the center to the edge of the disk.

Sun revolves around the center every 250 years

Page 11: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

Nuclear Bulge

The center of the Galaxy Dimension 1kpc by 6kpc Shaped like a football

Crowded with stars which are 10 billions years old or older (population II)

Page 12: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

Nuclear Bulge Cont.

The most brightest region is called Sgr A ~ 2 x 106 M of Sun within 1 pc Stars are only 1000 AU apart A collision every 106 years

Page 13: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.
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Types of Stars

Population I: Younger, metal-rich stars Found in disk

Population II: Older, metal- poor stars Found in halo

Page 16: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

View from Earth

Can only be seen on a clear night

Looks like a band of stars splashed on the sky

Can’t see spiral structure from Earth, images of structure created from computer modeling based on information from stars as they orbit the galaxy

Most of it in invisible from Earth due to being in the disk

5,000-8,000 stars visible from Earth

Page 17: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

View from Earth

Page 18: Milky Way Galaxy Cierra Yoshikawa Tomohiro Hoshino.

Works Cited “Our Solar System in the Milky Way Galaxy.” N.p.

N.d. Web. 16 April 2011. <http://www.enchantedlearning.com/subjects/astronomy/solarsystem/where.shtml>.

“Our own Galaxy-The Milky Way.” Cambridge Cosmology: Galaxies, N.d. Web. 16 April 2011. <http://www.damtp.cam.ac.uk/research/gr/public/gal_milky.html>.

“The Milky Way Galaxy.” N.p. 25 Aug. 2005. Web. 16 April 2011. <http://seds.org/messier/more/mw.html>.

“The Milky Way Galaxy.” University of California, San Diego Center for Astrophysics & Space Sciences, N.d. Web. 16 April 2011. <http://casswww.ucsd.edu/public/tutorial/MW.html>.