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Structure of the Universe. Structure of the Universe Or What’s Out There and Where is it?. The Solar System. Note large separation of inner and outer planets. National Geographic Magazine. Remembering the names of the planets in order:. Mercury Venus Earth Mars Jupiter Saturn Uranus
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Structure of the Universe Or What’s Out There and Where is it?
The Solar System • Note large separation of inner and outer planets National Geographic Magazine
Remembering the names of the planets in order: Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune Pluto My Very Elegant Mother Just Sat Upon Nine Porcupines
The Inner Planets:: Mercury Venus Earth Mars Asteroids • Close together (Relatively) • Terrestrial (made of rock like Earth) • Size (escape velocity of atmosphere)
The Outer Planets:: Jupiter Saturn Uranus Neptune Pluto • Spread out (Relatively) • Gassy and icy giants • Size (escape velocity of atmosphere)
Where comets come from The Kuiper belt and Oort Cloud:: • Hundreds of millions of comet like bodies • 50,000 AU in radius • Total mass 10 to 100 times Earth’s mass • A tenth planet???
The Solar System (again) • Pluto is most likely a Kuiper belt object National Geographic Magazine
Galaxies (Hubble types): Contemporary Astronomy, J. Pasachoff
Elliptical Normal Spiral Barred spiral Peculiar Irregular Galaxies (Hubble types): Contemporary Astronomy, J. Pasachoff
The Milky Way Galaxy You are Here • 100,000 LY in diameter, 16,000-3,000 LY thick • Contains a hundred billion stars (1011) • Total star mass about 3 x 1041 kg • The Sun is about 28,000 LY from the galactic center • Not very big as galaxies go.
The Milky Way Galaxy • The Sun orbits once every 200 million years • Our speed of orbit is about 250 km/s National Geographic Magazine
The Milky Way Galaxy (closeup) We are in the middle of a “chimney” National Geographic Magazine
Elliptical Galaxy (Don’t make many new stars)
The Whirlpool Galaxy (spirals make stars In their arms in an on-going process)
Barred spiral channeling material into its core Giving birth to stars
There are many Galaxies... • There are about 1011 galaxies in the visible Universe • The closest is about 2 x 106 LY from us
Star Clusters (These are much smaller than galaxies) Photo and text courtesy Of the Hubble Space Telescope site This stellar swarm is M80 (NGC 6093), one of the densest of the 147 known globular star clusters in the Milky Way galaxy. Located about 28,000 light-years from Earth, M80 contains hundreds of thousands of stars, all held together by their mutual gravitational attraction. Globular clusters are particularly useful for studying stellar evolution, since all of the stars in the cluster have the same age (about 15 billion years), but cover a range of stellar masses. Every star visible in this image is either more highly evolved than, or in a few rare cases more massive than, our own Sun. Especially obvious are the bright red giants, which are stars similar to the Sun in mass that are nearing the ends of their lives.
Emission Nebulae – Actually emit light • Reflection Nebulae – Merely reflect light • Absorption Nebulae – Block the light of stars. • Planetary Nebulae – Ejected star material. • Nebulae • Clouds of gas and dust • Birthplace of solar systems and stars • Types of Nebulae
Large Scale Structures • Groups • Clusters • Super Clusters, Clouds, Walls, Voids
NGS Map of the Universe National Geographic Magazine
Groups • A few Million LY wide • 3 - 6 conspicuous galaxies • A dozen or so smaller galaxies • Only a few times more dense than the Universe • Some of the smaller galaxies orbit the larger ones • Orbital speeds are 100-200 km/s
Our own Local Group National Geographic Magazine
Clusters (of galaxies) • 10 - 20 Million LY wide • Hundreds to Thousands of galaxies • (10 - 20 times more dense than the Universe) • The largest gravitationally bound structures • Orbital speeds are around 1000 km/s (faster)
Our own cluster and supercluster: National Geographic Magazine
Super Clusters, bubbles, walls • Super Clusters: • 100 Million LY wide or more • Tens of Thousands of galaxies • Modest enhancement of density • Walls and bubbles: • Much larger than Superclusters
So, putting it all together: National Geographic Magazine