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Where are we?

Date post: 22-Feb-2016
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Where are we?. http://zebu.uoregon.edu/~js/ast122/. The Milky Way. We are here. Top view. Side view. ~200 billion stars. One revolution every ~200 million years. Comparison of different stars. Stars come in a wide range of sizes. And different emission temperatures…. - PowerPoint PPT Presentation
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Where are we? http://zebu.uoregon.edu/~js/ast122/
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Page 1: Where are we?

Where are we?

http://zebu.uoregon.edu/~js/ast122/

Page 2: Where are we?

We are here

• ~200 billion stars.• One revolution every ~200 million years.

Side view

Top view

The Milky Way

Page 3: Where are we?

Comparison of different stars

Stars come in a wide range of sizes

Page 4: Where are we?

And different emission temperatures…

• Typical star b.b. temperatures range from 3000K to 20,000K.

• Some stars look bluer, some look redder.

Page 5: Where are we?

Getting closer…

Page 6: Where are we?

The Sun

uv image

Page 7: Where are we?

Some details about the sun:

Gravitational collapse - high pressure, temperature

Thermonuclear reaction: 4H+ He + 2e+ + 2n + 26.5MeV(1eV = 1.6 x 10-19J)

Page 8: Where are we?
Page 9: Where are we?

Sun Facts I:

• Diameter: 1.4 million km

• Age: 4.5 billion years (lifetime 11 billion years)

• Mass: 2 x 1030 kg (330,000 x Earths) (99.8% of mass of solar system)

• Density: 1.41 (water = 1)

• Composition (by mass): Hydrogen: 73%, Helium: 25%, Others: 2%

Page 10: Where are we?

Sun facts II:

• Distance from Earth: 149.6 million km.

• Distance to nearest Star: 9.46 million million km.

• Luminosity: 4 x 1026 J s-1 (390 billion billion Megawatts).

• Solar Cycle: 8 - 11 years.• Temperature at Surface: 5,800°C (10,500 °F).• Temperature of Core: 14 million°C (22.5 million °F)• Pressure at core: 250 billion atmospheres (2.5 x 1016 Pa)• Every second 700 million tons of hydrogen converted to 695 million tons helium, and 5 million tons of energy.

Page 11: Where are we?

Sunspots and coronal loops:jets of plasma trapped by sun’s magnetic field

NASA (uv image from TRACE)

Page 12: Where are we?

We are very small!

(NASA, TRACE)

Page 13: Where are we?

Sunspots II

Royal Swedish Academy of Sciences Vacuum telescope

Page 14: Where are we?

Structure of the Solar System

Solar system formed from cloud of gas/debris from supernova

Oort cloud - extends out 50,000 AU (1000 x Pluto’s orbit)(nearly a light year, 25% of distance to nearest star)

Page 15: Where are we?

Structure of the Solar System

> 70,000 objects with radius >1 km, including dwarf planets> 35,000 Kuiper Belt objects greater than 100 kmLargely composed of frozen ices (volatiles - methane, water, amonia)

Kuiper belt - Neptune to ~55AU

Page 16: Where are we?

Structure of the Solar System

Dwarf planet (plutoid): 1) is in orbit around the Sun.2) has sufficient mass for its self-gravity to overcome rigid body forces

so that it assumes a hydrostatic equilibrium (near-spherical) shape.3) has not cleared the neighborhood around its orbit.4) is not a satellite.

Page 17: Where are we?

Pluto (demoted 2006):

Radius: 1137 kmMass: 1.3x1022 kmOrbit: 5.9x109 kmMade of: rock, ice Moons: 1Atmosphere: ~tenuous

CO2, CH4

Eliot Young (SwRI) et al., NASA

Page 18: Where are we?

Neptune:

Radius: 24,766 kmMass: 1.0x1026 kgOrbit: 4.5 x 109 kmMade of: ices (H20, CH4, NH3), rock, hydrogen (15%) heliumAtmosphere: yes Moons: 13 known

- Internal heat source radiates twice the energy it receives

- Fastest winds in solarsystem > 2000km/hr

1 day = 16 hours1 year = 60,225 days

(http://seds.lpl.arizona.edu/nineplanets)

Page 19: Where are we?

Neptune’s fast winds?

Under such conditions, the methane found in Neptune's atmosphere also decomposes, as the bonds holding methane's four hydrogen atoms dissolve and the carbon atoms may bind to one another in the extreme pressure to form diamonds (according to a new hypothesis by a team at the University of California at Berkeley and experiments conducted by Robin Benedetti). Hence, a rain of diamonds may be falling toward Neptune's core, which release heat through friction with its heavy atmosphere (Curtis Rist, Discover, September 2000).

Random fact:-

Scientists know diamonds can form in other places in space, too, besides the Earth. For example, the biggest diamond in the galaxy is the entire crystallized core of a dwarf star, 2,500 miles across, that weighs 5 million trillion trillion pounds, which translates to approximately 10 billion trillion trillion carats, or a one followed by 34 zeros.

Page 20: Where are we?

Uranus:

Radius: 25,559 kmMass: 8.7x1025 kgOrbit: 2.9 x 109 kmMade of: ices, rock,

hydrogen, heliumAtmosphere: yes Moons: 27

n.b. axis of rotation parallel to plane of orbit!

(http://seds.lpl.arizona.edu/nineplanets)

Day: 17 hoursYear: 30,700 days

1 season = 1 year.

Page 21: Where are we?

Saturn:

Radius: 60,268 kmMass: 5.7x1026 kgOrbit: 1.4 x 109 kmMade of: hydrogen, helium

ice, and rockAtmosphere: yes Moons: 31

Least dense planet0.7 g cm-3 (water = 1)

NASA, Hubble

(http://seds.lpl.arizona.edu/nineplanets)

Below molecular hydrogen and helium layer, a layer of metallic hydrogen: - a liquid soup of ionized protons and electrons. - occurs for pressures > 4 x 109 Pa

10832 days

1 year = 10832 days1 day = 11 hours

Page 22: Where are we?

Jupiter:

Radius: 71,492 kmMass: 1.9x1027 kgOrbit: 7.8 x 108 kmMade of: hydrogen (90%),

helium (10%), ice, and rock

Atmosphere: yes Moons: 61

Day: 9.8 hoursYear: 4,333 days

Europa Io(http://seds.lpl.arizona.edu/nineplanets)

Page 23: Where are we?

http://www.alienalley.com/andrew1.html

An interior view

Page 24: Where are we?

http://www.alienalley.com/andrew1.html

An artist’s view!

Page 25: Where are we?

The Asteroid belt

Region where Jupiter’s gravity prevented formation of planetsMade of rock and ice.Largest object: Ceres (~950 km radius)

Frequent asteroid collisions a major Earth hazard…

Page 26: Where are we?

Mars:

Radius: 3,397 kmMass: 6.4x1023 kgOrbit: 2.3 x 108 kmMade of: rockAtmosphere: yes (CO2)Moons: 2

1 year = 78 days1 day = 25 hours

NASA & (http://seds.lpl.arizona.edu/nineplanets)

VallesMarineris

Page 27: Where are we?

Biggest bump in the solar system: Olympus Mons, 24km high!

Page 28: Where are we?

Mars contd:- machines on Mars...

Page 29: Where are we?

Victoria crater (true color), seen by Martian rover

Page 30: Where are we?

Martian landscapes

dunes

Gullies in a crater

Dust devils over dunes

Pockmarksin dry ice at the poles

Page 31: Where are we?

It’s a tough neighbourhood out there….

Phobos, moonof Mars

Page 32: Where are we?

Earth:

Radius: 6,678 kmMass: 5.9x1024 kgOrbit: 1.5 x 108 kmMade of: rockAtmosphere: yes (nitrogen, oxygen, argon)Moons: 1

Specific density 5.52

(http://seds.lpl.arizona.edu/nineplanets)

Densest planet insolar system

1 day = 25 hours1 year = 365.25 days

Page 33: Where are we?

Venus:

Radius: 6,052 kmMass: 4.9 x 1024 kgOrbit: 1.1 x 108 kmMade of: rockAtmosphere: yes (CO2)Moons: No

Surface pressure:90 atm

Surface temperature:~750K

1 year = 225 days1 day = 243 days!

Visible from space Surface

Venera 10

(http://seds.lpl.arizona.edu/nineplanets)

Page 34: Where are we?

Mercury:

Radius: 2,440 kmMass: 3.3x1023 kgOrbit: 5.8 x 107 kmMade of: rockAtmosphere: yes (unstable)Moons: No

Temperatures vary from 90K to 700K - largest range in solar system

(http://seds.lpl.arizona.edu/nineplanets)

1 year = 88 days1 day = 59 days!


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