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Solar System Overview FYI … Distance Not To Scale …
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Solar System Overview

Feb 23, 2016

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Jenis

Solar System Overview. FYI … Distance Not To Scale …. The Sun. At the Center (and we do go around it …..) 99.85% mass of Solar System 92% H / 8% He Source of solar wind and space weather. Inner Planets. “Terrestrial Planets” Rocky Dense Metal cores (iron). - PowerPoint PPT Presentation
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Page 1: Solar System Overview

Solar System Overview

FYI … Distance Not To Scale …

Page 2: Solar System Overview

The Sun• At the Center (and we do go

around it …..)

• 99.85% mass of Solar System

• 92% H / 8% He

• Source of solar wind and space weather

Page 3: Solar System Overview
Page 4: Solar System Overview

Inner Planets• “Terrestrial

Planets”• Rocky• Dense• Metal cores (iron)

Page 5: Solar System Overview

Asteroids

• “Minor planets” or “planetoids” or “planetesimals” less than 1000 km across

• Asteroid Belt between Mars and Jupiter

• Occasionally run into Earth and other planets (oops)

Ida

Encountered on Aug 28th, 1993 by the Galileo Spacecraft, en route to Jupiter

Dactyl

Page 6: Solar System Overview

Asteroids• Asteroids -> Meteoroid -> Meteor -> Meteorite

1000-10 km -> 10m-100 µm -> space rock trapped by gravity (burning up) -> space rock that actually hits the surface of a

planet

Page 7: Solar System Overview
Page 8: Solar System Overview

Meteoroid fragment discovered in Argentina; on display at the Museum of Nature, Ottawa, Canada

Page 9: Solar System Overview
Page 10: Solar System Overview

Barringer Crater (Canyon Diablo)

1.2 kilometers wide170 m deep

~ 50 000 years ago

Used by NASA during the 1960’s to prepare for moon landing

Winslow , Arizona

Page 11: Solar System Overview

Outer Planets

• Large!• Gases and liquids• No solid surface• May have a small solid core• Tumultuous atmospheres - rapid winds,

large storms• Rotate relatively quickly

Page 12: Solar System Overview

Kuiper Belt

• Disk of debris at the edge of our Solar System

• Pluto is a KB Object (sorry!)

• Source of short-period comets

Page 13: Solar System Overview
Page 14: Solar System Overview

Oort Cloud

• A hypothesized sphere of comets surrounding the inner solar system and the kuiper belt

• ~50 000 AU from the Sun

• Helps in explaining the regularity of comets within the Solar System

Page 15: Solar System Overview
Page 16: Solar System Overview

Inner Planets!

Page 17: Solar System Overview

• Smallest planet (0.4 Earth diam)

• Closest to Sun, moves around fastest (88 days)

• Surface -173 to 427 ºC• ? Ice Caps – no tilt of axis so

poles are cold• No atmosphere• Mariner 3 fly-bys in 1974 and

1975 – 40% of surface mapped

Mercury#1, Coffee Bean

Page 18: Solar System Overview

What are these?How did they form?

Page 19: Solar System Overview
Page 20: Solar System Overview

Venus#2, Large Blueberry

• Nearly the same size as Earth (.95)

• Slowest rotation of any planet (243 days)

• Spins backwards

• Surface temp 377 to 487 C

• Cloud covered – radar observations

• Dry!• Very thick atmosphere mostly

CO2• Surface pressure is 100 times

higher than Earth’s• Runaway greenhouse

Can see it in the night sky without a telescope!

Page 21: Solar System Overview

Why is Venus hotter than Mercury?

Page 22: Solar System Overview

Earth#3, Cherry

7900 mile (12756 km) diameter

23.5 degree axis tilt (seasons!)

Surface temps –73 to 48 C

Thick atmosphere, mild greenhouse effect

Liquid water – lots! - at surface

Can see it without a telescope!

Page 23: Solar System Overview

Geologically active?Core, mantle, crustMagnetic field?

Page 24: Solar System Overview

Who Cares About a Magnetic Field?We do!

Page 25: Solar System Overview

Aurora Borealis

Page 26: Solar System Overview

Aurora Austrailus

Page 27: Solar System Overview

6794 km diameter (4,220 miles) – about ½ of Earth’s

25 degree axis tilt (seasons!)

Rotates once every ~24 hours and orbits the Sun once every 687 days

Very cold -83 to -33 C (-117 to -27 F)

Thin atmosphere, 95% CO2, & 3% N

Iron Oxide covers its surface (RED)

Two small moons - Phobos (Fear) and Deimos (Terror)

Hosting 5 functioning spacecrafts: Mars Odyssey, Mars Express, Mars Reconaissance Orbiter, Mars Rover: Opportunity and Curiosity

Liquid water cannot exist on the surface of Mars due to low atmospheric pressure, except at the lowest elevations for short periods

Mars#4, Pea

Can see it in the night sky without a telescope!

Page 28: Solar System Overview

North

Page 29: Solar System Overview

South

Page 30: Solar System Overview

The Gas Giants

Page 31: Solar System Overview

• 89,000 miles (143,000 km) diameter – 11x Earth• 2x mass of all other planets combined (318 x Earth);

100 pounds on Earth = 254 on Jupiter• 90% H and 10% He (75/25% by mass) • Methane, water, ammonia, rock • Rocky core – liquid metallic hydrogen – electrical

conductor, generates magnetic field• Similar to Solar Nebula

Jupiter#5, Small Cantaloupe

Page 32: Solar System Overview

• Cloud-tops average = -153°C = -244°F. • 10 hour rotation / 12 year orbit• Fly-bys: Pioneer 10, 11, Voyager 1, 2, Ulysses,

Cassini• Orbiter: Galileo – 8 years (recently “visited”

the planet), Probe

JupiterCan see it in the night sky without a telescope!

Page 33: Solar System Overview

Giant Red Spot – at least 300 years old

3 x size of EarthWinds up to 400 km /

hr“Jr”

Storms on Jupiter

Page 34: Solar System Overview

Why Doesn’t Jupiter Blow Up?

Page 35: Solar System Overview

• 9x the size of Earth• 75% hydrogen and 25% helium • Water, methane, ammonia and "rock“• Rocky core• Winds up to 500 m / second• -290 F• Rings – 185,00 miles wide / /2 mi thick• Water ice in rings• 56 moons and counting• 11 hour rotation / 29 year orbit• Pioneer / Voyager Fly-by / Cassini/Huygens!

Saturn#6, Large Orange

Page 37: Solar System Overview

False Color

Rather chilly in the rings

Red: -261 F Blue -333 F

Green -298 F

Dirty Snow

Turquoise= water iceRed = “dirty”

Page 38: Solar System Overview

Titan!Clues to Early Earth?

Page 39: Solar System Overview

Earth

Titan

Page 40: Solar System Overview

TitanClues to Early

Earth?

Average surface temperature –179CAtmosphere of N (>90%), CH4, ArHydrocarbon-rich rivers/seas (ethane – C2H6)Water iceAtmosphere 1.5 x Earth

Page 41: Solar System Overview

Uranus# 7, Kiwi First planet discovered with a telescope!

Page 42: Solar System Overview

Uranus• 4x the size of Earth• 15% H, little helium – mostly ices• Uniform through out; no rocky core• Blue from methane absorption of red light (atmosphere) atmosphere has mostly hydrogen and helium• 11 rings, 27 satellites• -350 F at surface• 18 hour rotation, 84 year orbit• Spins on an axis inclined almost 90 degrees• Voyager fly-by

Page 43: Solar System Overview

Neptune#8, Apricot or nectarine

Page 44: Solar System Overview

Neptune• Ices and rock - 15% H and little He• H, He, methane atmosphere (blue!)• Uniform through out; small rocky

core?• Had storm “Great Dark Spot” MIA

since Voyager 2• Pretty Good White Spot (Scooter)

zipped around every 16 hours….• 4 Rings – unknown composition• 13 moons• 18 hour rotation / 165 year orbit• Voyager (1989)

Page 45: Solar System Overview

PlutoGrain of Rice

Page 46: Solar System Overview

Pluto • Diameter - 1,413 miles (2274 km) - 2/3 size of Earth’s Moon

• Rotation: 6 1/3 days• Orbit: 248 years highly elliptical• Sometimes is inside Neptune’s orbit (20 yrs)• Light from Sun takes 5.5 hours to reach it• Surface of water and methane ice, frozen

nitrogen• When closer to the Sun, heat produces an

atmosphere

Page 47: Solar System Overview

Is Pluto a Planet?• Orbits a star• Round• Not a star or a moon• “Cleared Out”/ “Dominates” its orbit

What Makes a Planet a Planet?

Page 48: Solar System Overview

Is Pluto a Planet?Yes No

It has always been considered a planet

Very smallVery elliptical orbitOut of plane of eclipticSame material as Kuiper belt objectsFound other “non-planets” that were larger

Page 49: Solar System Overview

August 24th, 2006

Page 50: Solar System Overview

New Horizons:Pluto-Kuiper Belt Mission

• January 2006 Launch!• July 2015 – Pluto!• 2016-2020 – Kuiper Belt

Page 51: Solar System Overview

Comets• Dirty snowballs - small objects of ice,

gas, dust, tiny traces of organic material

Page 52: Solar System Overview

Comet Parts

Nucleus, ComaDust tail – white, “smoke,” reflects sun. 600,000 to 6 million miles longIon tail – Solar UV breaks down CO gas, making them glow blue. 10’s of millions of miles

Page 53: Solar System Overview

Hale-Bopp Comet

First seen on July 23rd, 1995

• Read section 28.3• Q: 2, 3

• Read section 28.4• Q: 2, 3, 4, 5