The Solar System. Terms Ecliptic –Imaginary plane within which the 8 major planets orbit the Sun...
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Transcript of The Solar System. Terms Ecliptic –Imaginary plane within which the 8 major planets orbit the Sun...
The Solar System
Terms• Ecliptic
– Imaginary plane within which the 8 major planets orbit the Sun
– Apparent path of Sun across the sky as seen from Earth
PSCI 131: The Solar System
Terms: EclipticPSCI 131: The Solar System
From: Wikipedia.org
The Solar System• The Early Solar System• Overview• The Terrestrial Planets• The Jovian Planets• Dwarf Planets• Asteroids• Comets• Meteoroids
PSCI 131: The Solar System
The Early Solar System
The Early Solar SystemPSCI 131: The Solar System – The Early Solar System
From: jcconwell.wordpress.com
The Nebular Theory
The Early Solar SystemPSCI 131: The Solar System – The Early Solar System
Planets formed from collisions of smaller objects
The Nebular Theory
Solar System Overview
Overview of the Solar System• Sun: >99% of solar system’s mass
• Major planets– 4 terrestrial– 4 Jovian
• Dwarf planets– 5 recognized so far by IAU
PSCI 131: The Solar System – Overview
Overview of the Solar System• Asteroids, comets, meteoroids
– Leftover material from solar system formation– Fragments from collisions
• Dust, gas, radiation
PSCI 131: The Solar System – Overview
The 8 Major Planets
What Is A Major Planet?
• Spherical
• Orbits Sun
• Not a moon
• Has cleared its orbital path of other objects
PSCI 131: The Solar System
Major Planets and SunPSCI 131: The Solar System – The 8 Major Planets
The major planets, shown to scale
The Four Terrestrial Planets• “Terrestrial”: Earth-like• Mercury, Venus, Earth, Mars
PSCI 131: The Solar System – Terrestrial Planets
The terrestrial planets, shown to scale
From: wikipedia.org
The Four Terrestrial Planets
• Small• Rocky• Dense• Thin atmospheres• Short years• Long days• Main heat source: Sun
PSCI 131: The Solar System – Terrestrial Planets
EARTH VENUS
MARS MERCURY
From: wikipedia.org
MercuryPSCI 131: The Solar System – Terrestrial Planets
From: wwu.edu
From: wikipedia.org From: wikipedia.org
• Orbital period: 88 days
• Rotation period: 59 days
• Temp range: -270° F – 870° F
• Atmosphere: None
Venus
PSCI 131: The Solar System – Terrestrial Planets
Cloud cover of Venus.
From: ircamera.as.arizona.edu
Surface of Venus, photographed with cloud-penetrating radar. From: annesastronomynews.com
• Orbital period: 225 days
• Rotation period: 243 days
• Temperature: 900° F
• Atmosphere: 97% CO2
Earth
PSCI 131: The Solar System – Terrestrial Planets
Earth from low-altitude orbit.
From: astexhibits.com
Earth as seen from the Moon.
From: science1.nasa.gov
• Orbital period: 365.25 days
• Rotation period: 23 hr 56 min
• Temperature: 58° F (2012 average)
• Atmosphere: Nitrogen, oxygen, argon, water, CO2
Mars
PSCI 131: The Solar System – Terrestrial Planets
Mars from low-altitude orbit, showing atmosphere.
From: wikipedia.org
• Orbital period: 687 days
• Rotation period: 24 hr 37 min
• Temperature: -80° F (average)
• Atmosphere: Thin, CO2
MarsPSCI 131: The Solar System – Terrestrial Planets
Volcanoes and water ice clouds on Mars.From: jpl.nasa.gov
Olympus Mons volcano
Olympus Mons. Cliff at base is 5 miles high. Inset shows height compared to Earth mountains.From: wikipedia.org
The Four Jovian Planets• “Jovian”: Jupiter-like• Jupiter, Saturn, Uranus, Neptune
PSCI 131: The Solar System – Jovian Planets
The Jovian planets, shown to scale
From: cseligman.com
The Four Jovian Planets
• Large• Gas & ice• Low density• Long years• Short days• Main heat source: internal (from gravitational
compression)
PSCI 131: The Solar System – Jovian Planets
Jovian planets compared to the Sun and Earth (far right) Modified from: wikipedia.org
JupiterPSCI 131: The Solar System – Jovian Planets
Jupiter as it would look if it were the same distance from Earth as the Moon.
From: tholtz.com
• Orbital period: 12 years
• Rotation period: 9 hr 56 min
• Temperature: -234° F (cloud tops)
• Atmosphere: Hydrogen, helium
From: photojournal.jpl.nasa.gov
Jupiter’s Atmosphere
PSCI 131: The Solar System – Jovian Planets
Cross-section of Jupiter compared with Earth. 125°K is about -234°F; 2000°K is about 3100°F.
• Mostly H and He
• Would have become a sun if it had been bigger
• Pressure within atmosphere is high enough to make liquid and metallic hydrogen
Jupiter: The Great Red SpotPSCI 131: The Solar System – Jovian Planets
High-res photo of the Great Red Spot, an ancient storm the size of three Earths.
SaturnPSCI 131: The Solar System – Jovian Planets
Saturn imaged by the Cassini-Huygens spacecraft, 2008. From: nasa.gov
• Orbital period: 30 years
• Rotation period: 10 hr 30 min
• Temperature: -288° F (cloud tops)
• Atmosphere: Hydrogen, helium
Saturn’s rings and Earth, taken by Cassini-Huygens spacecraft, 2008. From: nasa.gov
Earth as seen from Saturn
Saturn’s Moon TitanPSCI 131: The Solar System – Jovian Planets
Comparison of Titan with Earth and Earth’s moon.
• Atmosphere: Nitrogen, methane
•Only moon known to have an atmosphere
• Bodies of stable liquid on surface
•Methane, ethaneTitan’s surface. From: nasa.gov
• Orbital period: 84 years
• Rotation period: 17 hr 14 min
• Temperature: -357° F (cloud tops)
• Atmosphere: Hydrogen, helium, frozen ammonia and methane
•Rotates on its side:
UranusPSCI 131: The Solar System – Jovian Planets
Uranus showing rings and cloud
bands. From: nasa.gov
Axis
• Orbital period: 165 years
• Rotation period: 16 hr 7 min
• Temperature: -392° F (cloud tops)
• Atmosphere: Hydrogen, helium, frozen ammonia and methane
NeptunePSCI 131: The Solar System – Jovian Planets
Neptune with cloud bands, cirrus clouds (white) and storm systems (dark spots). From: nasa.gov
The Dwarf Planets
PSCI 131: The Solar System
What Is A Dwarf Planet?
• Spherical
• Orbits Sun
• Not a moon
• Has NOT cleared its orbital path of other objects
PSCI 131: The Solar System
Five Recognized Dwarf Planets(Listed in order of decreasing size)
• Eris• Pluto• Makemake• Haumea• Ceres
• All are located in “debris belts”
PSCI 131: The Solar System – Dwarf Planets
Debris Belt LocationsOrbit of Earth
Orbit of MarsASTEROID
BELT
SUN
KUIPER BELT
Orbit of Uranus
Orbit of Neptune
Debris Belt Locations
ASTEROID BELT
KUIPER BELT
Orbit of Uranus
Orbit of Neptune OORT CLOUD
Five Recognized Dwarf Planets
• Eris: Kuiper Belt• Pluto: Kuiper Belt• Makemake: Kuiper Belt• Haumea: Kuiper Belt• Ceres: Asteroid Belt
• Oort Cloud: No recognized dwarf planets; trillions of comets
PSCI 131: The Solar System – Dwarf Planets
The Smaller Objects: Asteroids, Comets, &
Meteoroids
PSCI 131: The Solar System
Asteroids• Size: 10s to 100s of miles
• Shape: Irregular
• Composition: Rock, metal
• Atmosphere: None
• Location: Mostly in Asteroid Belt between Mars and Jupiter
PSCI 131: The Solar System – Smaller Objects
(doesn’t look like this)
PSCI 131: The Solar System – Smaller Objects
The Asteroid Belt
What Does the Asteroid Belt Look Like?
PSCI 131: The Solar System – Smaller Objects
It’s mostly empty space
Asteroids: Earth CrossersPSCI 131: The Solar System – Smaller Objects
Comets• Size: average diameter about 5 miles
• Shape: Irregular
• Composition: Ice, rock & metal fragments
• Atmosphere: None
• Location: Kuiper Belt & Oort Cloud
PSCI 131: The Solar System – Smaller Objects
Halley’s Comet, 1986
From: dailygalaxy.com
CometsPSCI 131: The Solar System – Smaller Objects
Structure of a comet
CometsPSCI 131: The Solar System – Smaller Objects
A comet’s coma and tail only form near the Sun. The tail always points away from the Sun.
CometsPSCI 131: The Solar System – Smaller Objects
Comet Shoemaker-Levy struck Jupiter in 1994.
Meteors• Size: sand grain
(average)
• Composition: Rock, metal
PSCI 131: The Solar System – Smaller Objects
Meteors• Meteor: within a planet’s atmosphere
• Meteorite: has struck the ground
• Meteoroid: still in space
PSCI 131: The Solar System – Smaller Objects
The Chelyabinsk “Meteor”, February 15, 2013
• Approx. mass: 11K tons • Approx. size: 60 ft• Velocity: 41K mph• Altitude of airburst: 76K feet• Energy: 500K tons of TNT• Injuries: 1,491• Damage: 7,200 buildings
PSCI 131: The Solar System – Smaller Objects
VIDEO: Chelyabinsk meteor airburst and building damage