310 likes | 325 Views
Explore the formation of our solar system using data from the Lunar and Planetary Institute. Learn about planet orbits, rotations, and differentiation, and discover how the solar nebula evolved into our diverse planetary system over billions of years. Engaging images and activities for teacher workshops included.
E N D
Formation of Our Solar System By the Lunar and Planetary InstituteFor Use in Teacher Workshops Image: Lunar and Planetary Laboratory
Some data to explain: 1. Planets isolated 2. Orbits ~circular / in ~same plane 3. Planets (and moons) travel along orbits in same direction…. same direction as Sun rotates (counter-clockwise viewed from above) Lunar and Planetary Institute image
Some more data to explain: 4. Most planets rotate in this same direction Mercury 0° Venus 177° Earth 23° Mars 25° Jupiter 3° Saturn 27° Uranus 98° Neptune 30° NASA images edited by LPI
And some more data to explain: 5. Solar System highly differentiated: Terrestrial Planets (rocky, dense with density ~4-5 g/cm3) Jovian Planets (light, gassy, H, He, density 0.7-2) Images: Lunar and Planetary Laboratory
How Did We Get a Solar System? Image: LPI Huge cloud of cold, thinly dispersed interstellar gas and dust – threaded with magnetic fields that resist collapse Hubble image
How Did We Get a Solar System? Image: LPI Concentrations of dust and gas in the cloud; material starts to collect (gravity > magnetic forces) Hubble image
How Did We Get a Solar System? Gravity concentrates most stuff near center Heat and pressure increase Collapses – central proto-sun rotates faster (probably got initial rotation from the cloud) Image: LPI
How Did We Get a Solar System? • Rotating, flattening, contracting disk - solar nebula! Equatorial Plane Orbit Direction NASA artwork
How Did We Get a Solar System? • After ~10 million years, material in center of nebula hot enough to fuse H • “...here comes the sun…” NASA/JPL-Caltech Image
How Did We Get a Solar System? • Metallic elements (Mg, Si, Fe) condense into solids at high temps. Combined with O to make tiny grains • Lower temp (H, He, CH4, H2O, N2, ice) - outer edges Planetary Compositions Hubble photo
How Did We Get a Solar System? Inner Planets: • Hot – Silicate minerals, metals, no light elements, ice • Begin to stick together with dust clumps Image: LPI
How Did We Get a Solar System? • Accretion - particles collide and stick together … or break apart … gravity not involved if small pieces • Form planetesimals, up to a few km across Image: LPI
How Did We Get a Solar System? • Gravitational accretion: planetesimals attract stuff • Large protoplanets dominate, grow rapidly, clean up area ( takes ~10 to 25 My) Image: LPI
How Did We Get a Solar System? Outer Solar System • Cold – ices, gases – 10x more particles than inner • May have formed icy center, then captured lighter gases (Jupiter and Saturn first? Took H and He?) Image: LPI
How Did We Get a Solar System? The Asteroid Belt ? Should have been a planet instead of a debris belt? Jupiter kept it from forming Eros image
How Did We Get a Solar System? Beyond the Gas Giants - Pluto, Charon and the Kuiper Belt objects Chunks of ice and rock material Little time / debris available to make a planet – slower!!
Early in the Life of Planets • Planetesimals swept up debris • Accretion + Impacts = HEAT • Eventually begin to melt materials • Iron, silica melt at different temperatures • Iron sank – density layering Image from LPI
Pause to recall the Play Doh accretion activity But wait, there’s more …. We can differentiate!
When did Our Solar System Form … How do We Know? Image: Lunar and Planetary Laboratory
When Did the Solar System Form? • 4.56 billion years ago • How do we know? (evidence for formation) • Lunar samples - 4.5 to 4.6 Ga • Meteorites - 4.56 Ga • Earth – 3.9 (or 4.4 Ga) Lunar meteorite Meteorite photo by Carl Allen
Earliest history of Solar System - chemical and physical info about formation and building blocks of planets (rest of stuff was pulled into the Sun or other planets….) Sample Return 1/15/2006 • Stardust Passed through Comet Wild 2 Coma 1/2004 Stardust image
We Can Also Look Around …. Close-up of "Proplyds" in Orion Thanks Hubble! Hubble images
Comets • Dirty snowballs - small objects of ice, gas, dust, tiny traces of organic material
Comet Parts Image credit: K. Jobse, P. Jenniskens and NASA Ames Research Center Nucleus, Coma Dust tail – white, “smoke,” reflects sun. 600,000 to 6 million miles long Ion tail – Solar UV breaks down CO gas, making them glow blue. 10’s of millions of miles
Naming Comets NASA/ JPL image of Comet Halley
What’s in a Tail? Image credit: K. Jobse, P. Jenniskens and NASA Ames Research Center