How did this get Here?.

Slides:



Advertisements
Similar presentations
Chapter 6 The Earth and Moon. Distance between Earth and Moon has been measured to accuracy of a few centimeters using lasers (at McDonald Observatory)
Advertisements

The Earth and moon viewed from Mercury The Earth viewed from Saturn.
Solar System Physics I Dr Martin Hendry 5 lectures, beginning Autumn 2007 Department of Physics and Astronomy Astronomy 1X Session
Earth has formed in our solar system  We need to understand planetary formation Constraints: Astronomical observations Study of meteorites Study of planets.
This Set of Slides This set of slides covers age and formation of solar system, exoplanets. Units covered: 33, 34.
Lunar Facts The moon ended its formation period approximately 4 billion years ago. After the period of formation, the surface of the moon continued to.
Origin of the Moon September 1, 2010 Bonnie Meinke September 1, 2010 Bonnie Meinke.
Theories of the Origin of the Moon. Theory One early theory was that the moon is a sister world that formed in orbit around Earth as the Earth formed.
How was Luna formed and how does she affect and interact with both Earth and Sol?
Earth and Moon Statistics By the Lunar and Planetary Institute For use in teacher workshops.
Lesson 8a Moons, Asteroids and Rings. Europa These interactions also keep Europa in a slight elliptical orbit as well. But since Europa is farther from.
Formation of the Solar System
Formation of the Solar System Chapter 27 page 684-
Pre-solar nebula Protoplanetary disk: condensation and accretion Solar wind (beginning of fusion) Collisions continue Planetary migration (orbits shifting)
The Moon Formation. Lunar Facts The moon ended its formation period approximately 4 billion years ago. After the period of formation, the surface of the.
Bellringer What phase of the moon must be occurring for you to be able to witness a total solar eclipse?
Week 10 Day 1 Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break .
The Origin of the Solar System. In the beginning, we started out looking like this, just a huge cloud of gas in space….
Moon Lesson 3 Formation of the Moon. More detail on the lunar composition The Moon’s bulk composition is similar to the Earth’s but not identical. The.
Origin of the Moon 2 September 2015.
Origin of Our Solar System
Late Work Due 12/20/13 Remember ain’t no butts about it! Sticking your head in the sand won’t make the deadlines go away 11 Days Remain.
Earth’s Moon How did our Moon form? and What’s been happening since?
Section 11: More on Tidal Forces
Phases and Appearance. Ground Based Observations Moon has light and dark areas on it Light and dark not randomly distributed There are a few bright.
How was Earth formed?. Big Bang Theory 13.7 billion years ago 13.7 billion years ago Creation of all matter Creation of all matter Hydrogen and Helium.
The History of the Earth. We know how the Earth and Solar System are today and this allows us to work backwards and determine how the Earth and Solar.
Thought Question What does the solar system look like as a whole? Why does the solar system look the way it does? Can we explain how the solar system.
Chapter 6: Terrestrial Planets -The Moon. Earth’s interior is revealed by seismology, the study of earthquakes. Layers are revealed: A layered object:
The Moon Several theories have been proposed to explain the origin of the Moon.
© 2017 Pearson Education, Inc.
Newton’s laws & gravity & tides
5 lectures, beginning Autumn 2007
© 2017 Pearson Education, Inc.
Our Moon! …done that…) (Been there….
Theories of Formation for the Moon
The Origin of the Solar System
Making Our Solar System: Planetary Formation and Evolution
The Moon “Jupiter! I did a song! You ain’t got one!” "Camembert?"
Respond to the following: How did the moon get there?
Why do we have a satellite?
Origin of the Moon 22 September 2017.
Ch. 8: Earth as a Planet.
Evolution of the Early Earth
THE MOON.
Chapter 7 The Moon.
EARTH'S MOON: LUNA.
Our Moon 4.5 Billion Years Ago
Earth’s Moon a Describe daily changes due to rotation, seasonal changes due to the tilt and revolution of the Earth, and tidal impact due to the.
Notes The Moon.
Origin of the Moon 13 February 2018.
Bell Ringer What is the order of the planets?
Origin of the Solar System
Chapter 7 The Moon.
The Formation of the Solar System
The Moon.
What remnants of early solar system structure remain?
The Jovian Planets Huge worlds, heavily mantled in gas at the time of the formation of the Solar System.
Origin of the Moon 11 September 2018.
Rising Carbon Dioxide Levels
Respond to the following: How did the moon get there?
The Moon (Phases, Eclipses, and Tides)
3A Objectives Describe the nebular theory in detail.
Origin of the Moon 12 February 2019.
Formation Theories.
Reading: Chapter 11: Gas Giants
The Moon Topographic map from Lunar Reconnaissance Orbiter.
Q due Thursday, March 3, 6:00 pm.
Presentation transcript:

How did this get Here?

Why is that question? The earth has a bulk density of 5.5 grams per cubic centimeter. This density reflects the composition of material at the location in the solar system where the Earth was assembled via accretion. Logically one would therefore expect the moon to the have the same density  However, the moon has a density of 3.3 grams per cubic centimeter. The moon is also an anomaly because its mass compared to the earth is 1/80 and there is very large for a planetary satellite

So the moon did not co-form with the Earth Possibilities for Lunar Origin: The moon formed by accretion somewhere else in the solar system where the material would form an object with a density of ~3.5 g/cc. So where would this place be? In the vicinity of Mars  okay how the hell did it get here then? It separated out of the Earth after the Earth formed and differentiated? Since the mantle of the Earth has a density of 3.5 g/cc then the overall composition of the Moon must be like that of the Earth’s mantle. But what is the mechanism that would cause this separation? This was a mysterious problem for about 30 years until finally, computer simulations improved to the point that offered a plausible explanation.

Earth Encounter between Molten Earth and Mars size Planetesimal Step 1: The Mars planetesimal is poised to strike the molten protoplanet earth which has already differentiated

Step 2: The impact into the molten earth sends large molten lumps of debris out of the earth - mostly from the middle layers of the differeniated earth.

Step 3: The debris ring of molten ejecta coalesces, by accretion, into a single object. The density of that object would be similar to the density of the middle layers of the earth (e.g. about 3.5 grams/cc). In computer numerical models, this coalescence occurs fast, on a timescale of about 100 million years.

The problem with this scenario is that the probability of a direct collision is small. However, the same result can occur if there is not a direct collision but instead there is a close passage by the Mars sizes object. Here is the Sequence if it was a close passage as shown below:

Step 1: A tidal force is exerted on the molten earth which causes an obvious deformation.

Step 2: The deformation actually separates from the earth initially as a whole molten blob whose composition again reflects the middle layers of the Earth

Step 3: However, this molten blob is gravitationally perturbed by the combined forces of the Earth and the still near Mars size object so it distengrates into a debris ring.

After a 100 million years or so, the debris ring has coalesced into the moon, and the Earth has cooled so that water vapor in its atmosphere (combined with bombardment by comets) has produced the oceans

Since the moon formed from the condensation of a debris ring in relatively near-earth orbit, the moon was initially quite close to the earth. At this time (4.6 billion years ago) the earth was rotating quite rapidly (about once every 5 hours). The nearby moon exerted large tidal forces on oceans which acts a source of friction slowing down the rotation of the Earth. This process continues to day. To conserve total system angular momentum, the response of the moon is then to move farther away from the earth at a rate of 3.8 cm per year.