03/30/16 The moon has much lower average density than Earth or the other terrestrial planets & almost no core. It’s a lot like Earth’s mantle. http://www.8planets.co.uk/the-planets.

Slides:



Advertisements
Similar presentations
Impact Cratering Dating Nathan Marsh. Relative Dating Simple but not as informative Measures the crater densities (craters per square kilometer) Generally.
Advertisements

Interior structure, origin and evolution of the Moon Key Features of the Moon: pages
Moon rocks, dust and lunar meteorites Key Features of the Moon: pages and
25.1 ORIGIN AND PROPERTIES OF THE MOON
How are they different? By the Lunar and Planetary Institute For use in teacher workshops Moon Formation / Processes.
The Moon Astronomy 311 Professor Lee Carkner Lecture 13.
The Moon Astronomy 311 Professor Lee Carkner Lecture 13.
The Moon Astronomy 311 Professor Lee Carkner Lecture 13.
Yen-Shan Lim PTYS 395 October 16, The Concepts of Maria Maria – dark, smooth, low plains (occupy 16% of the lunar surface area) Before space age,
Hydrogen isotope ratios in lunar rocks indicate delivery of cometary water to the Moon Greenwood, James P., et al. Presented by Patrick Harner.
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 10 Our Barren Moon CHAPTER 10 Our Barren Moon.
Section 1: Earth’s Moon Preview Key Ideas Exploring the Moon
Moon, Moon Phases & Eclipses. The Moon Calendar The current standard calendar is solar calendar (Gregorian calendar) – counting days The moon phases.
Chapter Four The Moon: The Earth’s Closest Neighbor.
Formation of the Moon What properties were known about the moon prior to Apollo? Orbital Period Mass and Size and therefore Density Gravity was 1/6 as.
Our Barren Moon Chapter Ten. Guiding Questions 1.Is the Moon completely covered with craters? 2.Has there been any exploration of the Moon since the.
I. The Highlands  Surface feature that is light in color, high in elevation (mountainous), and heavily cratered.
List all the characteristics you can think of about the moon?
8 TH GRADE SCIENCE THE MOON. HOW WAS THE MOON FORMED? It is about 4.6 billions years old. (Same age as Earth) Scientists have measured the age of the.
Our Barren Moon Chapter Ten. Guiding Questions 1.Is the Moon completely covered with craters? 2.Has there been any exploration of the Moon since the Apollo.
Chapter 22 Section 3 Earth’s Moon. Earth vs. Moon 3,475 km 12,756 km Earth has 1 natural satellite  the Moon No specific name other than Moon Unusual.
The Earth as a Terrestrial Planet Mass -- 6 x gm (6 x kg) Size -- diameter 12,756 km (eq.) Density – mean 5.5 gm/cm 3 Surface -- 71% water.
The Moon Chapter 10. The Earth Moon System Primary Surface Features.
Part II: Solar System The Moon Audio update: 2014Feb23.
Sampling Moon Rocks. Why do we have seasons? Explain. The tilt of the Earth. There are times of the year where the southern hemisphere is tilted more.
The Earth’s Moon The Earth’s Moon. Satellites Definition: Any body that orbits a larger body Definition: Any body that orbits a larger body 1957: First.
The Moon.
 Satellite – an object that orbits a more massive object  Ex: The Moon  Ex: Moons of other planets  Many of the planets have satellites.
Earth’s Moon How did our Moon form? and What’s been happening since?
Earth’s Moon - Luna. Lunar surface features There are 5 basic surface features.
American Unmanned Mission: Surveyor ( )
John Young from Apollo 16, April 1972 Lunar Geology.
Universe Tenth Edition Chapter 10 Our Barren Moon Roger Freedman Robert Geller William Kaufmann III.
Exploring NASA’s Moon Rocks, Lunar Soil Samples & Meteorite Disks!!
Lunacy. Revolution :365 days Rotation: 24 hours Gravity: 9.8 m/s 2 Surface temps –73 to 48 C (- 100 to 120F) Thick atmosphere, mild greenhouse effect.
A look at our nearest neighbor in Space! The Moon.
A look at our nearest neighbor in Space! The Moon Free powerpoints at
The Moon The Earth's moon is not the largest satellite in the solar system. However, it is closer in size to its planet than any other satellite (with.
A look at our nearest neighbor in Space! The Moon.
Mission: Moon!. What is it like on the Moon? Length of Day Atmosphere Temperature Water Radiation Gravity Landscape.
EARTH’S MOON.  Structure  3,476 km in diameter  1/18 the mass of the Earth  No air or liquid water  Temperature range: 100◦C to -120◦C (212◦F to.
 The only natural satellite of our planet is the moon, named “The Moon”  Some publications will refer to it as “Luna”
Moon Notes Chapter 2 Section 2.
Lunar Evolution: A “Life Story” View of the Moon
Exploring the Moon.
Respond to the following: How did the moon get there?
The Moon.
The Earth as a Terrestrial Planet
Chapter 9 Review BAAM!.
Geology of the Moon, Mercury, and Mars
Late Heavy Bombardment
The Moon 28.2.
The Moon Chapter 10.
Section 1: Earth’s Moon Preview Key Ideas Exploring the Moon
22.3 – Earth’s Moon.
The Earth as a Terrestrial Planet
Section 1: Earth’s Moon Preview Key Ideas Exploring the Moon
The Moon November 11, 2018.
Rock and Roll at the Apollo 17 Site
Section 2: The Moon The Moon, Earth’s nearest neighbor in space, is unique among the moons in our solar system. K What I Know W What I Want to Find Out.
The Moon Astronomy 311 Professor Lee Carkner Lecture 13.
Lunar rocks: witnesses to the ancient history of the solar system
Respond to the following: How did the moon get there?
Section 1: Earth’s Moon.
40Ar-39Ar Dating of Apollo Impact Melts- Searching for Imbrium
Surface Rocks - There are basically two kinds of surface rock on the Moon.
Global Elemental Maps of the Moon: The Lunar Prospector Gamma-Ray Spectrometer by D. J. Lawrence, W. C. Feldman, B. L. Barraclough, A. B. Binder, R. C.
The Moon – Earth’s Natural Satellite
Apollo and Beyond cont..
Chapter 25 – The Moon Section 25.1
Presentation transcript:

03/30/16 The moon has much lower average density than Earth or the other terrestrial planets & almost no core. It’s a lot like Earth’s mantle. http://www.8planets.co.uk/the-planets Stevenson, Making the Moon, Physics Today, Nov 2014 1

2 http://www.makingthemodernworld.org.uk/learning_modules/maths/06.TU.02/?section=11

The six Apollo landings which took place between 1969 and 1972 provided scientists with huge amounts of lunar data in the form of photography and orbital experiment results, sample collections and surface operations http://www.lpi.usra.edu/lunar/missions/apollo/. 3

Apollo Lunar Surface Experiments Package (ALSEP) 4

http://www. spacesafetymagazine http://www.spacesafetymagazine.com/aerospace-engineering/nuclear-propulsion/infographic-atomic-batteries-deep-space-missions/ 5

The terrestrial record shows high attenuation, whereas the lunar seismogram shows intense scattering due to the fractured regolith and very weak attenuation due to the lack of intergranular water 6

7

03/30/16 Highlands – Anorthosite: intrusive igneous rock characterized by a predominance of plagioclase feldspar Apollo 16 landing site 4.19 Ga 8 http://airandspace.si.edu/exhibitions/attm/wl.an.1.html http://www.psrd.hawaii.edu/April04/lunarAnorthosites.html 8

Largest nearside basin - formed ~ 0.5 Ga before basalt 03/30/16 Mare basalt – 3.3 Ga Apollo 15 landing site Mare Imbrium Largest nearside basin - formed ~ 0.5 Ga before basalt https://ase.tufts.edu/cosmos/print_images.asp?id=5 9 9

https://ase.tufts.edu/cosmos/print_images.asp?id=5 03/30/16 10 https://ase.tufts.edu/cosmos/print_images.asp?id=5 10

Press & Siever 11

Stevenson, Making the Moon, Physics Today, Nov 2014 12