Two Billion Years of Magmatism in One Place on Mars

Slides:



Advertisements
Similar presentations
The Terrestrial Planets
Advertisements

What caused Mt. St. Helen’s to erupt?
Interior structure, origin and evolution of the Moon Key Features of the Moon: pages
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)
Earth Science 10.1 Volcanoes and Plate Tectonics
STRUCTURE OF THE EARTH Noadswood Science, 2011.
Mega-volcano movie lab M. How can evidence gathered by different scientists around the world support the existence of a mega volcano in the prehistoric.
VOLCANIC HAZARDS ASSESSMENT Human-based Data Sources Geochemical Data Geophysical Data.
Time to Solidify an Ocean of Magma The Moon melted when it formed. How long did it take.
Magma Ocean Solidification: Oldest Lunar Zircon COSMOCHEMISTRY iLLUSTRATED Time to Solidify an Ocean of Magma The Moon melted when it formed. How long.
1 Lecture #02 - Earth History. 2 The Fine Structure of The Universe : The Elements Elements are a basic building block of molecules, and only 92 natural.
Chips Off an Old Lava Flow Lava flows with compositions like those of mare basalts began to form before.
TOPS Top 10 Geography in conjunction with How come the most volcanic place on Earth is nowhere near a.
Chapter 3 – Volcanoes.  Volcanic belts from along the boundaries of Earth’s plates.  There are 600 active volcanoes on land and many more beneath the.
Earth’s Layered Structure
Unit D Vocabulary Howard Middle School 6 th grade Earth Science.
Moons Features and Phases Chapter 28. General Information Satellite: a body that orbits a larger body. Seven planets in our solar system have smaller.
Lesson2c – Plate tectonics The Effects of Plate Tectonics.
The Earth’s Structure. Inside the Earth Age of the Earth- Believed to be 4.6 Billion Years Old! Core: The center of the earth that consists of very hot.
Copyright © 2014 All rights reserved, Government of Newfoundland and Labrador Earth Systems 3209 Unit: 4 The Forces Within Earth Reference: Chapters 4,
Miss Nelson SCIENCE ~ CHAPTER 6 VOLCANOES. Volcanoes and Plate Tectonics SECTION 1.
Learning Goals Identify locations where volcanoes are most likely to form. Explain the factors involved in volcanic eruptions. Evaluate the features.
Mars clays may have volcanic source Deposits didn’t need flowing water to form, new research suggests By Erin WaymanErin Wayman Web edition : Sunday, September.
Volcanoes
Over the last 100,000 years – an extremely uncertain story.
Volcanic Activity Earth Science Mr. Barry.
Chapter 7 Volcanoes.
What Causes Volcanoes? 11/9/ pgs IN: What causes volcanoes?
The Principles of Planetary Geology By: Katie McCormick and Kyle Lennox.
Volcanoes This power point has facts which are based on volcanoes.
Volcanoes. Ag Earth Science – Chapter 10.1 viscosity A measure of a fluid’s resistance to flow.
Tectonic Landscapes: Hotspots
How come the most volcanic place on Earth is nowhere near a plate margin? TOPS Top 10 Geography in conjunction with
Plate Tectonics Earth Science.
Plate Tectonics Sea-floor Spreading.
Leah Salditch February 27, 2017 Mars Final Project
Meteorite Formation Times and the Age of Jupiter
Learning Goals Identify locations where volcanoes are most likely to form. Explain the factors involved in volcanic eruptions. Evaluate the features.
More Evidence for Plate Tectonics
Changes to Earth.
#14 Hotspots and Magnetic Reversals Notes
Volcanism and an Ancient Atmosphere on the Moon
Magnesium-rich Basalts on Mercury
Primeval Water in the Earth
Magnesium-rich Basalts on Mercury
Exploring Mars: The Inside Story
The Importance of When Two important age studies of Martian meteorites: Baddeleyites in shergottite NWA 5298 Evolved, alkalic clasts in Black Beauty sample.
A Sample from an Ancient Sea of Impact Melt
#11 Hotspot Volcano Notes
Plate Tectonics.
Titanium Isotopes Provide Clues to Lunar Origin
Titanium Isotopes Provide Clues to Lunar Origin
Water Inside Mars Enriched Shergottites: High La/Yb
New Martian Meteorite: Northwest Africa (NWA 7034)
Timeline of Martian Volcanism
Younger Age for Oldest Martian Meteorite
What happens at plate boundaries (stays at plate boundaries).
Moon enriched in 182W/184W compared to Earth.
Time to Solidify an Ocean of Magma
Hot Spots.
Damp Moon Rising Overview: The discovery in 2008 by Alberto Saal (Brown University) and colleagues that lunar volcanic glasses contain water surprised.
Water Inside Mars Enriched Shergottites: High La/Yb

VOLCANOES AND PLATE TECTONICS
Changes to Earth.
Deep Sea Drilling.
Volatile Elements Test Models for the Origin of the Moon
Fig. 3 (A) Source mixing array for shergottite Lu-Hf and Sm-Nd source compositions calculated using equations of Nyquist et al. (A) Source mixing array.
Ch – 15 Plate Tectonics II.
Presentation transcript:

Two Billion Years of Magmatism in One Place on Mars Summary: Thomas Lapen and Minako Righter (University of Houston), and colleagues at Aarhus University (Denmark), the Universities of Washington (Seattle), Wisconsin (Madison), California (Berkeley), and Arizona (Tucson), and Purdue University (Indiana) show that a geochemically-related group of Martian meteorites formed over a much longer time span than thought previously. So-called depleted shergottites formed during the time interval 325 to 600 million years ago, but now age dating on a recently discovered Martian meteorite, Northwest Africa (NWA) 7635, extends that interval by 1800 million years to 2400 million years. NWA 7635 and almost all other depleted shergottites were ejected from Mars in the same impact event, as defined by their same cosmic-ray exposure age of ~1 million years, so all resided in one small area on Mars. This long time span of volcanic activity in the same place on the planet indicates that magma production was continuous, consistent with geophysical calculations of magma generation in plumes of hot mantle rising from the core-mantle boundary deep inside Mars. Left: Seven chemical separates from NWA 7635 fall along a line, indicating an age of 2403 ± 140 million years. The uncertainty derives from the small amount of scatter around the line. Thus, formation of the depleted shergottites began at least 2400 million years (2.4 billion years) ago and lasted at least until 325 million years ago (the age of the youngest depleted shergottite dated so far). Right: Measurements of isotopes produced by cosmic rays allow cosmochemists to determine the time of ejection from Mars. This diagram shows ejection ages of different types of shergottites. Note that 11 depleted shergottites (red diamonds) were ejected about a million years ago. The crystallization (eruption) ages of this set of lava flow samples, including NWA 7536, ranges from 325–2400 million years, indicating an extensive period of eruptions in one small region of Mars, possibly a single volcano. Reference: Lapen, T. J., Righter, M., Andreasen, R., Irving, A. J., Satkoski, A. M., Beard, B. L., Nishiizumi, K., Jull, A. J. T., and Caffee, M. W. (2017) Two Billion Years of Magmatism Recorded from a Single Mars Meteorite Ejection Site, Science Advances, v. 3, no. 2, e1600922, doi: 10.1126/sciadv.1600922. New Sm-Nd age dating on depleted shergottite NWA 7635 extends the time of magmatic activity by 1.8 billion years in a volcanic center that provided us a coherent group of Martian meteorites. NWA 7635 and ten other depleted shergottites were ejected from Mars at the same time, about a million years ago, indicating a long duration of magmatism in one place on Mars.