PPT-Changes to Earth’s Surface
Author : leah | Published Date : 2023-10-04
Layers of the Earth Constructive vs Destructive Forces Destructive Forces break down features on the Earths surface Constructive Forces build up features on the
Presentation Embed Code
Download Presentation
Download Presentation The PPT/PDF document "Changes to Earth’s Surface" is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.
Changes to Earth’s Surface: Transcript
Layers of the Earth Constructive vs Destructive Forces Destructive Forces break down features on the Earths surface Constructive Forces build up features on the surface of the Earth . superweak. angular ground motions. JINR: J. Budagov, M. Lyablin., G. Shirkov.. CERN: J-Ch. Gayde, D. Mergelkuhl. Main principle : use reflected laser beam from horizontal surface liquid . θ. ψ. Laser. Earth is a Planet. 1. Inside Earth. In molten Earth . chemical differentiation. . . Fe. , . Ni . rich core, . Si . crust and mantle. Density . 5500 kg/m. 3. Pressure, density, temperature increase with depth. Lecture 8: October 30, 2014. A Job Offer. (. Apply only if . you scored > 60% on midterm 1.). You Are Invited!. Astro. 1 Observing Session (Optional, Just for Fun). WHEN: November 13. th. at 7-9pm . Earth is a Planet. 1. Inside Earth. In molten Earth . chemical differentiation. . . Fe. , . Ni . rich core, . Si . crust and mantle. Density . 5500 kg/m. 3. Pressure, density, temperature increase with depth. The National Weather Service counts on two sources for information:. Radar. Weather Balloon. Data collected from the atmosphere. Data collected from the Earth’s surface . In order to forecast the weather, meteorologists make measurements of:. How does the Earth Change?. Geology. In your Science journal record the UEQ. How does the Earth Change?. Activating Strategy:. Your lab group will have the opportunity to use your observation skills and inferring skills to predict the contents of three film canisters.. Mapping, spectroscopy and geologic analysis of Earth’s “sister” planet. Venus. The Basics, pre-1960. Radius 95% of Earth, mass 82%. 92X Earth atmospheric pressure, 97% CO2. 462°C surface temp. The orbits of Venus and Mercury show that these planets never appear far from the Sun.. Orbital and Physical Properties. The . terrestrial planets have similar densities and roughly similar sizes. , but their rotation periods, surface temperatures, and atmospheric pressures vary widely.. Learning Target:. What is necessary for life to be present in our solar system?. Science Starter:. Pg. 2 Life on Earth Workbook…Answer question 1. Supplies: Life on Earth Workbook. 1. Heartbeat. 2. Return Papers. Tectonic plates are huge rock pieces within the earth’s crust. The plates are usually marked by fractures or fault lines formed when the plates tear apart or slide or collide past each other. This results in a change of the earth’s interior masses which send out powerful shock waves with enough force to alter the surface of the earth. The shock waves can thrust up cliffs and open huge cracks on the ground leading to an earthquake event. Created by Winds. Coriolis Effect- The shifting of ocean currents and surface winds from their expected paths caused by the rotation of the earth. Gulf Steam – ocean current in the northern Atlantic ocean, brings warm water from Africa to the Americas. Jase. Love, Gilbert Espinoza, Oscar . Pedroza. Planet Profile. Mass: 4,867,320,000,000,000 billion kg (0.815 x Earth). Equatorial Diameter: 12,104 km. Polar Diameter: 12,104 km. Equatorial Circumference: 38,025 km. WATER RESOURCE DEVELOPEMENT. Prepared By: (Group-3). Vadlani Ronak. Patel Shivanshu. Patel Parth. Thaker Rajvi. Leuva . Nisarg. Patel Rudra. ALPHA COLLEGE OF ENGINEERING & TECHNOLOGY, KHATRAJ. Gap-Filling Activities. CL#12-3066. SKG breakdown. Atmospheric SKGs. 2. Large uncertainties in atmospheric models directly increase mission risk, reduce payload margins by increasing entry system mass, limit landing sites, and may force non-optimal technology choices.
Download Document
Here is the link to download the presentation.
"Changes to Earth’s Surface"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.
Related Documents