MSIP Banner
Home
What is MSIP?
Activity Formats
Getting Started
Application
Curriculum
Resources
FAQs
Team Results
Teacher Events
Online Forum

Team Results

MSIP team led by Charles Lindgren

Teacher Name: Charles Lindgren
School Name: Gates Intermediate
Grade Level: 6 - 8
City: Scituate
State: MA
Country: USA

Science Question:
Channels exist on both Earth and Mars. They are usually formed by moving liquid water or lava. All channels contain two walls and a floor. The walls and floors of channels contain many interesting features. For our project we wanted to see if it was possible to determine the size and relative age of slump features in a Martian channel. Is it possible to determine the relative ages and surface areas of slump features on Mars?
Main Results:
Surface Area:
The three features we examined were almost the same size. Just by looking at them you could make a rough estimate that they would be. We don’t really know what conclusions can be drawn from that other than roughly the same conditions existed that caused the three events. Whether the same size “marsquake” occurred, or the same sized object impacted to generate the same force, or whatever reason, almost the same amount of material was released each time.

Relative Age:
The crater count has the relative age from youngest to oldest being middle, top, bottom of the image.


Extra Comments:
Area Name: Tiu Valles
Latitude (N): 15
Longitude (E): 327
image4
THEMIS context image
image2
Students' THEMIS image
Contact Us
MSIP - Home NASA ASU's Mars Education Program is a major partner of NASA's Mars Exploration Program Arizona State University