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The Importance of my Job:

 
Remember, a successful sample retrieval is necessary for getting the samples back to Earth where scientists can study them for signs of past water and possibly life!


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Background

 
 
Follow these directions to learn more about the rover that you will be working with today. 

BACKGROUND

In this mission, you will be collaborating with the Navigation (NAV) and Energy (NRG) teams to collect samples with the Sample Fetch Rover (SFR). You are responsible for analyzing the terrain to make sure it is safe for the rover to travel on. The image below shows the different parts of the rover, and describes the use of each part.

Sample Fetch Rover displaying it's NAVCam, Robotic Arm, Solar Panels, and Sample Tube Storage. The NavCam is used to locate the sample tubes at each depot, and to analyze the terrain on each path. The robotic arm is used to retrieve the samples at each depot. The storage rack is used to hold the collected samples so that the rover can return them to the MAV. The solar panels provide the energy needed to move the rover and collect samples.



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Research

 
 
Follow these directions for researching the different types of terrain on Mars:

TERRAIN

There are four main types of terrain that the rover could encounter in Jezero crater: Smooth regolith, Sand ripples, Cratered terrain, and Rocky terrain. Continue reading to get a definition of each terrain type. Below each definition, you will see photos showing what this terrain type looks like on Mars and on Earth.


Smooth regolith is the easiest terrain for the rover to travel on. “Regolith” refers to a layer of loose sand and rocky material on top of hard, flat rock. This terrain looks like smooth, flat ground. It might have a few small rocks, or look a bit sandy, but there are no sand dunes.

Two images side by side. The left showing smooth Regolith on Mars' surface and the right showing smooth regolith on Earth's surface.


Terrain with sand ripples looks similar to sand dunes on Earth. In places where the dust on the surface of Mars is very thick, it has been shaped into waves or ripples. We call this terrain type sand ripples.

two images side by side the left showing sand ripples on Mars' surface and the right showing sand ripples on Earth's surface.


Cratered terrain is smooth or slightly sandy terrain with one or more distinct craters. The craters will look like shallow circular holes in the surface, with a slightly raised rim. The terrain around the crater might look smooth, sandy, or rocky. But, if there is at least one crater in the area, then the terrain is cratered.

Two images side by side the left showing Cratered terrain on Mars' surface and the right showing Cratered Terrain on Earth's surface.


The final terrain type, rocky terrain, is characterized by the many rocks that are present. These rocks stick up from the surface, and are usually a slightly different color than the surrounding dusty surface. This terrain type requires the most energy for the rover to travel on.

Two images side by side the left showing Rocky Terrain on Mars' surface and the right showing Rocky Terrain on Earth's surface.

GEO RESEARCH QUESTIONS

NAV will be selecting a path based on the map shown below. Make sure to check the chat for a message from NAV.
Map of all four Paths the Rover could take. Path A, 2 km, 7 Samples. Path B, 3 km, 6 Samples. Path C, 2.5 km, 7 Samples. Path D, 5.5 km, 17 Samples.
stop+vector.jpg

STOP HERE UNTIL YOU GET A MESSAGE FROM NAV WITH A PATH SELECTION.

 

Terrain Analysis

 
Follow the instructions below to determine the terrain of NAV’s chosen path. 




geo terrain data log

Notepad



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Elevation

 
 

ELEVATION

The elevation of a location identifies the height of the location. On Earth, elevation is usually given in comparison to sea level. For example, as “10 meters below sea level.” This elevation may also be written as “-10 meters,” or “negative 10 meters.” Since Mars has no ocean, the elevations on Mars are given in relation to the “zero elevation,” which is a specific elevation that was chosen by scientists.

Because the samples that you are retrieving today are located inside Jezero crater on Mars, most of the elevations you look at today will be negative, or “below the zero elevation.”

Slope is a word that scientists use to describe how steep something is. The slope of a path tells you how quickly the elevation rises or falls as you travel along the path. Slope is determined by looking at how much the elevation changes and how long the path is.
Follow the instructions below to determine how steep the selected path is:



geo elevation data log

Notepad




For example, if the path length is 4 kilometers and the elevation change is 130 meters, then the slope is “moderate.”
Chart of Path Length in km and the Elevation Change in meters to determine Slope. The slopes determine by Path length and elevation change can be determined as flat, slight, moderate, steep or very steep.

Chart of Path Length in km and the Elevation Change in meters to determine Slope. The slopes determine by Path length and elevation change can be determined as flat, slight, moderate, steep or very steep.

Send the terrain and slope information to the NRG team:







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Upon Reaching The Depot

 
 
It has been noted on previous Mars missions, such as Curiosity, that the Martian surface can be hard on rover wheels. Now that the rover has reached the depot, we need to check the condition of the wheel rims before beginning the return journey to the Mars Ascent Vehicle (MAV). Here is an image taken of the wheels after reaching the depot:
 
Test
 
To rate the condition of these wheels, please consult the examples in the Wheel Condition Research Log below:

geo wheel condition research

1. If the wear on the wheels is low, please let NRG know that no action is required:






This is GEO. I have a message for the NRG team. I have examined the condition of the wear on the wheels. Based on my evaluation, there is only low wear on the wheels. No action is required.



2. If the wear on the wheels is moderate, please let NRG know that the rover should drive backwards and at half speed for its return trip to the MAV:






This is GEO. I have a message for the NRG team. I have examined the condition of the wear on the wheels. Based on my evaluation, there is moderate wear on the wheels. My recommendation is that we drive backwards and at half speed to return to the MAV.



3. If the wear on the wheels is extreme, please let all teams know that the rover may be unable to complete the journey back:






This is GEO. I have a message for ALL teams. I have examined the condition of the wear on the wheels. Based on my evaluation, there is extreme wear on the wheels. The rover may not be able to complete the journey back to the MAV. We should consult the FLIGHT DIRECTOR for guidance on how to proceed with the mission.



Watch this video of Perseverance exploring the Jezero Crater Delta.



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Make a Final Decision

 
 
You must now work with all of the other teams to determine how many samples can be gathered at the depot, and if you will be able to launch the samples before the dust storms arrives.



Sample Image of where to find the pen tool, text tool, and more on the Mission Decision Board. The pen tool, post-it note and text box buttons are all to the left of the Mission Decision Board. The pen tool is first, the post-it note is fourth and the text box is seventh.

Sample Image of where to find the pen tool, text tool, and more on the Mission Decision Board. The pen tool, post-it note and text box buttons are all to the left of the Mission Decision Board. The pen tool is first, the post-it note is fourth and the text box is seventh.



a. How many samples should be picked up before returning to the MAV?
b. IF there is a dust storm approaching, is there enough time for the rover to return to the MAV before the dust storm arrives?

While you wait, did you know:
And, click here to explore the rock samples collected by the actual Perseverance Rover!
In 2020 the crater Jezero was chosen for Perseverance landing and exploration. Scientists have reason to believe that this crater once held water. Landing at Jezero had a lot of risks since the basin is surrounded by steep cliffs. The slightest error during landing could have seen an end to Perseverance. In spite of this, the team decided that the potential of water rich samples was worth it!

In 2020 the crater Jezero was chosen for Perseverance landing and exploration. Scientists have reason to believe that this crater once held water. Landing at Jezero had a lot of risks since the basin is surrounded by steep cliffs. The slightest error during landing could have seen an end to Perseverance. In spite of this, the team decided that the potential of water rich samples was worth it!

 
Once all team members agree on a Final Decision, you will have successfully completed the Mars Sample Fetch Rover mission simulation.

Congratulations, GEO, and here’s hoping for a successful mission ahead!
 

Select Next Path

 
 
NOTE: Only move onto this section if all team members have agreed on a Final Decision and there is remaining time for your mission simulation.

Once the rover successfully returns the samples collected on the path chosen by NAV, it is time to plan for a second Sample Fetch Rover mission. If you were to send the rover to a second depot, which path would you select? Follow the directions below to select which path the rover should visit next.

Diversity of samples that may be discovered within the mission. 20 samples inside the Jezero system and 17 outside the Jezero system.

Diversity of samples that may be discovered within the mission. 20 samples inside the Jezero system and 17 outside the Jezero system.

ALL SAMPLES


The next image shows you which samples are cached at each depot.
Diversity of samples broken down into four groups. Path A, 7 samples.  Path B, 6 samples. Path C, 7 samples. Path D, 17 samples.

Diversity of samples broken down into four groups. Path A, 7 samples. Path B, 6 samples. Path C, 7 samples. Path D, 17 samples.

SAMPLES BY PATH


geo sample diversity data log