Model Overview & Print Notes

Summary

"How Many Oceans & How Many Atmospheres has Mars lost to Rust celebrating the 2021 February 18 Arrival at Mars of Perseverance Rover"

A "Mars Introduction/Lesson/Discussion" including various size & scale terrain models of the Perseverance landing region, class discussion topic ideas, and fun web links with remarkable insights & detail relevant to Mars (presented further below the models info).

NASA "Where is Perseverance Rover" Map

Choose 3D globe projection or VR (Google carboard supported :-) at NASA Mars Trek link to Jezero Crater Perseverance landing ellipse.

This is also an example of a high detail terrain model making process (more details in the "Print" section below). This work expands upon the easier 'point, click, drag' "Generate 3D Print file" tool which is built into the NASA Mars, Moon, Mercury, Vesta & Ceres Treks. Students may enjoy using the Trek tool to make their own mid-detail 3D printable models of their favorite craters, etc. I describe that built-in web tool in more detail in a separate Moon Trek 'thingi' https://www.thingiverse.com/thing:4732510.

I have included a variety of model sizes & scales from relatively small & easier to print up to a large quad that is more difficult to print.

'smallest' model: ~1cm = 1km (1:100k) .STL model with 5x height exaggeration of the Jezero Crater Perseverance Rover Landing Ellipse region.

'larger' model (included in a .ZIP file): ~1cm = 200m (1:20k) .STL model with 5x height exaggeration to show the detail of the dunes in features like Belva crater

'larger' area model (included in a .ZIP file): ~1cm = 2.5km (1:250k) .STL model with 10x height exaggeration showing western Jezero Crater area. Made from a preliminary DEM that still shows stitching in areas.

Quad of adjacent models (included in a .ZIP file) for the landed rover's planned science & exploration region: ~1cm = 200m (1:20k) .STL model with 5x height exaggeration

  • JEZ_hirise_SE.stl (rover's actual landing area)
  • JEZ_hirise_SW.stl (Belva crater & potential rover path area)
  • JEZ_hirise_SE.stl.stl (eroded alluvial fan)
  • JEZ_hirise_NW.stl (Neretva Vallis entrance) (I had several challenges printing this one.)

Why Send a unique Rover to a very special place on Mars? A few example gains from such an endeavor:

  • Attempt a significant engineering unknown: Fly an extremely special helicopter (images & description) in air so thin, on another planet, after the 'shake, rattle & roll' of launch, plus about 8 months of space travel !
  • Help us understand important long-term planet dynamics affecting our ability to grow food & live in cities near flooding shorelines as climate changes on our own planet Earth.
  • Look for signs of life on Mars from the distant past to further appreciate & understand life on Earth.
  • Inspire students & governments by innovating new tools & techniques that actually perform well in new & difficult environments & demonstrating the power of skilled people harnessing their differences, in a collaborative yet challenging process of working together.

What engineering unknown makes the Mars Helicopter special? Exploring a few similarities & differences between current Mars & Earth will help reveal the difficult & remarkable challenge of flying a Mars Helicopter...

Mars & Earth today are quite different, but both have day times & night times & a Mars 'day' which is called a sol, is only about 40 minutes longer than the current 24 hour Earth 'day' (Earth had much shorter days in the past & will have much longer days in the future as the Moon continues to move farther away...).

Mars today has a dry surface. No rain puddles to trap the Mars Helicopter....but, sand dust in the air, & sand pits & sand dunes (Perseverance's 1st Mars panorama) & cold nights freezing the electronics & batteries will be a challenge. Where on the Mars terrain model(s) do you see or would expect sand dunes? Where on Earth could you find a dry dune surface similar to places on Mars?

Mars in the distant past may have been more similar to Earth today & more parts of Earth could continue to become more like Mars (description). Mars is a bit further from the Sun than Earth, but both Earth & Mars are at 'friendly' distances from the Sun...not too close & not too far. However, Mars has a very different size than Earth & that changes many important things.

Compare the model with the NASA 'artists' drawing of the probable ancient lake in Jezero crater...

  • Match the river in the NASA drawing to similar looking features on the model(s). What features might have been under water in the past? Where might there have been ancient shore lines?

  • What signs of that ancient water can you see in this model? For example, large alluvial fan (maybe students have seen such a pattern in a nearby creek, pond, or rain puddle), Neretva Vallis water cut through the crater's rim,...

  • Which meteor craters likely formed from impacts that occurred after this Mars lake became dry...for example, craters that show well defined rims with minimal erosion?

  • Identify on your model(s) the regions shown in different colors in the USGS coloring activity or USGS geologic map. What differences in texture, flat/steepness/slope, height/elevation, & number of meteor craters do you observe on the models between the different colored regions shown in the geologic map?

The USGS colors represent different types of rock formations...some formed by erupting volcanoes, some by sands blown by the wind, and others made by 'dirt' sediments carried by flowing water.

However, Mars's actual surface color is generally 'rusty'. This color might be because Mars may have lost about one Earth ocean's amount of water (specifically the hydrogen(H) part of water high in the upper atmosphere) to space...possibly leaving the oxygen part of water behind to leave both the Mars ancient ocean & atmosphere to become rock 'rust' on the surface rocks. Rocks with iron will rust with oxygen to make the 'rusty' colored dusts that help make Mars appear to have a reddish/orangish/pinkish colors from a distance..

Now the remaining 'water' is in a few, sometimes very pretty, clouds as shown in these images, but appears to be mostly in salt brines (pdf) or frozen as ices in polar caps & under the dust 'soil':

With the 'smaller' model = 1:100,000 = 1cm:1km:

Use a string and small ruler to measure & record an estimate of the diameter of Belva crater

locate the center of the landing target ellipse on the model, then measure & record an estimate of its diameter

Why is the target landing area such a 'big' ellipse? Compare the approximate diameter of the ellipse that you just measured and compare it to the 470 million kilometers Perseverance has traveled to get to that landing site...that is even farther than the distance light travels from the Sun to Earth. "By time of landing, Perseverance will have covered 292.5 million miles (470.8 million kilometers), and Mars will be about 130 million miles (209 million kilometers) away from Earth; at that point, a transmission will take about 11.5 minutes to reach the spacecraft." Remarkable since the flight was a direct shot from Earth with no stops along the way.

If you also printed one of the 1:20k models such as the 'larger' model or the "quad", find its area & features in the 'smaller' 1:100k model or 'larger area' 1:250k model & compare the difference in detail. Also, compare details within 1cm = 200m (1:20K) model itself such as the locations & orientations of the sand dunes in various features.

  • Choose a 'favorite feature of interest' on the model & discuss why.

    For example, my 3rd grade child suggested the peaks near the center of the landing ellipse as 'ancient islands in the crater when it was a lake' & we discussed the impact of a change in water depth over time.

  • There is also the option to follow the rover: mark its path on the model(s) over the next few years & put colored dots at places of key discoveries (and possibly print a matching handout with details of the discovery index keyed with the same color dot) as the science team explores.

Print Settings

Printer Brand:

Creality

Printer:

Ender 5

Rafts:

Doesn't Matter

Supports:

No

Resolution:

0.12

Filament: eSun PLA+ Silver

Notes:

General method:

NASA Mars, Moon, Mercury, Vesta & Ceres Treks have a built in 'point, click, drag' "Generate 3D Print file" tool that works well for medium sized parts of a planet ( I show that simple tool in a different 'thingi' post at https://www.thingiverse.com/thing:4732510 ).

For detailed areas, downloading a detail DEM from the NASA Trek & then using QGIS with the DEMto3D plugin see "Create STL from DEM files with the QGIS DEMto3D extension" produces much higher detail models.

DEM data downloaded from the NASA Mars Trek. Make your own models of this area easily as well using data from:

NASA Mars Trek link to Jezero Crater Perseverance landing ellipse.

The specific DEM I downloaded from the NASA Mars Trek (see the relevant screenshot):

  • the 1:20k models are made from: JEZ_hirise_soc_006_DTM_MOLAtopography_DeltaGeoid_1m_Eqc_latTs0_lon0_blend40.tif

  • large area model made from the preliminary:
    NES_JEZ_MID_DEM_Mosaic_HiRISE_CTX_HRSC_GCS_MARS_07-10-2018.tif
Slicer: Cura 4.8
  • 'vase mode' = “spiralize outer contour” in Cura
  • Scale 100%
  • Raft optional
  • 0.12 layer height (works well with 0.8 nozzle in Vase mode with PLA+)
  • Y at 30 (gives a gentle curve of the bowden tube with the Ender 5)
What I used to print this:
  • Orientation: use whichever axis your printer prints with best
  • Nozzle: 0.8mm steel nozzle
  • Printer: ‘stock’ Creality Ender 5 pro with the v1.1.5 mainboard using a custom compile of Marlin 1.1.9.1 to include manual bed corner leveling & manual bed mesh leveling.
  • Filament: eSun PLA+ 'silver color' (steel nozzle print T 220C)
'vase mode' = 'spiralize outer contour' printing advantages:
  • short print time
  • fast movement mostly in one axis = excellent print quality
  • no infill (reduces ghosting and other printing artifacts)
  • constant extrusion (= no retraction artifacts, etc)
  • improved visual: print layer is perpendicular to the vertical of the model
  • minimizes filament requirement
  • 0.8 (or 0.6) nozzle gives a sturdy single wall rectangle shell print within a few hours.
Find your favorite craters & land forms & make & share your own with the NASA Trek web “Generate 3D print file” tool or for detail areas download a DEM & make one with QGIS and the DEMto3D plugin...

https://trek.nasa.gov/mars/

Enjoy!

Make a Clipped Extent in QGIS & process with the DEMto3D plugin

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Custom Section

NASA JPL EDL Video: https://youtu.be/4czjS9h4Fpg

https://mars.nasa.gov/mars2020/multimedia/videos/?v=461

Mars Sound Recordings

Great rocks & Helicopter:

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Ingenuity Flight Log

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Jezero 360 Panorama Links:

Panorama: "Spanning the Delta of Mars' Jezero Crater" December 15, 2021

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Explore with Perseverance: 3D terrain

Mars Jezero Crater Weather

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USGS Jezero Geology PDF

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USGS Astrogeology Jezero Geology Formations (Student Activity)

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https://www.usgs.gov/center-news/coloring-activity-explore-jezero-crater-mars-2020-perseverance-rover

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Mars Perseverance Rover Landing Site Jezero Crater: Mars Lesson built with the "NASA Mars Trek" & QGIS

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STL
JezeroCraterQGIS_PerseveranceLandingElipse1to100K.stl
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ZIP
JezeroCloseUp02h1t20k.zip
Geometry Asset
ZIP
HIRISECTX_MarsGCS_JezeroWestArea02e1to250k_model.zip
Geometry Asset

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