EVA Report – December 26th

Crew 236 EVA Report 26-DEC-2021

EVA # 7

Author: Kasey Hilton

Purpose of EVA: Collection of samples from region D and Mancos Shales from Copernicus Hwy for analysis of water content and analog for rocks found in Gale Crater

Start time: 12:00

End time: 16:00

Narrative: EVA # 7 was cancelled due to extremely high winds

Destination: Region D and the Morrison and Mancos Shell boundary on Copernicus (2 stops)

Coordinates (use UTM NAD27 CONUS): N4254000, W515575

Participants: Kasey (CMD), Cesare (XO), Dylan (ASTRO), Pavi (ENG)

Road(s) and routes per MDRS Map: Cow Dung Rd north to Brahe Hwy, Brahe Hwy west to Copernicus Hwy, south on Copernicus Hwy

Mode of travel: Driving to the west side of Region D and walking down Copernicus Hwy

Crew 236 – EVA Report – 24-Dec-2021

[Commander's EVA Report – December 24th]

Crew 236 EVA Report 24-DEC-2021

EVA # 5

Author: Kasey Hilton

Purpose of EVA: Evaluation of soil and ground conditions for additional potential habitat locations

Start time: 13:00

End time: 16:00

Narrative: EVA was canceled this afternoon due to winds and rain in the morning, making the ground very muddy. Will try this EVA again on 25DEC2021.

Destination: End of Galileo Rd/Area F

Coordinates (use UTM NAD27 CONUS): N4251500, E519750

Participants: Kasey (CMD), Vladimir (GHO), Dylan (ASTRO)

Road(s) and routes per MDRS Map: Cow Dung Rd north to Galileo Rd, then heading down into area F around Compass Rock

Mode of travel: Driving and walking

EVA Report Dec 23rd

Crew 236 EVA Report 23DEC2021

EVA #4

Author: Cesare Guariniello

Start time: 9.31 AM

End time: 12.02 PM

Narrative: The team began EVA preparation around 9 and entered the airlock at 9.31, just at the beginning of the EVA window. Crew Journalist replaced his earpiece that caused issues on EVA #3. After depressurization, the crew boarded the vehicles and headed south along Cow Dung road. After a drive of about 5 km, the crew walked towards Barainca Butte. Along the way, XO had a couple of stops to collect rock samples. One rock is brown and black and heavily vesiculated (possibly scoria). Other rocks came down from upper layers of hard mudstone and conglomerates. Meanwhile, SCI took rock temperature measurements for a project on thermal inertia of minerals at MDRS. ENG and JOU assisted and documented the work. The EVA crew reached the south side of Barainca Butte and continued its research proceeding counterclockwise around the butte. After having walked about one quarter of the perimeter of the butte, JOU noted some increasing fogging of the helmet and asked to position the fan switch at maximum speed. The fogging decreased, but JOU reported the fans slowing down. The crew decided to reduce the EVA time and began walking towards the vehicles. Unfortunately, within just a few minutes, JOU experienced a total loss of the fans which, on Mars, would require an urgent contingency rescue or would result in loss of the crewmember. Since the fogging disappeared quickly and JOU reported receiving enough air from underneath the collar, he elected to keep his helmet on for the drive back to the Hab. During the drive back, the crew met some astronauts onboard terrestrial-looking vehicles. The crew stopped the vehicles on the side of Cow Dung road, south of Kissing Camel range, to let the unknown astronauts pass by, with a brief and very amicable exchange of nods and smiles. The crew returned to the Hab about one hour earlier than the expected time, without further incidents.

Destination: Around Barainca Butte

Coordinates (use UTM NAD27 CONUS): N4247200, W519000

Participants: Cesare (XO), Tyler (SCI), Ben (JOU), Pavi (ENG)

Road(s) and routes as per MDRS Map: from the Hab south on Cow Dung Road, west towards Barainca Butte (region J)

Mode of travel: Driving and walking

Vehicles used: Curiosity and Opportunity

Cesare Guariniello

XO/HSO

Crew 236

EVA Report – December 22nd

Crew 236 EVA Report 22-Dec-2021

EVA #3

Author: Cesare Guariniello, XO/HSO Crew 236

Start time: 9.41 AM
End time: 10.28 PM

Narrative: The team first entered the airlock at 9.41. During depressurization, one crew member experienced a problem with the microphone, and after 3 minutes of repressurization the crew came back into the Hab to fix the problem. After the second depressurization, the EVA crew boarded the vehicles and headed south.

About 10 minutes into the drive, loud static was heard in the communication channel. The EVA crew stopped at the side of the road to troubleshoot the problem. XO assessed the radios and found that one radio was stuck in transmission mode (TX), thus preventing one EVA crew member from receiving communication. Switching a radio showed that the issue was in the earpiece, possibly the cable (since the earpiece does not have a vox setting).

As per EVA rules, for reasons of safety, the EVA was aborted due to one crew member has lost communication. The EVA crew returned to the Hab immediately, with no further anomalies.

Destination: Around Baranca Butte (INTENDED)

Coordinates (use UTM NAD27 CONUS): N4247200, W519000

Participants: Cesare (XO), Tyler (SCI), Ben (JOU), Pavi (ENG)

Road(s) and routes as per MDRS Map: from the Hab south on Cow Dung Road, west towards Baranca Butte (region J)

Mode of travel: Driving and walking

Vehicles used: Curiosity and Opportunity

Crew 260 EVA#1/2 Report for November 2nd

Crew 260 EVA Report 02-11-2021

EVA # 1

Author: Commander Jen Carver-Hunter

Purpose of EVA: Geologic sample collection

Start time: 10:30

End time: 12:30

Narrative: The EVA team departed the Hab 10:40, taking Cow Dung Road in medium-range speed, to see how Oppy would perform after the overheating during the training day. After crossing Robert’s Rock Garden, we incremented the speed and reach the 1101 intersection (Note for future EVAs and crews to take the southern entrance to not disrupt the natural wash). We reached our desired location where we collected our first geological targets as part of our mission objectives. After finding the needed samples, we went back to the main road and on our way North we stopped just before the Kissing Camels to go West and collect our petrified wood samples. We explored all the way to the beginning of the wash and noticing what time was it, we proceeded to return to the Hab after a successful EVA.

Destination: Road to Barranca Butte and Southwest Kissing Camel Ridge

Coordinates (use UTM NAD27 CONUS): 519700, 4247300 and 518200, 4249300

Participants: Atila, Katie, Adela

Road(s) and routes per MDRS Map: Hab road to Cow Dung Road to 1101 and back

Mode of travel: Rovers on roads, on foot off road

EVA # 2

Author: Commander Jen Carver-Hunter

Purpose of EVA: Geologic sample collection

Start time: 2:00

End time: 3:30

Narrative: The EVA team departed the Hab at 14:00. We followed Cow Dung Road to the 1101 intersection, and followed 1101 a few hundred yards to our first destination. We collected samples as part of our science mission objectives. Then we returned to the main road and turned to the north. The Opportunity Rover overheated just south of Kissing Camel Ridge, and we safely moved her to the side of the road. We piled into the remaining 2 rovers and continued on to Kissing Camel Ridge, where we collected samples at the base of the wash. Due to the onset of headaches and thirst, the EVA team returned to the Hab earlier than expected at 1530.

Destination: Road to Barranca Butte and Southwest Kissing Camel Ridge

Coordinates (use UTM NAD27 CONUS): 519700, 4247300 and 518200, 4249300

Participants: Jen, Tracy, David, Brandon

Road(s) and routes per MDRS Map: Hab road to Cow Dung Road to 1101 and back

Mode of travel: Rovers on roads, on foot off road

Crew 228 EVA#6 Report October 6th

Crew 228 EVA Report 06-Oct-2021

EVA #6

Author: Inga Popovaite and David Laude

Purpose of EVA: Exploration of Candor Chasma

Start time: 13.00

End time: 16.00

Narrative:

Dave and Inga drove to one of the entrances to Candor Chasma and explored the beginning of the canyon. The area is beautiful and breathtaking; the canyon is worth spending more time in. There was ample evidence for water flow along dry stream beds with rounded pebbles along the bed. Sedimentary layers were abundant. Also seen is what appeared to be limestone. They took a lot of photos and a few videos for outreach purposes. Inga interviewed Dave about his love for canyons. They took four radios; two of them either died due to low battery or started malfunctioning. Wind picked up on the second half of the EVA during the drive back and it was hard to communicate with VOX setting on. The wind noise caused radios to activate transmit via the VOX function. This helped to drain the batteries. A couple of lessons for the future: backup radios are a must; when it is windy it might be better to have the radio transmit manually operated.

Destination: Candor Chasma.

Coordinates (use UTM NAD27 CONUS): 38.4155 N, -110.768 W

EVA Participants: Dave Laude, Inga Popovaite

Road(s) and routes per MDRS Map: We traveled on Cow Dung Road 0110 and then along Galileo Rd 1104/Cactus Rd 1104.

Mode of travel: Driving, walking

Vehicles you will be using (If applicable): Curiosity and Spirit

EVA Report – October 05th

EVA #5

Author: Lindsay Rutter

Purpose of EVA: Collecting endolith and non-endolith rock samples on the Jotunheim structure

Start time: 0817

End time: 1032

Narrative:

Dave and Lindsay departed the HAB using the Opportunity and Curiosity rovers. The weather was cloudy, with a chance of rain. They turned left onto Cow Dung Road and proceeded North, until they arrived without incident at the intersection with Galileo Road. They parked approximately 50m North of the intersection, established contact with HabCom, and indicated they would likely experience radio blackout while circumnavigating the Jotunheim feature, and would return to an area with reception by 1000. They then dismounted the rovers, and traversed the remaining 500m to the structure by foot.

During the walk, they encountered numerous features that were visually similar to the target destination, but they did not experience difficulty finding it because Lindsay had already reached the structure using the same route in a previous EVA. Upon arrival, they conclusively identified the target destination with the aid of GPS. They then began to circumnavigate the structure counterclockwise. At five separate points along the structure, Lindsay collected samples, primarily on the structure’s slopes. Lindsay selected triplicate samples of endolith rocks and triplicate samples of non-endolith rocks. She donned extra large lab gloves over her spacesuit gloves and collected the rocks into sterilized bags for follow-up analysis. Dave recorded GPS coordinates, elevation, and collection time for each sample using the GPS Essentials application. He also manually recorded the metadata in a field notebook.

Dave and Lindsay departed the Jotunheim feature at 0958. Along the return walk, they attempted to reestablish connection every 30 seconds with HabCom, and successfully reestablished contact about halfway on the return walk to their rovers. Upon arriving at the rovers, Lindsay’s radio displayed a low battery warning and began failing to properly transmit and receive, despite it being fully charged at the beginning of the EVA. She rectified the issue by reconnecting her headpiece with her backup radio.

Dave and Lindsay began to depart Southward on Cow Dung Road, heading back to the HAB. About halfway of the return distance, they noted an off-white, elevated, and dome-shaped feature about 10m from the Westside berm of the road, that could be investigated in a future EVA. They returned to the HAB without incident. Less than one minute after entering the airlock, they were informed light precipitation had begun.

Destination: Jotunheim Structure

Coordinates: zone 12 4251912 N 518799 E (38.41712 N, -110.78466 W [NAD27])

Participants: L. Rutter, D. Laude

Road(s) and routes per MDRS map: Cow Dung Road 0110

Mode of travel: Opportunity and Curiosity rovers, walking

Crew 228 EVA #5 Report October 4th

EVA #5

Author: Jin Sia, Inga Popovaite

Purpose of EVA:

1.0) Scout and record candidate points of entry to the river delta
south of Robert’s Rock Garden for future EVAs to use (approx. 1.5 h.)
These points will only be explored near the bottom of the escarpment
so that their locations and the regolith structural properties can be
recorded; there will be no attempts to scale the full height of the
escarpment.

2.0) Validate viewshed calculation of MDRS GIS map in southern section
of Cow Dung Road for radio communications, especially in the vicinity
of Robert’s Rock Garden.
2.1) Investigate predicted reception corridor south of Robert’s Rock Garden.
2.2) If time remaining, conduct a similar investigation for the
northern section of Cow Dung Road, up to the intersection with Galileo
Road.

3.0) Film video footage for outreach.

4.0) Inga’s data collection for her dissertation on EVA crew
interaction between themselves and with HabComm.

Start time: 0900

End time: 1230

Narrative:

For the first part of the EVA, Inga and Jin drove to Robert’s Rock
Garden in Spirit and parked on the south side of the formation.

Inga then led the team to the entry of what is now known as Path 1, a
potential entry point to the delta that was previously found by Dave
and Inga on EVA #4. They tested the path and found that it was safely
scalable if done so slowly and with care. They found a summit to the
path, although they did not complete the ascent of the escarpment as
that was outside of the EVA plan. They discovered an alternate path
(which, similarly to Path 1, appears to have been carved by water
flow) that did not have the staircase-like structure of Path 1. This
has been named Path 2. The pair found that it was possible to descend
through Path 2 with slowness and care, especially by stepping over or
detouring around bramble-filled pits. However, it was found to require
detouring through relatively steep inclines.

Both conclude that it is possible to safely ascend the escarpment in
EVA suits, given optimal environmental conditions (good lighting, cool
air temperature), generous time constraints, good physical condition,
proper technique, and experienced hikers. It is a challenging hike
that should not be attempted in non-optimal conditions. Inga and Jin
also recommend using Path 1 over Path 2, as the main detour required
for Path 2 is difficult to negotiate. The GPS locations for the summit
to Path 1 and the entrance to Path 2 have been recorded for
revisiting.

After checking in with HabComm, Jin and Inga proceeded south to
investigate further alternate delta entry points. Visual surveys of
the area did not reveal any paths that were obviously easier than
Paths 1 or 2.

At that location, Inga interviewed Jin in the field about the work the
team was doing and the motivation for it. In addition to documenting
fieldwork, Inga aimed to figure out how to take video interviews
wearing EVA suits. She took additional radio with her and used a voice
recorder to record sound from it while she and Jin were communicating
via headsets. This audio will be overlayed with the video footage.

Following the interview, the team returned to the region immediately
south of Robert’s Rock Garden to check radio reception at multiple
points within it. Jin conducted a total of 14 comms checks with
HabComm every 50-100 m, then graded each check on a 4-level scale
based on the quality of the response. He found that the viewshed
calculation in ArcGIS was very conservative in this area, and that
communications were possible in a much larger region than predicted.
ArcGIS calculated that the reception corridor would fan out at an
angle of 13 degrees. However, the true extent of the fan where
communications are possible exceeds 90 degrees if one is reasonably
far away from the Kissing Camel Ridges. Perhaps this is caused by
reflection, refraction, and/or diffraction of radio waves on the
terrain. In the mean time, Inga shot several short videos for media
outreach purposes.

After characterizing the reception corridor south of Robert’s Rock
Garden, Inga and Jin drove north on Cow Dung Road, during which Jin
collected reception quality data approximately once per minute. He
collected 11 datapoints south of the Hab.

On passing the Hab, approximately 45 minutes were remaining in the
EVA, so the team decided to press on to characterize radio
communications in the northern section of Cow Dung Road. Jin collected
18 datapoints. Then, the team returned to the Hab on time.

Jin discovered that while there were no pockets of complete radio
blackout between the Kissing Camel Ridges and Galileo Road, there were
noticeable decreases in transmission quality in areas where the
viewshed calculation predicted there would be blackouts. The
transition to complete radio blackout north of Galileo road was found
to begin approximately where the viewshed calculation predicted it
would. The thickness of the boundary between reception and blackout is
between 300 and 600 m. Due to the subjective nature of evaluating
reception quality and the low resolution of the data, Jin could not
obtain high precision in his analysis.

Ironically, the team encountered problems not with radio reception,
but with their radio units in the field. Both Inga and Jin brought two
radios each for redundancy, but both of Inga’s radios failed in the
field, and Jin’s primary radio failed. Jin noticed that near failure,
the radio battery indicator drops substantially while transmitting.
Dave and Jin suspect that this due to the age of the batteries,
causing them to hold less charge and to have higher equivalent series
resistances. As a result, when the radio draws current while
transmitting, the battery’s internal voltage drop increases as
predicted by Ohm’s Law, causing the battery indicator to drop. Dave is
in the process of systematically testing the radio batteries while
transmitting.

Crew 228 has made a number of findings in this EVA. Firstly, it
successfully tested hiking trails that permit access to the dried-up
river delta, although these trails are challenging to negotiate and
should only be attempted by experienced EVA personnel. Secondly, it
found that viewshed calculation can be a helpful guide in finding
radio blackout regions, but its precision is low; it is on the order
of hundreds of metres.

Destinations:

1) Robert’s Rock Garden
2) Escarpment ~700 m southwest of Robert’s Rock Garden entering river delta
3) Search region south of Robert’s Rock Garden
4) Cow Dung Road at Galileo Road intersection

Destination coordinates:

DESTINATION TARGET COORDINATES (DD WGS84) TARGET COORDINATES (UTM NAD27)
— —

1 38.3932857°N -110.7903910°W
zone 12 4249269 N 518369 E
2 38.3880215°N -110.7955099°W
zone 12 4248684 N 517923 E
3 In same region as 2
4 38.4175715°N -110.7814639°W
zone 12 4251966 N 519142 E

Participants: Inga Popovaite, Jin Sia

Road(s) and routes per MDRS Map: Cow Dung Road 0110

Mode of travel: Rover and foot

Crew 228 EVA#4 Report -October 2nd

Crew 228 EVA Report 02-Oct-2021

EVA # 4

Author: Inga Popovaite

Purpose of EVA: Exploratory EVA to underexplored region SW from Robert’s Rock Garden

Start time: 9.06

End time: 12.49

Narrative: Dave and Inga decided to start EVA 30 min earlier because of the sunny and warm (76F) day ahead. Exited the airlock and took Perseverance and Curiosity for a drive south to Robert’s Rock Garden. They planned to walk to a river-delta looking region that was, as per crew knowledge, underexplored. On the map it looked like a moderate hike of ~ 600 meters towards a dried river delta on the other side of a small ridge. The digital map on ArcGIS indicated passageways to the delta, thus the EVA crew were hopeful that they can get to the point of interest with the assistance of a gps unit and a less-detailed map.

The EVA crew lost radio connection with the Hab right around Robert’s Rock Garden and found themselves all alone in the eery red desert. They followed the plan and walked west along the Kissing Camels Ridge until they were forced to stop. Dried river beds that showed up in the map as passable routes were narrower than expected and not passable with EVA suits. The EVA crew tried to ascend the ridge but it became too steep and unsafe to continue. In the end the EVA crew were unable to reach their final destination. However, they took photos and recorded GPS coordinates of potential pathways for future crews to explore.

The EVA crew was more successful on the way back. They ventured to Dave’s supply ship and successfully retrieved a box of granola.

Another successful part of the journey was testing out improvised sun visors. They draped shirts over helmets and suits to block out the sun on the walk back. It was possible to block the sun out and still keep one’s field of vision.

Jin acted as primary HabComm during the EVA and was concerned about his lack of knowledge about the EVA team’s status during the blackout. Based on the events that transpired, he devised several operational and communications protocol recommendations to improve future EVAs. He interviewed the EVA team after their return about their observations near the river delta escarpment and determined the reason the planned path was so much more challenging than expected. The path up the escarpment consisted of a staircase-like structure with each ‘step’ being on the order of 1-2 metres tall. While the average slope was gentle, the staircase structure itself was dangerous to negotiate in EVA suits. Due to the small size of the steps, the digital elevation model did not have a sufficiently small pixel size to resolve them, making the path look deceptively flat. After investigating several alternate paths up the escarpment, we have concluded that it is probably unreasonably risky to scale it in EVA suits without specialized climbing equipment.

Destination: Parked at Robert’s Rock Garden, aimed for dried river delta in the SW of it, did not make it past the ridge

Coordinates (use UTM NAD27 CONUS):

ROBERT’S ROCK GARDEN 38.39331 N -110.78966; W 4249269 N 518369 E

DELTA ENTRY 38.39281 N -110.79600 W 4249212 N 517815 E (did not reach this point)

Participants: Inga Popovaite, Dave Laude

Road(s) and routes per MDRS Map:

Cow Dung Road; parking at Robert’s Rock Garden and walking west following the Kissing Camel Ridge West.

Mode of travel: Driving, walking

Inga Popovaitė,

Crew 228 EVA#1 Report – September 30th

Crew 228 EVA Report 30-09-2021
EVA # 1

Author: Lindsay Rutter

Purpose of EVA: We performed an initial checkout of EVA suits while walking around the campus, tested walking up the hill in front of HAB, then tested driving the Opportunity rover during this easy and nearby EVA, all while testing radio communications and HABCOM procedures. We also tested the collection of regolith for the DNA sequencing study.

Start time: 0930

End time: 1130

Narrative: EVA was successful. We timed a full walk-around of the campus as five minutes. We tested walking up the hill in front of the HAB. We decided to drive only one Rover (Opportunity) because Inga was unable to see the driving apparatus due to the lower edge of her space helmet becoming an obstacle. So, both EVA crew drove in Opportunity, with Lindsay serving as the driver. Radio communications were successful and we reached our destination of Marble Ritual, where we collected samples. After adjustments, Inga was able to view the driving apparatus, and she drove Opportunity back to the HAB.

Destination: Marble Ritual (~600M drive + ~100M walk) after a walk-about around the tunnel connected structures for some outside EVA suit testing before driving.

Coordinates (use UTM NAD27 CONUS): 38.407 N 110.783 W

Participants: L. Rutter & I. Popovaite

Road(s) and routes per MDRS Map: Cow Dung Rd 0110

Mode of travel: Rovers

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