EVA Report – March 1st

EVA Report:
EVA #8 Crew members: Alexandre Martin (EVA leader), Benoît FLOQUET, Laurent BIZIEN, Jérémy AUCLAIR

Author: Alexandre Martin

Location:
Near Pooh’s Corner: 12S-518900E-4250900N
Lith Canyon: 12S-518300E-4256500N

Time: departure at 9:00 p.m. Duration: 3h

Purposes:
• Replace the battery of the LOAC
• Explore Lith Canyon

Narrative:
We started our EVA placing Laurent’s solar panels experiment next to the GreenHab. After a small trip to Pooh’s Corner to deal with our instruments, we rode our ATV to explore Lith Canyon. We made a large 1h40 walk there, enough to visit a great part of it. We then went back to the Hab, yet we were not able to contact our Habcom. We discovered later that this was a walkie-talkie issue, maybe because of the weather (fast winds). 10 minutes later, he was finally able to hear us, and we could come back in the Hab

9:00 am: EVA#8 left airlock
9:15 am: EVA#8 left the Hab
9:16 am: EVA#8 arrived at Pooh’s corner
9:25 am: EVA#8 left Pooh’s Corner
9:45 am: EVA#8 arrived at Lith Canyon
11:25 am: EVA#8 left Lith Canyon
11:45 am: EVA#8 back at the Hab
12:00 am: EVA#8 back in the Hab

EVA Report – February 27th

EVA Report:

EVA #7 Crew members: Laurent BIZIEN (EVA leader), Benoît FLOQUET, Louis MANGIN, Gabriel PAYEN, Victoria DA-POIAN

Author: Laurent BIZIEN

Location:

Near Pooh’s Corner: 12S-518900E-4250900N

Hab surroundings

Time: departure at 2:12 p.m. Duration: 1h30 (shortened by 1h15)

Purposes:

  • Replace the battery of MegaARES
  • Train to emergency procedures

Narrative:

We started the EVA by splitting the involved members of the crew in two teams (we have learnt later by Shannon that it wasn’t something to do in EVA so I take the responsibility of such a decision error). Team red, composed of Victoria, Gabriel and Benoît took a Rover, Curiosity, and an ATV, 350.2. They went to Pooh’s Corner in order to change the battery of MegaARES and also checked the battery of LOAC instrument. At the same time, team blue, Louis and I, did the usual checks of the other Rovers (today, only Opportunity was there) and ATVs and of the water tanks. We also tried to inflate the tires of ATV 350.1. We didn’t succeed for the front left tire.

Team red quickly returned and we could start the emergency procedures. On the morning, I had made a speech to the other members of the crew about the emergency procedures some future marsonauts could encounter in EVA.

We started with a basic situation. One person simulating a health problem and another person to make a review. After a few instances, we followed up on emergency transportation. To do so, we brought Curiosity next to a person simulating a victim. The exercise’s goal was to transport the victim up to the Rover, from different ways depending of the victim’s injury. Finally, we performed realistic injury cases (bone traumatism, unconsciousness, respiratory arrest…) leading to emergency transportation and LSPs in the Rover’s trunk.

Realizing that the emergency procedures in EVA were very limited due to the lack of ability to move of the backpacks and of the helmets, we decided to return to the Hab. We carried Victoria into the main airlock and Gabriel stayed with her while Louis, Benoît and I went back to the Hab by the engineering airlock in order to simulate an emergency return.

2:12 p.m.: EVA#7 left Airlock

2:15 p.m.: Team red left the Hab

2:20 p.m.: Team red’s arrival at Pooh’s corner

2:30 p.m.: Team red’s leaving from Pooh’s corner

2:35 p.m.: Team red’s arrival at the Hab

2:40 p.m.: Beginning of the emergency procedures

3:40 p.m.: End of the emergency procedures

3:45 p.m.: EVA#7 back in the Hab

EVA Report – February 26th

Dear CapCom,

Here is the EVA Report:

26 Feb 2018

EVA #6 Crew members: Jérémy Auclair (EVA leader), Victoria Da-Poïan, Gabriel Payen, Alexandre Martin

Location:

– Near Pooh’s Corner: 12S-518900E-4252000N

– White Rock Canyon: 12S-520200E-4247500N

Time: departure at 09:09 a.m. Duration: 2 hour 13 minutes

Narrative: My first EVA as EVA leader went really well ! We changer the battery that powered the LOAC instrument (the old one was completely empty), we tested the battery powering the MegaARES instrument and confirmed it needed to be changed quickly (tomorrow). Otherwise both instruments are supporting the desert conditions perfectly. We then went to white rock canyon for exploration and photography. The walk went perfectly, the temperature was perfect, our reparations on the back packs prevented the apparition of fog on our helmets. We started to walk inside the canyon and on our way back we walk on the ridge (at a safe distance) to change the point of view. We finished the walk around 11am. Having nothing else to do we went back to the Hab to refill the ATVs and end the EVA. Everything went fine.

Purposes:

– LOAC: Maintenance – replacement of the battery

– MegaARES: Maintenance – Battery level test

– White Rock Canyon – Exploration and photography

Vehicles: 1 Rover (Curiosity), 2 ATVs (350.1, 350.2)

9:09 a.m.: EVA#6 left Airlock

9:15 a.m.: EVA left the Hab using Curiosity, ATVs 350.1 and 350.2

9:23 a.m.: Arrival on the working place

9:25 a.m.: Beginning of LOAC battery replacement and MegaARES battery test

9:35 a.m.: End of maintenance

9:40 a.m.: Beginning of the drive for White Rock Canyon

10:00 a.m.: Arrival at White Rock Canyon and beginning of walk

10:50 a.m.: End of walk and beginning of the drive back to the Hab

11:05 a.m.: Arrival at the Hab

11:15 a.m.: Entry in the Airlock

Best,

Victoria

Commander of Crew 189

EVA Report

Hello again CapCom,

Here is today’s EVA report:

EVA Report:
EVA #3 Crew members: Louis Mangin (EVA leader), Benoit Floquet, Laurent Bizien, Alexandre Martin

Author: Louis Mangin
Location: Around the Hab 12S-518100E-4250700N
Near Pooh’s Corner: 12S-518900E-4250900N
Cactus road: 12S-52200E-4252700N

Time: departure at 9:30 p.m. Duration: 2 hours

Purposes:
– Deploy the LOAC after reparation
– Check MegaARES status
– Explore around Cactus Road
– Shoot Media photos

Narrative:
We started by getting a lot of gear out of the engineering airlock: wastes, LOAC and tools. We then struggled to start the ATVs because of the coldness. When arrived on site, I had fog on my helmet because of the walk carrying the device, so that I didn’t see exactly chat happened, but while plugging the power wire, the power system overheated, and wires melted. I then disconnected the battery, but it was already too late. We evaluated then that only the power system was touched and apparently were right to guess so. Anyway, we packed everything back and went back to the hab to bring the sensor back. At the same time Benoit had checked the MegaARES and everything was fine there. After letting the broken LOAC in the engineering airlock, we headed to Cactus Road. We then climbed a hill, went to an entrance of Candor Chasma and shoot some group photos with our school’s banner. The fog intensified for the ones wearing the first version of the suits, and it was pretty cold, so that we headed back to the Hab early.

9:30 a.m.: EVA#3 left Airlock
9:40 a.m.: EVA left the Hab using two ATVs and one rover
9:45 a.m.: Arrival at place of interest
10:00 a.m.: Failure due to LOAC’s power system overheating
10:20 a.m.: Back to Hab to put back the LOAC
10:30 a.m.: Leaving the Hab to Cactus Road
10:40 a.m.: Exploration of Cactus Road surroundings
11:15 a.m.: Leaving Cactus Road
11:30 a.m.: EVA End

Louis Mangin

EVA Report – February 20th

EVA Report:

EVA #2 Crew members: Victoria Da-Poian (EVA leader), Jérémy Auclair, Gabriel Payen, Benoit Floquet

Location: – Around the Hab 12S-518100E-4250700N

Time: departure at 09:30 a.m. Duration: 2 hour 40 minutes

Narration: I was really happy to explore again the red cliffs with my new crew. Since this morning, everyone has experienced the EVAs. We managed to deploy one experiment (the MegaARES) but a small problem interrupted the LOAC deployment. We will fix it with Jérémy in order to try again tomorrow. Even if Gabriel had a very foggy helmet (fans problems), and everyone seems really happy and I have to say the photos Benoit took are really nice. During our EVA, we had a very nice teamwork. I am very proud of our common work and I am looking forward to going back to EVA with them.

EVA Report – February 19th

Hello Graeme,

Here is our first EVA’s reports. We experienced a better weather than expected so that we were able to stay longer on the outside and visit the surroundings!

EVA Report:
EVA #1 Crew members: Louis Mangin (EVA leader), Jérémy Auclair, Alexandre Martin,

Location: Around the Hab 12S-518100E-4250700N
Near Pooh’s Corner: 12S-518900E-4250900N
Under Eastern Kissing Camel Ridge: 12S-518500E-4249700N
Top of Hab Ridge: 12S-517800E-4249700N
Zubrin’s head: 12S-519500E-4248100N

Time: departure at 2:00 p.m. Duration: 1 hour 50 minutes

Purposes:
– Find a location to deploy our two atmosphere study devices – First EVA logger in situ test
– Exploration and EVA training for newcomers
– First photos and videos shots

1:58 p.m.: EVA#1 left Airlock
2:01 p.m.: EVA left the Hab using Deimos & Opportunity
2:09 p.m.: Arrival on first place of interest: Pooh’s Corner 2:40 p.m.: Leaving Pooh’s Corner
2:50 p.m.: Arrival on second place of interest
3:00 p.m.: Climbing to the top of Hab Ridge (third place of interest) 3:25 p.m.: Getting back on the rovers
3:35 p.m.: Going to Zubrin’s head to shoot photos
3:50 p.m.: Getting back in the Hab

Best,

Louis Mangin
Crew 189 Commander

EVA Report – February 9th

Crew 188 EVA #14 Summary Report 09FEB2018

Author’s name: Julia DeMarines, Crew Astronomer, Green Hab Operator

Purpose of EVA: To perform additional video filming using either the GoPRO or Insta360 PRO camera on the ridge around the Hab. While walking, we will collect rock and plant samples for in-situ chlorophyll samples for analysis.

Location of EVA: Hab Ridge
UDM27 Coordinates: 12S, 5175750E, 54250500N

Number of EVA Crew: 3

Participants: Ryan Kobrick, Sarah Jane Pell, Julia DeMarines

EVA Commander: Julia DeMarines




Road(s) and routes per MDRS map:


1) Exit Hab and head to the hills directly west to the Hab

2) Walk to the Sagan Road


3) Climb to summit Hab Ridge

4) Follow the road on Hab Ridge Road as time allows

Mode of Travel: Walking

Vehicles you will be using (if applicable): None.

Duration: 2 hours 41 minutes


EVA Departure Time: 10:26


EVA Return Time: 13:07

Summary:

We left the hab a little after the predicted time due to two last minute bathroom needs. The weather was sunny with some haze and no wind. The crew soon felt overheated, helmets/glasses were fogging up and had to stop frequently to let the sun burn off the fog. Once on the ridge, Julia selected two sites for chlorophyll detection samples, and Sarah Jane set up her Insta360º Pro camera for three different shots. Ryan recorded the journey on a GoPro camera to document the experience. Once our objectives were accomplished we turned around and walked back to the hab.

EVA Report – February 9th

EVA #15 EVA Report 09Feb2018

Author’s name: Tatsunari Tomiyama AHFP, Health & Safety Officer

Purpose of EVA: To collect micrometeorite soil samples at the Tooth Ridge and take photo and video for the mission documentary.

Location of EVA: Toothy Ridge

UDM27 Coordinates: 12 S, 516871 E, 4255884 N

Number of EVA Crew: 3

Participants: Zac Trolley, Tatsunari Tomiyama, Renee Garifi

EVA Commander: Renee Garifi

Rovers used: ATV

1, 2, 3

Duration: 1hours 29minutes

EVA Departure Time: 14:16

EVA Return Time: 15:45

Summary:

The objective of this EVA was to collect meteorite samples at the toothy ridge. We prepared and entered the airlock in timely manner. However, all crew members have issues breathing while walking. Therefore, we decided to return to avoid a critical incident. The details on our breathing issues for crew members will be reported in the operation report. Please reference the operation issue report as a detailed summary.

EVA Report – February 8th

EVA #13 EVA Summary Follow-up 08Feb2018

Start Time: 10:20

End Time: 13:40

Purpose of EVA: To reconnaissance of Candor Chasma for future EVA mission planning.

Destination: Candor Chasma

UDM27 Coordinates: 12 S 520217 E, 4251607 N

Participants: Ryan Kobrick, Zac Trolley, Sara Jane Pell

Road(s) and routes per MDRS map:

1. Take the entrance road (Driving)

2. Turn left Cow Dung Road (Driving)

3. Turn right Galileo Road (Driving)

4. Turn right Cactus Road (Driving)

5. Park on Cactus Road and walk to the Candor Chasma

6. Return by the same routes.

Mode of Travel: Rover and Pedestrian

Vehicles you will be using (if applicable): Sprit and Opportunity

Mode of travel: Walking and Driving
Vehicles used: Curiosity and Spirit

Since EVA – 13 , several analogue astronauts (of varying height, neck/head girth, lung capacity and fitness) could only maintain a maximal breathing rate for a maximum of a couple of minutes before exhaustion would cause them to reduce their breathing rate, forcing them to suspend their activity, to mitigate CO2 build-up and low visibility condensation/fog inside the helmet. We found that several crew were experiencing the effects of low-oxygen and high-CO2 build up while performing mild walking, even driving vehicles, in warm conditions with low wind.

I t is our assumption that the ambient wind plays a big role in circulating the air within the helmet, and when there is no wind, the internal fans to not have sufficient flow to perform an air exchange at the same rate as the crew members’ breathing level. The fans in the MDRS Analogue Astronaut suits produce 200 Cubic Feet per Minute – this measurement is based on an unencumbered and unrestricted output.

This afternoon we did a full survey of the suit s and their function, and found a systemic fault in the suits. Four of the six suits were running on only one fan. The fan that was on the switch side of the suit has their blades bent and would not rotate. In some cases the fans could be dislodged, and in others the blades were permanently bent. The LEDS still light up, and (half the air) air still flow s through both tubes, so this design flaw was not found until now.

EVA Report – February 7th

EVA #12
Author’s name: Dr. Sarah Jane Pell, Artist-in-Residence, Journalist

Purpose of EVA: To create a photo and video tribute to the international Winter Olympic Games in Pyeongchang, South Korea utilizing VR education and to connect our Artist in Residence’s Performing Astronautics work with our crew’s backup Commander Dr. Soyeon Yi, South Korean Astronaut.

Location of EVA: South of Marble Ritual (walking), Pooh’s corner (vehicle)
UDM27 Coordinates: 518800 E, 4250600 N

Number of EVA Crew: 4
Participants: Zac Trolley, Sarah Jane Pell, Julia De Marines, Renee Garifi
EVA Commander: Renee Garifi

Road(s) and routes per MDRS map:
1. Take East on Entrance Road (Driving)
2. Turn Left onto Cow Dung Road (Driving)
3. Park on Cow Dung Road at Marble Ritual
4. Walk to filming location in field

Mode of Travel: Rover and Pedestrian
Vehicles you will be using (if applicable): Curiosity, Spirit, and Deimos

Summary:
During the breakfast and EVA briefings, Dr. Pell prepared the crew with the design of the tasks including choreography, staging, camera set up, the sequence of required shots, and all equipment required on site. The Crew prepared themselves by taking photos with our national flags, and then Mars Flag, then playing an orchestral recording of the official Mars Anthem “Rise to Mars”. Mumbai, India-born opera singer Oscar Castellino, composed the uplifting score, with inspirational words co-written by Castellino and Mars Society President Dr. Robert Zubrin.

As the EVA #12 team arrived at the Marble Ritual site, Pell initiated a series of challenges to inform research into Performing Astronautics. The team activities included the Insta360º Pro (a.k.a. Magpie) recording from 6 camera lenses in 4K 360 Pano. The crew performed to the camera, as it represented multiple vantages for the potential audience: as if they commanded an amphitheatre or arena, on Mars, and in direct live-stream via VR to Earth.

The first task was to install a Martian “eternal flame”. After consultation with the public, José Cordeiro, Energy advisor to the Singularity University, suggested that we create a Solar Flame (of course). We achieved this by fashioning a silver survival blanket into the shape of a flaming plume and seated it aloft one of the Marble Ritual dishes. It glistened like a beacon of hope, emitting warmth and representing our symbol of eternal peace among nations, and planets.

The Crew then gathered for the Opening Ceremony tribute. First, we processed around the Insta360 Pro behind the official flag-bearer of the Martian National Flag [Zac Trolley, Engineer] and assembled in front of the Eternal Flame. Then nation-by-nation, we processed around the Magpie, to stand as the anthem played behind the Australian, Japan, Canadian, and United States flags. All of these scenes will be overlaid during post-production and editing so that in total, the four-person crew will serve simultaneously as the official 20 person delegation from many nations.

Let the games begin!

The first activity was a relay race around the arena. Each crew-member ran a leg of the race around the Magpie, and passed glowing batons between them without incident. The analogue astronauts made it through to the finals, and huddles over the Insta360 Pro to review their time trials discuss tactics and mentally prepare for the finals. Their preparation paid off. There was great jubilation as Renee Garifi crossed through the yellow ribbon finish line!

After earning an excellent score for her dark and expressive ribbon routine, United States’ Renee Garifi became the individual rhythmic gymnastics Mars Olympic champion with the perfect score of 10:10. Another memorable performance, Zac Trolley of Canada delivered a mesmerizing routine incorporating more dance elements than artistic floor exercise, only to botch the final ribbon toss, and fall to the ground gasping for air. He was quickly attended by officials and given oxygen on site. Later his coaches explained that he is fully recovered and was keen to defend his reigning title.

Given the altered gravity and range of climatic conditions on Mars, the Official Interplanetary Olympic Committee decided to include a long jump in both Mars Winter and Summer athletics. The men’s long jump has been included in Earth’s Olympic athletics since the first Summer Olympics in 1896. The women’s long jump was introduced over fifty years later in 1948 and was the second Olympic jumping event for women after the high jump, which was added in 1928.

On Mars, there is no gender divide. With a pressure-packed jump, Dr. Sarah Jane Pell representing Australia was the first to make the leap across the red regolith, and she made it straight to the finals. She ended up with the Silver medal on her penultimate jump with a mark of18.37 meters.

At the end of a great day at the Marble Ritual arena, all medal winners stood on the podium to a jubilant crowd, their hearts on their chests as the national anthem played in the afternoon sun.

While Astrophysicist Neil deGrasse Tyson tweeted up a storm in 2012 by asking his followers, "How about a Mars Olympics?, we celebrate the human spirit with our speculative fiction for a future Mars Olympiad, with the dual purpose of exploring the range of movement and performance expression with the MDRS life support suits in this analogue terrain.

By today’s technological and biological standards, all athletes would be suffocated by the Martian atmosphere and frozen by the extreme temperatures, however, the MDRS EVA-12 helped us fashion a sense of play and performance experimentation based on coming together to work collectively in the spirit of exploration. It also provided a springboard for connecting audiences with the VR outreach opportunity to explore how they might fare with 38% of gravity.

Perhaps we would finally crack the code to human flight. Until then, Crew 188 send our very best wishes to all the nations of planet Earth coming together in peaceful competition for Earth’s 2018 international Winter Olympic Games in Pyeongchang, South Korea.

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