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MARTIAN METEOROLOGY- WEATHER FORECASTING EVA FROM AN ANALOG MARTIAN HABITAT Buckner, D. K., de Leon, P., Anamika, F., Henson, P. G. University of North Dakota, Department of Space Studies, NASA EPSCoR ABSTRACT Crew-controlled life support systems are essential for manned exploration of planetary surfaces. On Mars, dust storms are often unpredictable, can obscure satellite communications, and will threaten daily and Extravehicular Activity (EVA). (Figure 1) To combat this issue, a low-cost, user-friendly, closed-loop weather monitoring system utilizing high altitude balloons was developed and tested at the University of North Dakota’s Inflatable Lunar/Mars Analog Habitat (ILMAH). Crews fabricated sensor packages inside the habitat, filled and launched the instruments on weather balloons during EVA, then tracked and downlinked instrument data from inside the habitat. Successful execution of these EVAs suggests that balloons are a viable platform for autonomous, local weather forecasting on Mars. SYSTEM OVERVIEW GOAL: Develop a crew-controlled, balloon-based system for Martian astronauts to autonomously, locally monitor weather conditions. KEY ELEMENTS : Instrumentation Flexible sensor arrays fabricated by crew EVA tools and procedures Balloon fill tools modified to interface with suits Communication and telemetry systems Multiple closed-loop and open-network systems Data Acquisition Live downlink of radiosonde and position data, post-flight retrieval of additional data Figure 1: global dust storm 2018, Mars Reconnaissance Orbiter [NASA/JPL-Caltech/MSSS] Figure 2: ILMAH mission VI crew launching a weather balloon EVA PROCEDURES Tools: custom toolbelt, stabilization structure, modified fill tools to interface with suit gloves Procedures (1-2 hrs on EVA): 1. Capcom in habitat, manages operations 2. 2 crewmembers don suits, exit ILMAH THANKS INSTRUMENTATION Instruments fabricated, programmed, and assembled into payload package in ILMAH EVA module (Figure 3) Variety of low cost, miniature atmospheric sensors, cameras, and transmitters Live downlink (radio) Radiosonde : temperature, pressure, humidity data Live downlink (satellite) GPS : flight path data Network comms For contact between ground station and payloads Includes both closed-loop and open networks different devices Figure 4: ILMAH mission IV crewmember assembling radiosonde Figure 5: ILMAH mission VI crew working together to fill balloon Figure 7: mission V launch with live data transmission from payload Figure 6: block diagram of ground station to payload communications Engineering lab facilities Enables modular payload design Supports multiple weather conditions, crew needs, and applications 3. Fill balloon 4. Establish ground station to payload connectivity 5. Launch balloon 6. Re-enter ILMAH, doff suits 7. Downlink data from instruments package FUTURE WORK CONCLUSION : The results of these three EVA tests in the ILMAH support system viability and suggest that high altitude balloons are a feasible platform for local, autonomous weather monitoring on Mars. FUTURE WORK IN THE ILMAH: Continued system testing with future crewed missions Ergonomic analysis of tools for enhanced crew comfort Expanded payload package with additional instrumentation and telemetry capabilities Communication line development Tethered system for data collection during heavy dust conditions, allowing crew to physically retrieve sensor and data during obscured communications Figure 8: balloon with suspended dust sensor tethered to the planetary surface, enabling manual retrieval FUTURE WORK, MARS SCENARIO: Martian materials analysis ISRU creation of tools, balloon system, lifting gas, etc. Custom payload packages for direct Mars utilization Integration with various habitat designs Thanks to the University of North Dakota and the Department of Space Studies for supporting this research, NASA EPSCoR for funding the ILMAH and related EVAs, the ILMAH mission IV, V, and VI crewmembers for conducting these launches and aiding in system development Figure 3: the Inflatable Lunar/Mars Analog Habitat with EVA module DATA ACQUISITION Crew comms Managed by Capcom Radio : verbal between all 3 crewmembers Video : EVA suit cams provide feed to Capcom for live view and enhanced safety COMMUNICATION Post-flight Imagery , dust , other atmospheric sensors Requires payload retrieval following flight Future: tether unit to ensure is recovered when live downlink obscured by dust

MARTIAN METEOROLOGY- WEATHER FORECASTING EVA FROM … · On Mars, dust storms are often unpredictable, can obscure satellite communications, and will threaten daily and Extravehicular

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Page 1: MARTIAN METEOROLOGY- WEATHER FORECASTING EVA FROM … · On Mars, dust storms are often unpredictable, can obscure satellite communications, and will threaten daily and Extravehicular

MARTIAN METEOROLOGY- WEATHER FORECASTING EVA FROM AN ANALOG MARTIAN HABITAT

Buckner, D. K., de Leon, P., Anamika, F., Henson, P. G.University of North Dakota, Department of Space Studies, NASA EPSCoR

ABSTRACTCrew-controlled life support systems are essential for mannedexploration of planetary surfaces. On Mars, dust storms areoften unpredictable, can obscure satellite communications,and will threaten daily and Extravehicular Activity (EVA).(Figure 1) To combat this issue, a low-cost, user-friendly,closed-loop weather monitoring system utilizing high altitudeballoons was developed and tested at the University of NorthDakota’s Inflatable Lunar/Mars Analog Habitat (ILMAH). Crewsfabricated sensor packages inside the habitat, filled andlaunched the instruments on weather balloons during EVA,then tracked and downlinked instrument data from inside thehabitat. Successful execution of these EVAs suggests thatballoons are a viable platform for autonomous, local weatherforecasting on Mars.

SYSTEM OVERVIEWGOAL: Develop a crew-controlled,balloon-based system for Martianastronauts to autonomously, locallymonitor weather conditions.

KEY ELEMENTS:Instrumentation

• Flexible sensor arrays fabricated by crewEVA tools and procedures

• Balloon fill tools modified to interface with suitsCommunication and telemetry systems

• Multiple closed-loop and open-networksystems

Data Acquisition• Live downlink of radiosonde and position data,

post-flight retrieval of additional data

Figure 1: global dust storm 2018, Mars Reconnaissance Orbiter [NASA/JPL-Caltech/MSSS]

Figure 2: ILMAH mission VI crew launching a weather balloon

EVA PROCEDURESTools: custom toolbelt, stabilization structure, modified fill tools to interface with suit glovesProcedures (1-2 hrs on EVA):1. Capcom in habitat, manages operations2. 2 crewmembers don suits, exit ILMAH

THANKS

INSTRUMENTATION• Instruments fabricated, programmed, and

assembled into payload package in ILMAH EVA module (Figure 3)

• Variety of low cost, miniature atmospheric sensors, cameras, and transmitters

Live downlink (radio)• Radiosonde:

temperature, pressure, humidity data

Live downlink (satellite)• GPS: flight path

data

Network comms • For contact

between ground station and payloads

• Includes both closed-loop and open networks different devices

Figure 4: ILMAH mission IV crewmember assembling radiosonde

Figure 5: ILMAH mission VI crew working together to fill balloon

Figure 7: mission V launch with live data transmission from payload

Figure 6: block diagram of ground station to payload communications

• Engineering lab facilities

• Enables modular payload design

• Supports multiple weather conditions, crew needs, and applications

3. Fill balloon4. Establish ground

station to payload

connectivity 5. Launch balloon6. Re-enter ILMAH,

doff suits7. Downlink data

from instruments package

FUTURE WORKCONCLUSION: The results of these three EVA tests

in the ILMAH support system viability and suggestthat high altitude balloons are a feasible platform forlocal, autonomous weather monitoring on Mars.

FUTURE WORK IN THE ILMAH:• Continued system testing with future crewed

missions• Ergonomic analysis of tools for enhanced crew

comfort• Expanded payload package with additional

instrumentation and telemetry capabilities• Communication line development• Tethered system

for data collection during heavy dust conditions, allowing crew to physically retrieve sensor and data during obscured communications

Figure 8: balloon with suspended dust sensor tethered to the planetary surface, enabling manual retrieval

FUTURE WORK, MARS SCENARIO:

• Martian materials analysis• ISRU creation of tools, balloon system, lifting gas,

etc.• Custom payload packages for direct Mars

utilization• Integration with various habitat designs

Thanks to the University of North Dakota and theDepartment of Space Studies for supporting thisresearch, NASA EPSCoR for funding the ILMAH andrelated EVAs, the ILMAH mission IV, V, and VIcrewmembers for conducting these launches andaiding in system development

Figure 3: the Inflatable Lunar/Mars Analog Habitat with EVA module

DATA ACQUISITION

Crew comms• Managed by Capcom• Radio: verbal between all 3 crewmembers• Video: EVA suit cams provide feed to

Capcom for live view and enhanced safety

COMMUNICATION

Post-flight• Imagery, dust, other atmospheric sensors• Requires payload retrieval following flight• Future: tether unit to ensure is recovered

when live downlink obscured by dust