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HI-SEAS habitat (Mauna Loa)

Moon

Unreviewed draft

This page was built from a teammate-supplied list. The text is teammate-written, unreviewed. Sources pending.

Summary

not provided

Location

Country
USA (Hawaii)
Coordinates
19.60, -155.49
Elevation (m)
2500
Year first used as an analog
2013

Terrain and geology

not provided

Climate

not provided

Parameters matched

not provided

Why it is an analog

Longest NASA-funded Mars isolation missions, on barren basalt.

Key differences: where the analogy breaks down

Thick air; tropical high-altitude climate; Earth gravity.

Experiments done

HI-SEAS missions (2013-2018: 4, 8 and 12-month Mars missions) studying crew cohesion, food, sleep and 20-min communication delays; later lunar and Mars campaigns.

Experiments proposed

Habitat ops; suited EVA on basalt; ISRU demonstrations; dust airlock trials; communication-delay operations.

How to adjust it

Regolith (cinder) berms around the dome; dust-control airlock tests; Mars-sol scheduling.

Access

not provided

Hazards

not provided

Sources

Sources pending (no sources in CSV).

v1 score, percentile and overlap flag

A descriptive lookup of scores v1 already stored. It is not a test, and a high percentile here does not show that this is a good analog.

v1 used this site
Unknown. The nearest v1 site, "mauna kea", is about 24.3 km away, and the files cannot say whether v1 meant the same place.

Stored v1 scores near HI-SEAS habitat (Mauna Loa)
Score viewResultPercentileScoreDistance to tile (km)Overlap flag
Connecting Ridge C1, BaseScored96.536.315.6Not in a flagged tile
Connecting Ridge C1, Landing and mobilityScored99.239.215.1In a flagged tile
Connecting Ridge C1, Power and nightScored96.526.315.6Not in a flagged tile
Shackleton rim, BaseScored92.840.119.8Not in a flagged tile
Shackleton rim, Landing and mobilityScored98.642.715.1Not in a flagged tile
Shackleton rim, Power and nightScored92.829.119.8Not in a flagged tile

Overlap flag: whether the tile used for the score is one v1 flagged as stable in its top group across the Monte Carlo runs.

What these scores can and cannot tell you
  • This is a lookup of scores v1 already stored. It is descriptive and is not a test of the method.
  • A site is matched to the best-scoring tile that passed the gates within the match radius. A different radius would give different numbers.
  • Tiles are large compared with most sites, so a score describes the surrounding area, not the site itself.
  • Scores exist only for tiles that passed the land-cover and data gates. A gated-out or unscored site has no score, which says nothing about how good an analog it is.
  • Percentile is the share of scored tiles in that view with a lower score.
  • The Moon score is effectively terrain only. Mars is a low-confidence secondary result.
  • v1 failed its negative controls, so a high percentile here does not show that a site is a good analog.
  • The ranking is not checked against independent data. Gravity, air, dust and radiation are not scored.
  • Sites are compared with views of their own body only.
  • Match radius: 20 km, the radius v1 used.

Mars

Unreviewed draft

This page was built from a teammate-supplied list. The text is teammate-written, unreviewed. Sources pending.

Summary

not provided

Location

Country
USA (Hawaii)
Coordinates
19.60, -155.49
Elevation (m)
2500
Year first used as an analog
2013

Terrain and geology

not provided

Climate

not provided

Parameters matched

not provided

Why it is an analog

Longest NASA-funded Mars isolation missions, on barren basalt.

Key differences: where the analogy breaks down

Thick air; tropical high-altitude climate; Earth gravity.

Experiments done

HI-SEAS missions (2013-2018: 4, 8 and 12-month Mars missions) studying crew cohesion, food, sleep and 20-min communication delays; later lunar and Mars campaigns.

Experiments proposed

Habitat ops; suited EVA on basalt; ISRU demonstrations; dust airlock trials; communication-delay operations.

How to adjust it

Regolith (cinder) berms around the dome; dust-control airlock tests; Mars-sol scheduling.

Access

not provided

Hazards

not provided

Sources

Sources pending (no sources in CSV).

v1 score, percentile and overlap flag

A descriptive lookup of scores v1 already stored. It is not a test, and a high percentile here does not show that this is a good analog.

v1 used this site
Unknown. The nearest v1 site, "mauna kea", is about 24.3 km away, and the files cannot say whether v1 meant the same place.

Stored v1 scores near HI-SEAS habitat (Mauna Loa)
Score viewResultPercentileScoreDistance to tile (km)Overlap flag
Jezero, BaseScored78.950.316.8Not in a flagged tile
Jezero, Ice resourcesScored78.950.316.8Not in a flagged tile
Jezero, Landing and mobilityScored70.853.016.8Not in a flagged tile
Jezero, Power and nightScored85.950.216.8Not in a flagged tile

Overlap flag: whether the tile used for the score is one v1 flagged as stable in its top group across the Monte Carlo runs.

What these scores can and cannot tell you
  • This is a lookup of scores v1 already stored. It is descriptive and is not a test of the method.
  • A site is matched to the best-scoring tile that passed the gates within the match radius. A different radius would give different numbers.
  • Tiles are large compared with most sites, so a score describes the surrounding area, not the site itself.
  • Scores exist only for tiles that passed the land-cover and data gates. A gated-out or unscored site has no score, which says nothing about how good an analog it is.
  • Percentile is the share of scored tiles in that view with a lower score.
  • The Moon score is effectively terrain only. Mars is a low-confidence secondary result.
  • v1 failed its negative controls, so a high percentile here does not show that a site is a good analog.
  • The ranking is not checked against independent data. Gravity, air, dust and radiation are not scored.
  • Sites are compared with views of their own body only.
  • Match radius: 20 km, the radius v1 used.