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Kilauea caldera and Ka'u Desert

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
19.41, -155.28
Elevation (m)
1100
Year first used as an analog
1969

Terrain and geology

not provided

Climate

not provided

Parameters matched

not provided

Why it is an analog

Apollo's most-used fresh-basalt training ground.

Key differences: where the analogy breaks down

Wet tropical climate on windward side; active volcanism hazards; no cold traps.

Experiments done

Apollo crews trained on fresh basalt, collapse pits and fissures; NASA BASALT project (2016-17) on Ka'u flows for EVA science operations.

Experiments proposed

Fresh-basalt sampling ops; pit-crater descent (lunar pits); thermal IR of cooling flows; EVA-timeline rehearsal with science backroom.

How to adjust it

Restrict to Ka'u desert; floodlit night EVAs; simulant cover on test lanes.

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 49.7 km away, and the files cannot say whether v1 meant the same place.

Stored v1 scores near Kilauea caldera and Ka'u Desert
Score viewResultPercentileScoreDistance to tile (km)Overlap flag
Connecting Ridge C1, BaseScored90.616.517.8Not in a flagged tile
Connecting Ridge C1, Landing and mobilityScored96.118.817.8Not in a flagged tile
Connecting Ridge C1, Power and nightScored90.611.917.8Not in a flagged tile
Shackleton rim, BaseScored78.929.117.8Not in a flagged tile
Shackleton rim, Landing and mobilityScored86.533.317.8Not in a flagged tile
Shackleton rim, Power and nightScored78.921.217.8Not 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.