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Conclusions
© Charles Chandler
 
The following table compares the performance of various hypotheses concerned rille formation, on the Moon and on Mars.1
 
SYMBOLS:
A. Predictable
B. Permissible
C. Unexpected
O. Irrelevant
X. Impossible
 
 
  erosion
via water
erosion
gas cloud
formed by
gas blow
formed by
lava tube
electric
eruption
impact
crack
wider at high end C C O B A B
channel sinuous A C O C A B
upper end crater B B O B A A
ends at diff. elev. A A O A A B
no out wash dep. C-X C-X B C-X A A
no chan. bridges A A O B-C A A
chan. cratering O O A O A A
trav. high ground X X B X B B
stray fr. surf. dip C-X C-X B C-X B B
on ridge crest X X A B A B
strata exposure B B A C-X A-B A
strata upturned X X A X A A
rille clustering C C B-C B-C A-B A
rille crossing C-X C-X A-O C-X B B
2nd rille in bottom B C C C B B
distinct rille/crater X     X C A
 

References

1. Juergens, R. E. (1974): Of the Moon and Mars, Part I: The Origins Of The Lunar Sinuous Rilles. PENSEE


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