National Academies Press: OpenBook

Organic Matter and the Moon, by Carl Sagan (1961)

Chapter: IV. LUNAR SUBSURFACE TEMPERATURES

« Previous: III. REPORTS OF GAS CLOUDS ON THE LUNAR SURFACE
Suggested Citation:"IV. LUNAR SUBSURFACE TEMPERATURES." National Research Council. 1961. Organic Matter and the Moon, by Carl Sagan. Washington, DC: The National Academies Press. doi: 10.17226/18476.
×
Page 22
Suggested Citation:"IV. LUNAR SUBSURFACE TEMPERATURES." National Research Council. 1961. Organic Matter and the Moon, by Carl Sagan. Washington, DC: The National Academies Press. doi: 10.17226/18476.
×
Page 23

Below is the uncorrected machine-read text of this chapter, intended to provide our own search engines and external engines with highly rich, chapter-representative searchable text of each book. Because it is UNCORRECTED material, please consider the following text as a useful but insufficient proxy for the authoritative book pages.

IV. LUNAR SUBSURFACE TEMPERATURES Kozyrev attributed his gas cloud to lunar vulcanism. In an effort to provide an alternative explanation, Fremlin (1959a) made a proposal which we now discuss. It should be emphasized that Fremlin's argument in no way depends on the validity of Kozyrev's reported observations. Portions of the Moon's surface are considered to be com- posed of dust particles in close physical contact. Because of the increase of hydrostatic pressure with depth, particle contact and hence the effective thermal conductivity also increase with depth, the derived relation for simple geometry being ke = 7 x 10"7 h1/2, (13) where ke is the effective conductivity in cal cm"* sec" C°" , and h is the depth in cm. Radioactive heat, released in the lunar in- terior, will tend to be localized at the depths of greatest thermal conductivity. The increase of temperature with depth from this cause is given by AT/Ah « J/ke, (14) where J is the heat flux due to radioactive decay in cal cm"2 sec"1. With a flux of 8.4 x 10"" cal cm"2 sec"1, Fremlin derived a temp- eration of about 750°C at a depth of 10 meters. He postulated that at some depth the temperature becomes so high that phase changes occur in the dust, volatiles being released as gases; with the re- mainder of the dust at this critical level melting and cooling. After- wards the particulate nature of the level has been destroyed, and the heat localization effect is operative henceforth only above this level. Jaeger (1959) has criticized the numerical values of conducti- vity and flux adopted by Fremlin. The high value assumed by Fremlin for the heat flux would prevent the Moon from having the tensile strength required to maintain its nonequilibrium figure, and this part of Jaeger's criticism is undeniably valid. But Fremlin (1959b) has adequately answered Jaeger's criticism of the adopted value for ke; a surface composed of both dust layers of low 22

conductivity and relatively bare rock of higher conductivity is in no conflict with microwave and eclipse observations. Taking a terrestrial value for the radioactive heat flux of J = 1. 2 x 10"" cal cm"2 sec"1—a factor of seven smaller than Fremlin's value — we find from equations (13) and (14). AT = 1.7 h1/2 C°, so that at a depth of ten meters the excess temperature is 54 C°. With J = 2. 3 x 10"' cal cm"2 sec"*, a value characteristic of chondritic meteorites, AT z 0. 33 h1/2 C°, so that at a depth of ten meters the excess temperature is 10 C°. From microwave observations it is known that the temperatures less than half a meter below the surface vary between 0° and - 70°C during a lunar day and night (Piddington and Minnett, 1949). The temperature variation is damped with depth, and at about ten meters-should be no more than a few C°. We conclude that time- constant biologically-optimum temperatures exist a few tens of meters under those areas of the Moon composed of congealed dust particles. 23

Next: V. POSSIBILITY OF AN INDIGENEOUS LUNAR PARABIOLOGY »
Organic Matter and the Moon, by Carl Sagan Get This Book
×
MyNAP members save 10% online.
Login or Register to save!
Download Free PDF

The immediate future seems to hold both the promise and the responsibility of extensive contact between man-made objects and the Moon.

Current United States plans tentatively call for the soft landing on the Moon of instrumentation designed to detect indigenous organisms or organic matter, possibly in a roving vehicle, by 1964-67 in the Surveyor and Prospector Programs. The Soviet Union apparently has the capability of performing similar experiments at an earlier date. It is clear that positive results would give significant information on such problems as the early history of the Solar System, the chemical composition of matter in the remote past, the origin of life on Earth, and the distribution of life beyond the Earth. By the same token, biological contamination of the Moon would represent an unparalleled scientific disaster, eliminating possible approaches to these problems. Because of the Moon's unique situation as a large unweathered body at an intermediate distance from the Sun, scientific opportunities lost on the Moon may not be recoupable elsewhere.

This monograph is concerned with the possibility of finding indigenous lunar organisms or organic matter, and with the possibility of their contamination by deposited terrestrial organisms or organic matter.

  1. ×

    Welcome to OpenBook!

    You're looking at OpenBook, NAP.edu's online reading room since 1999. Based on feedback from you, our users, we've made some improvements that make it easier than ever to read thousands of publications on our website.

    Do you want to take a quick tour of the OpenBook's features?

    No Thanks Take a Tour »
  2. ×

    Show this book's table of contents, where you can jump to any chapter by name.

    « Back Next »
  3. ×

    ...or use these buttons to go back to the previous chapter or skip to the next one.

    « Back Next »
  4. ×

    Jump up to the previous page or down to the next one. Also, you can type in a page number and press Enter to go directly to that page in the book.

    « Back Next »
  5. ×

    To search the entire text of this book, type in your search term here and press Enter.

    « Back Next »
  6. ×

    Share a link to this book page on your preferred social network or via email.

    « Back Next »
  7. ×

    View our suggested citation for this chapter.

    « Back Next »
  8. ×

    Ready to take your reading offline? Click here to buy this book in print or download it as a free PDF, if available.

    « Back Next »
Stay Connected!