The Moon and Life on Earth

2001 ◽  
pp. 279-290 ◽  
Author(s):  
Elfed Morgan
Keyword(s):  
The Moon ◽  
Leonardo ◽  
2021 ◽  
Vol 54 (1) ◽  
pp. 149-156
Author(s):  
Linda T. Elkins-Tanton

Starting in 2006, the author joined and then led field expeditions to central Siberia in search of answers to the greatest murder mystery in the history of Earth: the end-Permian extinction. The rocks that yielded answers were the same kinds of volcanic lavas that can be seen at night on the Moon, or in photos of Mars or Venus. The unyielding Russian engineering that owns the longevity record on the surface of Venus is now used to launch cosmonauts and astronauts from the other end of those same Siberian steppes. Not the data—not the years nor the numbers nor the temperature—but art, as Solzhenitsyn explained, is the only way to reach the heart and soften our pace as we move into another age of space exploration, this time as humans, the author hopes, and not as nations.


2021 ◽  
Author(s):  
Dora Klindžić ◽  
Daphne Stam ◽  
Frans Snik ◽  
Christoph Keller ◽  
Vidhya Pallichadath ◽  
...  
Keyword(s):  
The Moon ◽  

Author(s):  
Susan M. Gaines ◽  
Geoffrey Eglinton ◽  
Jürgen Rullkötter

“But did anyone really expect to find anything?” I ask Geoff, as he shows me the canister that had contained his sample of moon dust from the 1969 Apollo 11 mission. “Well, no,” he replied, “we didn’t think there’d ever been life on the moon. But we didn’t know. We thought there might be organic compounds.” And why not? People had been finding organic compounds in meteorites for more than a century, and no one was quite sure where they’d come from or how they’d formed. In 1834, the Swedish chemist Jöns Jakob Berzelius noted the high carbon content of a meteorite that had fallen in southern France a couple of decades earlier. Meteor showers in Europe were described as early as 1492, and their extraterrestrial provenance had been documented in 1803, when the distinguished French physicist Jean-Baptiste Biot featured among the scores of citizens who witnessed the stones falling from the sky above the village of l’Alsace. But the source of the carbon compounds Berzelius and others found in meteorites would remain controversial far into the next century. Another carbonaceous meteorite fell in Hungary in 1857, and the eminent chemist Frederick Wöhler—Berzelius’s student, and the first to show that one could create carbon compounds like those made by organisms from inorganic substances in the lab—found organic compounds that he was convinced were of extraterrestrial biological origin. A decade later, Marcellin Berthelot found what he called “petroleum-like hydrocarbons” in a meteorite that had fallen near Orgueil, France, in 1864. He postulated that the hydrocarbons had formed abiotically from reaction of metal carbides with water, but in the next few years there was a spate of meteorite treatises in which the fossils of an astounding assortment of exotic extraterrestrial creatures were described in minute detail. Louis Pasteur had just presented his famous experiment showing that a protected, sterile medium remained devoid of life ad infinitum and debunked the popular theory that life could burst spontaneously into being from nonliving matter, but now the debate shifted to the possibility that life on Earth had originated with live cells or spores delivered by meteorites from space.


IUBMB Life ◽  
2000 ◽  
Vol 49 (5) ◽  
pp. 411-420 ◽  
Author(s):  
Leopold Flohé, Jan R. Andreesen, Re
Keyword(s):  
The Moon ◽  

Author(s):  
D. Klindžić ◽  
D. M. Stam ◽  
F. Snik ◽  
C. U. Keller ◽  
H. J. Hoeijmakers ◽  
...  

LOUPE, the Lunar Observatory for Unresolved Polarimetry of the Earth, is a small, robust spectro-polarimeter for observing the Earth as an exoplanet. Detecting Earth-like planets in stellar habitable zones is one of the key challenges of modern exoplanetary science. Characterizing such planets and searching for traces of life requires the direct detection of their signals. LOUPE provides unique spectral flux and polarization data of sunlight reflected by Earth, the only planet known to harbour life. These data will be used to test numerical codes to predict signals of Earth-like exoplanets, to test algorithms that retrieve planet properties, and to fine-tune the design and observational strategies of future space observatories. From the Moon, LOUPE will continuously see the entire Earth, enabling it to monitor the signal changes due to the planet’s daily rotation, weather patterns and seasons, across all phase angles. Here, we present both the science case and the technology behind LOUPE’s instrumental and mission design. This article is part of a discussion meeting issue ‘Astronomy from the Moon: the next decades’.


1966 ◽  
Vol 25 ◽  
pp. 373
Author(s):  
Y. Kozai

The motion of an artificial satellite around the Moon is much more complicated than that around the Earth, since the shape of the Moon is a triaxial ellipsoid and the effect of the Earth on the motion is very important even for a very close satellite.The differential equations of motion of the satellite are written in canonical form of three degrees of freedom with time depending Hamiltonian. By eliminating short-periodic terms depending on the mean longitude of the satellite and by assuming that the Earth is moving on the lunar equator, however, the equations are reduced to those of two degrees of freedom with an energy integral.Since the mean motion of the Earth around the Moon is more rapid than the secular motion of the argument of pericentre of the satellite by a factor of one order, the terms depending on the longitude of the Earth can be eliminated, and the degree of freedom is reduced to one.Then the motion can be discussed by drawing equi-energy curves in two-dimensional space. According to these figures satellites with high inclination have large possibilities of falling down to the lunar surface even if the initial eccentricities are very small.The principal properties of the motion are not changed even if plausible values ofJ3andJ4of the Moon are included.This paper has been published in Publ. astr. Soc.Japan15, 301, 1963.


1962 ◽  
Vol 14 ◽  
pp. 441-444 ◽  
Author(s):  
J. E. Geake ◽  
H. Lipson ◽  
M. D. Lumb

Work has recently begun in the Physics Department of the Manchester College of Science and Technology on an attempt to simulate lunar luminescence in the laboratory. This programme is running parallel with that of our colleagues in the Manchester University Astronomy Department, who are making observations of the luminescent spectrum of the Moon itself. Our instruments are as yet only partly completed, but we will describe briefly what they are to consist of, in the hope that we may benefit from the comments of others in the same field, and arrange to co-ordinate our work with theirs.


1962 ◽  
Vol 14 ◽  
pp. 415-418
Author(s):  
K. P. Stanyukovich ◽  
V. A. Bronshten

The phenomena accompanying the impact of large meteorites on the surface of the Moon or of the Earth can be examined on the basis of the theory of explosive phenomena if we assume that, instead of an exploding meteorite moving inside the rock, we have an explosive charge (equivalent in energy), situated at a certain distance under the surface.


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