Details
Original language | English |
---|---|
Pages (from-to) | 335-339 |
Number of pages | 5 |
Journal | Advances in space research |
Volume | 22 |
Issue number | 3 |
Publication status | Published - 1998 |
Externally published | Yes |
Abstract
ASJC Scopus subject areas
- Engineering(all)
- Aerospace Engineering
- Physics and Astronomy(all)
- Astronomy and Astrophysics
- Earth and Planetary Sciences(all)
- Geophysics
- Earth and Planetary Sciences(all)
- Atmospheric Science
- Earth and Planetary Sciences(all)
- Space and Planetary Science
- Earth and Planetary Sciences(all)
- General Earth and Planetary Sciences
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In: Advances in space research, Vol. 22, No. 3, 1998, p. 335-339.
Research output: Contribution to journal › Article › Research › peer review
}
TY - JOUR
T1 - Simulation of planetary UV radiation climate on the example of the early Earth
AU - Rettberg, P.
AU - Horneck, G.
AU - Strauch, W.
AU - Facius, R.
AU - Seckmeyer, G.
N1 - Copyright: Copyright 2019 Elsevier B.V., All rights reserved.
PY - 1998
Y1 - 1998
N2 - Solar UV radiation is a dynamic driving force of organic chemical evolution. However, it may have severe constraints in biological evolution, for instance in the early history of life on Earth, before atmospheric evolution of a protective ozone layer. Today, the full spectrum of solar UV radiation is experienced only in space. In the experiment RD-UVRAD on D-2 the biological response to solar UV as a function of ozone concentrations down to very low values was investigated. Biofilms, biological UV dosimeters, were exposed to the extraterrestrial solar radiation on one of the two exposure trays mounted on the User Support Structure (USS) with free access to space. Different cut-off filters, which exclude UV of short wavelengths, and neutral density filters were used. After the flight the biofilms were developed and analyzed on ground. As a result a strong correlation between the increase in biologically effective UV radiation with decreasing (simulated) ozone concentrations was observed. Without any ozone the solar UV radiation is about three orders of magnitude more effective than today on Earth. This space experiment resulted in new insights in the environmental conditions of life on the early Earth and in the deleterious biological consequences of future stratospheric ozone depletion.
AB - Solar UV radiation is a dynamic driving force of organic chemical evolution. However, it may have severe constraints in biological evolution, for instance in the early history of life on Earth, before atmospheric evolution of a protective ozone layer. Today, the full spectrum of solar UV radiation is experienced only in space. In the experiment RD-UVRAD on D-2 the biological response to solar UV as a function of ozone concentrations down to very low values was investigated. Biofilms, biological UV dosimeters, were exposed to the extraterrestrial solar radiation on one of the two exposure trays mounted on the User Support Structure (USS) with free access to space. Different cut-off filters, which exclude UV of short wavelengths, and neutral density filters were used. After the flight the biofilms were developed and analyzed on ground. As a result a strong correlation between the increase in biologically effective UV radiation with decreasing (simulated) ozone concentrations was observed. Without any ozone the solar UV radiation is about three orders of magnitude more effective than today on Earth. This space experiment resulted in new insights in the environmental conditions of life on the early Earth and in the deleterious biological consequences of future stratospheric ozone depletion.
UR - http://www.scopus.com/inward/record.url?scp=0032405488&partnerID=8YFLogxK
U2 - 10.1016/S0273-1177
DO - 10.1016/S0273-1177
M3 - Article
VL - 22
SP - 335
EP - 339
JO - Advances in space research
JF - Advances in space research
SN - 0273-1177
IS - 3
ER -