
Name
... Many bacteria are also able to exchange genetic information by a process called conjugation. During conjugation, a hollow bridge forms between two bacterial cells, and genes move from one cell to the other. This transfer of genetic information increases genetic diversity in populations of bacteria. ...
... Many bacteria are also able to exchange genetic information by a process called conjugation. During conjugation, a hollow bridge forms between two bacterial cells, and genes move from one cell to the other. This transfer of genetic information increases genetic diversity in populations of bacteria. ...
Class notes
... This hypothesis was tested through the Doppler shift in stellar spectrum, which implied that matter was flying apart in all directions throughout the universe ...
... This hypothesis was tested through the Doppler shift in stellar spectrum, which implied that matter was flying apart in all directions throughout the universe ...
session iii - Problems of Practical Cosmology
... near-Earth asteroids. Primordial quark nuggets have been predicted to contain most of the baryonic number of the Universe. It has been suggested by J.E.Horvath to search for these nuggets in the asteroidal-mass range. Since the strange quark matter is expected to have a plasma frequency as high as 2 ...
... near-Earth asteroids. Primordial quark nuggets have been predicted to contain most of the baryonic number of the Universe. It has been suggested by J.E.Horvath to search for these nuggets in the asteroidal-mass range. Since the strange quark matter is expected to have a plasma frequency as high as 2 ...
Sun-Solar System Connection Roadmap: 2005-2035
... Sun-Solar System Connection Objectives Agency Strategic Objective: Explore the Sun-Earth system to understand the Sun and its effects on the Earth, the solar system, and the space environmental conditions that will be experienced by human explorers, and demonstrate technologies that can improve futu ...
... Sun-Solar System Connection Objectives Agency Strategic Objective: Explore the Sun-Earth system to understand the Sun and its effects on the Earth, the solar system, and the space environmental conditions that will be experienced by human explorers, and demonstrate technologies that can improve futu ...
1 Introduction
... underway at four ionosonde stations in Japan to monitor ionospheric disturbances that may cause GPS signal-based positioning errors and radio wave propagation failure. In terms of global activities, NICT has set up geomagnetic observation stations at 10 locations and HF radar at one location—mainly ...
... underway at four ionosonde stations in Japan to monitor ionospheric disturbances that may cause GPS signal-based positioning errors and radio wave propagation failure. In terms of global activities, NICT has set up geomagnetic observation stations at 10 locations and HF radar at one location—mainly ...
No Slide Title
... Study the environment and the solar wind interaction as well as the evolution and dynamics of solar system objects with focus on the inner planets, moons, asteroids, comets, and dust. Development of scientific instrumentation for satellite-based measurements in support of space exploration. ...
... Study the environment and the solar wind interaction as well as the evolution and dynamics of solar system objects with focus on the inner planets, moons, asteroids, comets, and dust. Development of scientific instrumentation for satellite-based measurements in support of space exploration. ...
ANAEROBIC NITROGEN FIXERS ON MARS. B. G. Lewis, Dept. of
... the process is biological nitrogen fixation, the transformation of N2 to NH3. The phenomenon is crucial for feeding the billions of our species on Earth. On Mars, the same process may allow us to discover how life can adapt to a hostile environment, and render it habitable. Hostile environments also ...
... the process is biological nitrogen fixation, the transformation of N2 to NH3. The phenomenon is crucial for feeding the billions of our species on Earth. On Mars, the same process may allow us to discover how life can adapt to a hostile environment, and render it habitable. Hostile environments also ...
Exploring Space!
... (NASA) is established to oversee the exploration of space 1969 First man, Neil Armstrong walks on the moon 1977 The Voyager 1 and Voyager 2 are launched to Jupiter, Saturn and beyond, they are now 10 billion km away and still sending back pictures to earth 1981 The first space shuttle, Columbia, was ...
... (NASA) is established to oversee the exploration of space 1969 First man, Neil Armstrong walks on the moon 1977 The Voyager 1 and Voyager 2 are launched to Jupiter, Saturn and beyond, they are now 10 billion km away and still sending back pictures to earth 1981 The first space shuttle, Columbia, was ...
Astronomy Study Guide
... 1. The force that tends to pull together matter in stars is ________ 2. The theory that explains the formation of the universe is the ____ ______ B. Our Galaxy 1. A light year is the __________________ light travels in a year. 2. Our galaxy is named the ___________ ________ 3. The Milky Way is what ...
... 1. The force that tends to pull together matter in stars is ________ 2. The theory that explains the formation of the universe is the ____ ______ B. Our Galaxy 1. A light year is the __________________ light travels in a year. 2. Our galaxy is named the ___________ ________ 3. The Milky Way is what ...
The Origin of Life on Earth
... membranelike structure, self-replication occurred, and DNA became established as the genetic material. A “chicken-or-the-egg” paradox emerges if DNA was the first genetic material. DNA codes for proteins, yet proteins are required for DNA replication, transcription, and translation. Thomas R. Cech a ...
... membranelike structure, self-replication occurred, and DNA became established as the genetic material. A “chicken-or-the-egg” paradox emerges if DNA was the first genetic material. DNA codes for proteins, yet proteins are required for DNA replication, transcription, and translation. Thomas R. Cech a ...
EXPOSE

EXPOSE is a multi-user facility mounted outside the International Space Station dedicated to astrobiology. EXPOSE was developed by the European Space Agency (ESA) for long-term spaceflights and was designed to allow exposure of chemical and biological samples to outer space while recording data during exposure.The results will contribute to our understanding of photobiological processes in simulated radiation climates of planets (e.g. early Earth, early and present Mars, and the role of the ozone layer in protecting the biosphere from harmful UV-B radiation), as well as studies of the probabilities and limitations for life to be distributed beyond its planet of origin. EXPOSE data support long-term in situ studies of microbes in artificial meteorites, as well as of microbial communities from special ecological niches. Some EXPOSE experiments investigated to what extent particular terrestrial organisms are able to cope with extraterrestrial environmental conditions. Others tested how organic molecules react when subjected for a prolonged period of time to unfiltered solar light.