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Overview and status of the Kepler Mission - Harvard
Overview and status of the Kepler Mission - Harvard

... Presently we know of more than one-hundred planets1 orbiting other stars with orbital periods from about one day to a few years. All of these planets are known or presumed to be gas-giants with minimum masses typically greater than that of Saturn, except for a few Earth-mass planets that are known t ...
Lyman-α: The Many Applications and Challenges of This Powerful
Lyman-α: The Many Applications and Challenges of This Powerful

... Hot exoplanets with Lyman-α tails Reconstructed stellar Lyman-α emission lines are also the background light sources for studying exoplanet atmospheres during transits. The discovery of significantly more Lyman-α line absorption during the transit of the exoplanet HD 209458b compared to STIS observa ...
The Astrobiology Primer - Mary Ann Liebert, Inc. publishers
The Astrobiology Primer - Mary Ann Liebert, Inc. publishers

... the stars throughout the course of their lifetimes and at their deaths. Practically, all elements heavier than helium—and thus all components of the organic molecules necessary for life to form—are produced by stars. (For a specific definition of “organic,” which is not equivalent to “biological,” s ...
Astronomy - Career Account Web Pages
Astronomy - Career Account Web Pages

... The most distant objects in the universe appear extremely red because their light is stretched to longer, redder wavelengths by the expansion of the universe. This object is at an extremely faint magnitude of 29, which is 500 million times fainter that the faintest stars seen by the human eye. The d ...
Lecture notes - itü | fizik mühendisliği
Lecture notes - itü | fizik mühendisliği

... nucleus is made up of frozen gases and dust. Eccentric orbit around the Sun. Most comets spend most of their time at vast distances from the Sun. When they approach the Sun, some gases will be vaporized and an extended coma will then be produced (of size 100000 km). The tail can be up to 1AU long. O ...
How the Solar System formed
How the Solar System formed

... nucleus is made up of frozen gases and dust. Eccentric orbit around the Sun. Most comets spend most of their time at vast distances from the Sun. When they approach the Sun, some gases will be vaporized and an extended coma will then be produced (of size 100000 km). The tail can be up to 1AU long. O ...
How the Solar System formed
How the Solar System formed

... nucleus is made up of frozen gases and dust. Eccentric orbit around the Sun. Most comets spend most of their time at vast distances from the Sun. When they approach the Sun, some gases will be vaporized and an extended coma will then be produced (of size 100000 km). The tail can be up to 1AU long. O ...
AWG recommendation on Cosmic Vision
AWG recommendation on Cosmic Vision

... After the first discovery of an extra-solar planet in 1995, there has been steady progress towards detecting planets with ever smaller masses, and towards the development of a broader suite of techniques to characterize their properties. There is no doubt that this trend will continue into the next ...
Earth - Space Science - Volusia County Schools
Earth - Space Science - Volusia County Schools

... • collect, analyze, and interpret data from the experiment to draw conclusions • determine an experiment’s validity and justify its conclusions based on: o control group, limiting variables and constants, multiple trials (repetition) or large sample sizes, bias, method of data collection, analysis, ...
Chapter 2
Chapter 2

... Complete the following concept map by correctly adding the connecting phrases or terms provided to the appropriate locations. Some items may be used more than once; others may not be applicable to this diagram. 1. converts simple elements such as 2. present in 3. for example 4. extrasolar planets su ...
Word - Lyon College
Word - Lyon College

... NASA achieve its goal of returning astronauts to the Moon by 2020. The U.S. Air Force spent a decade and well over $1 billion developing the Delta 4 and Atlas 5 under its Evolved Expendable Launch Vehicle (EELV) program, and the White House and Department of Defense want NASA to leverage that invest ...
Name - crespiphysics
Name - crespiphysics

... 1. What fraction of the sun’s energy that is intercepted by the earth does the earth actually absorb? As a result, what is the earth’s average temperature in degrees Fahrenheit (yes, I’m making you perform a conversion!)? What would the earth’s average temperature be (again in degrees Fahrenheit) if ...
Pluto and Kuiper Belt Object Notes
Pluto and Kuiper Belt Object Notes

... a) These comets seem to come from the Kuiper belt, a flatter distribution of objects beyond the orbit of Neptune. b) Comets on highly eccentric orbits spend most of their time far away from the Sun, an excellent example of Keppler’s second law. 6) As a comet gets closer to the Sun than those distant ...
Your Guide to the Universe
Your Guide to the Universe

... with their headlights on. One car is closer to you and the other one is further away. Which headlights would seem brighter and bigger? 3. Remember - even though it looks to us as if the Sun goes around the Earth, the real situation is that the Earth goes around the Sun. 4. The Sun is way bigger ...
The Interstellar Medium
The Interstellar Medium

... 20. The best vacuum chambers on Earth can reach densities of about 1,000,000 atoms per cubic centimeter. Which of the four components of the interstellar medium has lower densities than such a chamber? a. The hot coronal gas. b. The hot coronal gas and HII intercloud medium. c. The hot coronal gas, ...
A n   A n c i e n... How Astronomers Know the Vast Scale of Cosmic Time
A n A n c i e n... How Astronomers Know the Vast Scale of Cosmic Time

... wonderful universe. No wonder astronomy has inspired artists and poets through the ages, from ancient Greece to today’s television series. Astronomy, the study of the universe, reveals a cosmos that is vast, varied, and beautiful. The sky is our window on this universe. The sky and its contents are ...
02-Physics
02-Physics

... in the dense molecular clouds. These molecules may survive in comets and asteroids which could have bombarded the youthful Earth (and other planets) to provide an injection of organic molecules and volatiles (e.g. water) needed for their formation. Some speculation exists that life may ...
Science and the Universe - Wayne State University Physics and
Science and the Universe - Wayne State University Physics and

... Local Group of Galaxies M31, along with our Galaxy, is part of a small cluster of over 40 galaxies which is called the Local Group At distances of about 10 to 15 million LY, one finds other small galaxy groups or clusters At about 50 million LY, one finds a very large cluster containing thousands o ...
02. Earth in space
02. Earth in space

... Although we were able to explain Earth's position in space, the unique nature of our planet was not driven home until we were able to look at our home from the outside. The astronauts aboard the Apollo 8 spacecraft were the first to glimpse our home planet from space (Fig. 2). While orbiting the Moo ...
“Breakthroughs” of the 20th Century
“Breakthroughs” of the 20th Century

... The Universe did not just contain a single galaxy; there were actually huge numbers of them. (1999 Hubble Space Telescope observations led to an estimate of about 125 billion, and more recent modelling programs indicate that the number might be as high as 500 billion.) A second surprise was the real ...
Chapter 10
Chapter 10

... and death of stars, the theme of the next five chapters, we begin with a chapter about the gas and dust between the stars. It is the flour from which nature bakes stars. This chapter clearly illustrates how astronomers use the interaction of light and matter to learn about nature on the astronomical ...
absorption lines
absorption lines

... and death of stars, the theme of the next five chapters, we begin with a chapter about the gas and dust between the stars. It is the flour from which nature bakes stars. This chapter clearly illustrates how astronomers use the interaction of light and matter to learn about nature on the astronomical ...
Section 2 Movements of the Earth
Section 2 Movements of the Earth

... Why do scientists launch spacecraft beyond Earth’s atmosphere? Scientists launch spacecraft into orbit to detect radiation screened out by Earth’s atmosphere and to avoid light pollution and other atmospheric distortions. ...
1 VERSION 21A Cosmos+ A big bang family performance about the
1 VERSION 21A Cosmos+ A big bang family performance about the

... The solar system is the Earth’s cosmic family. It consists of everything that is held in by the grip of the Sun’s gravity: planets, dwarf planets, moons, comets, asteroids and other various small objects, and bigger things that have yet to be discovered. TOM7 The Sun and all the planets started out ...
Star Formation
Star Formation

... Visible (left) and infrared (right) views of the Orion nebula show new stars. These new stars can only been seen in infrared because the protostar’s cocoon nebula absorbs most of the visible light. ...
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Panspermia



Panspermia (from Greek πᾶν (pan), meaning ""all"", and σπέρμα (sperma), meaning ""seed"") is the hypothesis that life exists throughout the Universe, distributed by meteoroids, asteroids, comets, planetoids and, also, by spacecraft in the form of unintended contamination by microorganisms.Panspermia is a hypothesis proposing that microscopic life forms that can survive the effects of space, such as extremophiles, become trapped in debris that is ejected into space after collisions between planets and small Solar System bodies that harbor life. Some organisms may travel dormant for an extended amount of time before colliding randomly with other planets or intermingling with protoplanetary disks. If met with ideal conditions on a new planet's surfaces, the organisms become active and the process of evolution begins. Panspermia is not meant to address how life began, just the method that may cause its distribution in the Universe.Pseudo-panspermia (sometimes called ""soft panspermia"" or ""molecular panspermia"") argues that the pre-biotic organic building blocks of life originated in space and were incorporated in the solar nebula from which the planets condensed and were further —and continuously— distributed to planetary surfaces where life then emerged (abiogenesis). From the early 1970s it was becoming evident that interstellar dust consisted of a large component of organic molecules. Interstellar molecules are formed by chemical reactions within very sparse interstellar or circumstellar clouds of dust and gas. The dust plays a critical role of shielding the molecules from the ionizing effect of ultraviolet radiation emitted by stars.Several simulations in laboratories and in low Earth orbit suggest that ejection, entry and impact is survivable for some simple organisms.
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