pss_endl - University of Texas at Austin
... advantage: true masses (with Doppler), good for nearby stars! disadvantage: extreme precision (SIM) Micro-Lensing: advantage: sensitive to habitable zone planets disadvantage: requires star to move between us and background star Direct Imaging: advantage: it's a picture! (brightness, colors...) disa ...
... advantage: true masses (with Doppler), good for nearby stars! disadvantage: extreme precision (SIM) Micro-Lensing: advantage: sensitive to habitable zone planets disadvantage: requires star to move between us and background star Direct Imaging: advantage: it's a picture! (brightness, colors...) disa ...
STEP Mission: Search for Terrestrial Exo
... in predefined domains (additional programs). It requires some preparatory work, and the data reduction-without being exactly the same as Gaia will benefit from its developed structures. The data rate will reach 65Gb/day requiring the use of a 64-m antenna for 1.8 h each day. The final data processin ...
... in predefined domains (additional programs). It requires some preparatory work, and the data reduction-without being exactly the same as Gaia will benefit from its developed structures. The data rate will reach 65Gb/day requiring the use of a 64-m antenna for 1.8 h each day. The final data processin ...
Cat`s EyE - Chandra X
... ago because these objects looked like planets through small optical telescopes. Rather, a planetary nebula is a stage of life that our Sun will experience billions of years from now (see illustration below). ...
... ago because these objects looked like planets through small optical telescopes. Rather, a planetary nebula is a stage of life that our Sun will experience billions of years from now (see illustration below). ...
Another Earth in the Universe
... large stars and therefore are the best candidates for planetary systems in which life could be present. In fact, for biological evolution and for biochemical reactions to take place, very long periods of time are required, longer than the average age of the large stars. Furthermore, M dwarfs are ver ...
... large stars and therefore are the best candidates for planetary systems in which life could be present. In fact, for biological evolution and for biochemical reactions to take place, very long periods of time are required, longer than the average age of the large stars. Furthermore, M dwarfs are ver ...
The new europian project ROPACS (Rocky Planets Around …
... dwarf star with spectral type M3V, located 20.3 light years away from Earth. Its mass is estimated to be approximately a third of that of the Sun, and it is the 87th closest known star system to the Sun. Observations suggest that the star has at least four planets: Gliese 581 b, c, d, e. ...
... dwarf star with spectral type M3V, located 20.3 light years away from Earth. Its mass is estimated to be approximately a third of that of the Sun, and it is the 87th closest known star system to the Sun. Observations suggest that the star has at least four planets: Gliese 581 b, c, d, e. ...
PHYS 200 - Understanding the Universe
... deals with basic concepts in Astronomy in a descriptive way without using calculus. The students after completing this course should be able to: • grasp how physical principles are applied to understand cosmic objects. • Gain appreciation for science and scientific methods and to realize that progre ...
... deals with basic concepts in Astronomy in a descriptive way without using calculus. The students after completing this course should be able to: • grasp how physical principles are applied to understand cosmic objects. • Gain appreciation for science and scientific methods and to realize that progre ...
Questions to answer - high school teachers at CERN
... R* is the rate of star formation in our galaxy fp is the fraction of those stars that have planets ne is average number of planets that can potentially support life per star fl is the fraction of the above that actually go on to develop life fi is the fraction of the above that actually go on to dev ...
... R* is the rate of star formation in our galaxy fp is the fraction of those stars that have planets ne is average number of planets that can potentially support life per star fl is the fraction of the above that actually go on to develop life fi is the fraction of the above that actually go on to dev ...
Skymapper and Kepler K2: Finding the Origin of Hot Gas Giants
... determine which stars are young. • Data/pretty images prior to May 1 would really help the proposal for K2 targets! • This is standard “fast” survey data. ...
... determine which stars are young. • Data/pretty images prior to May 1 would really help the proposal for K2 targets! • This is standard “fast” survey data. ...
Volume 20 Number 4 March 2012 - Forsyth Astronomical Society
... The Kepler mission has discovered 11 new planetary systems hosting 26 confirmed planets. These discoveries nearly double the number of verified Kepler planets and triple the number of stars known to have more than one planet that transits (passes in front of) its host star. The planets orbit close t ...
... The Kepler mission has discovered 11 new planetary systems hosting 26 confirmed planets. These discoveries nearly double the number of verified Kepler planets and triple the number of stars known to have more than one planet that transits (passes in front of) its host star. The planets orbit close t ...
Top 5 Optical Telescopes
... polarimetric analysis of the radiation from astronomical objects out of reach of northern hemisphere telescopes Primary mirror is composed of an array of mirrors designed to act as a single larger mirror The mirror is made up of 91 identical hexagonal segments Is fixed at an elevation angle of 55° a ...
... polarimetric analysis of the radiation from astronomical objects out of reach of northern hemisphere telescopes Primary mirror is composed of an array of mirrors designed to act as a single larger mirror The mirror is made up of 91 identical hexagonal segments Is fixed at an elevation angle of 55° a ...
Terrestrial Planet (and Life) Finder
... Now estimate number of planets with life in our Galaxy (not number with intelligent, communicating life) If we leave out fi and fc (i.e. assume they are unity—all life forms develop our kind of intelligence and technology and try to communicate), we are calculating the number of life-bearing planet ...
... Now estimate number of planets with life in our Galaxy (not number with intelligent, communicating life) If we leave out fi and fc (i.e. assume they are unity—all life forms develop our kind of intelligence and technology and try to communicate), we are calculating the number of life-bearing planet ...
Astronomy Notes
... orbit once around the sun A month is roughly the amount of time required for the moon to orbit the Earth A day is the time required for the Earth to rotate once on its axis ...
... orbit once around the sun A month is roughly the amount of time required for the moon to orbit the Earth A day is the time required for the Earth to rotate once on its axis ...
Astronomy and Space articles by Martin George of the Launceston
... Many readers, no doubt, have watched one or more of the famous science fiction movies or series, with spectacular planetary landscapes and weird atmospheric effects. Some of them have two moons in the sky - quite a possible scenario for some planets, although we of course have only one. Another type ...
... Many readers, no doubt, have watched one or more of the famous science fiction movies or series, with spectacular planetary landscapes and weird atmospheric effects. Some of them have two moons in the sky - quite a possible scenario for some planets, although we of course have only one. Another type ...
The Daily Telegraph – London… 14th February 2008… New Solar
... Solar system because the two gas giant planets are similar sizes relative to their star as Jupiter and Saturn are to our sun. The smaller planet is roughly twice as far from its star as the larger one, just as Saturn is about twice as far from the sun as Jupiter. Planetary scientists who discovered ...
... Solar system because the two gas giant planets are similar sizes relative to their star as Jupiter and Saturn are to our sun. The smaller planet is roughly twice as far from its star as the larger one, just as Saturn is about twice as far from the sun as Jupiter. Planetary scientists who discovered ...
Ecology Review Science Department
... Using this information, the astronomer can conclude that the star A is older than the Sun. B will survive for several billion years. C is moving very quickly away from Earth. D has a mass similar to the mass of Jupiter. ...
... Using this information, the astronomer can conclude that the star A is older than the Sun. B will survive for several billion years. C is moving very quickly away from Earth. D has a mass similar to the mass of Jupiter. ...
WK10revisedoneweek
... the motions of the planets around the sun. •A comparison of the evolution and fate of high and low mass stars. •A description of Einstein’s Principle of Equivalence, its effects, and ...
... the motions of the planets around the sun. •A comparison of the evolution and fate of high and low mass stars. •A description of Einstein’s Principle of Equivalence, its effects, and ...
The Size and Structure of the Milky Way Galaxy
... Dark Matter: A Major Problem for Contemporary Physics and Astronomy • Stars are a small fraction of the mass of major galaxies • The dark matter problem becomes more pronounced as you go out in the universe • The form of the dark matter is unknown; probably not what you studied in chemistry • Possi ...
... Dark Matter: A Major Problem for Contemporary Physics and Astronomy • Stars are a small fraction of the mass of major galaxies • The dark matter problem becomes more pronounced as you go out in the universe • The form of the dark matter is unknown; probably not what you studied in chemistry • Possi ...
Name ______KEY Date Core ______ Study Guide Galaxies and the
... happened 14 billion years ago when the universe suddenly began to expand from one merged mass of matter or substance. At that time, all matter was dense and hot and the universe developed in less than a second. 300,000 years later, the first elements formed, then stars, planets and galaxies the next ...
... happened 14 billion years ago when the universe suddenly began to expand from one merged mass of matter or substance. At that time, all matter was dense and hot and the universe developed in less than a second. 300,000 years later, the first elements formed, then stars, planets and galaxies the next ...
Stellar Properties and Stellar Evolution Study Guide Name Why
... 5. A shock wave may be the stimulus that causes a nebula to start condensing to form new ...
... 5. A shock wave may be the stimulus that causes a nebula to start condensing to form new ...
Click here
... Supernovas: ___________________________ of a large star by explosion. o Produces silver, gold, and lead. ...
... Supernovas: ___________________________ of a large star by explosion. o Produces silver, gold, and lead. ...
An earthllke planet would have a rocky mantle surround
... row HZs close to the stars and are much longer lived. NASA's Kepler mission, scheduled at press time to launch in March. will tell us the frequency of earthlike planets in HZs. Kepler will look at 100,000 nearby stars in the direction of our galaxy's Orion Ann. It will measure slight dips in a star' ...
... row HZs close to the stars and are much longer lived. NASA's Kepler mission, scheduled at press time to launch in March. will tell us the frequency of earthlike planets in HZs. Kepler will look at 100,000 nearby stars in the direction of our galaxy's Orion Ann. It will measure slight dips in a star' ...
notes
... today and other stars that are ten billion years old, so unlike the planets of the Solar System, which can only be observed as they are today, studying exoplanets allows the observation of exoplanets at different stages of evolution. • When planets form they have hydrogen envelopes that cool and con ...
... today and other stars that are ten billion years old, so unlike the planets of the Solar System, which can only be observed as they are today, studying exoplanets allows the observation of exoplanets at different stages of evolution. • When planets form they have hydrogen envelopes that cool and con ...
PARTS OF THE UNIVERSE
... v Parallax: apparent shift in the position of an object when view from two different locations. v Parallax Example v Can be used to measure the distance of stars from Earth that are relatively close. v Proxima Centauri: closest star to earth v (4.3 light years away – 40 trillion km) ...
... v Parallax: apparent shift in the position of an object when view from two different locations. v Parallax Example v Can be used to measure the distance of stars from Earth that are relatively close. v Proxima Centauri: closest star to earth v (4.3 light years away – 40 trillion km) ...
The universe
... Planets around the sun and the surrounding planets revolve around the center of the galaxy (Milky Way). ...
... Planets around the sun and the surrounding planets revolve around the center of the galaxy (Milky Way). ...
Space Interferometry Mission
The Space Interferometry Mission, or SIM, also known as SIM Lite (formerly known as SIM PlanetQuest), was a planned space telescope developed by the U.S. National Aeronautics and Space Administration (NASA), in conjunction with contractor Northrop Grumman. One of the main goals of the mission was the hunt for Earth-sized planets orbiting in the habitable zones of nearby stars other than the Sun. SIM was postponed several times and finally cancelled in 2010.In addition to hunting for extrasolar planets, SIM would have helped astronomers construct a map of the Milky Way galaxy. Other important tasks would have included collecting data to help pinpoint stellar masses for specific types of stars, assisting in the determination of the spatial distribution of dark matter in the Milky Way and in the Local Group of galaxies and using the gravitational microlensing effect to measure the mass of stars.The spacecraft would have used optical interferometry to accomplish these and other scientific goals. This technique collects light with multiple mirrors (in SIM's case, two) which is combined to make an interference pattern which can be very precisely measured.The initial contracts for SIM Lite were awarded in 1998, totaling US$200 million. Work on the SIM project required scientists and engineers to move through eight specific new technology milestones, and by November 2006, all eight had been completed.SIM Lite was originally scheduled for a 2005 launch, aboard an Evolved Expendable Launch Vehicle (EELV). As a result of continued budget cuts, the launch date has been pushed back at least five times. NASA has set a preliminary launch date for 2015 and U.S. federal budget documents confirm that a launch date is expected ""no earlier"" than 2015. The budget cuts to SIM Lite are expected to continue through FY 2010. As of February 2007, many of the engineers working on the SIM program had moved on to other areas and projects, and NASA directed the project to allocate its resources toward engineering risk reduction. However, the preliminary budget for NASA for 2008 included zero dollars for SIM.In December 2007, the Congress restored funding for fiscal year 2008 as part of an omnibus appropriations bill which the President later signed. At the same time the Congress directed NASA to move the mission forward to the development phase. In 2009 the project continued its risk reduction work while waiting for the findings and recommendations of the Astronomy and Astrophysics Decadal Survey, Astro2010, performed by the National Academy of Sciences, which would determine the project's future.On 13 August 2010, the Astro2010 Decadal Report was released and did not recommend that NASA continue the development of the SIM Lite Astrometric Observatory. This prompted NASA Astronomy and Physics Director, Jon Morse, to issue a letter on 24 September 2010 to the SIM Lite project manager, informing him that NASA was discontinuing its sponsorship of the SIM Lite mission and directing the project to discontinue Phase B activities immediately or as soon as practical. Accordingly, all SIM Lite activities were closed down by the end of calendar year 2010.