astrophysics
branch of astronomy concerned primarily with the properties and structure of cosmic objects, including the universe as a whole. See astronomy.
Harvard-Smithsonian Center for Astrophysics
astronomical research institution headquartered in Cambridge, Massachusetts, U.S., on the campus of Harvard University. The CfA was created in 1973 by reorganizing the Harvard College Observatory and ...
Eddington, Sir Arthur Stanley
English astronomer, physicist, and mathematician who did his greatest work in astrophysics, investigating the motion, internal structure, and evolution of stars. He also was the first expositor of ...
Osterbrock, Donald Edward
American astrophysicist was conducting research as a graduate student when he discovered the spiral-arm structure of the Milky Way, and he later uncovered the processes that show how the Sun retains ...
Emden, Robert
physicist and astrophysicist who developed a theory of expansion and compression of gas spheres and applied it to stellar structure.
Handymen need not worry - The Sun
When your brain goes wrong, you cannot save money by operating on it yourself. Likewise, when the engine mapping system in your car goes berserk — and if it’s French, it will ...
INTEGRATED CIRCUIT AT 50 - International Herald Tribune
Today, a state-of-the-art chip contains more than a billion components packed into an area the size of a human fingernail. The question is whether the semiconductor industry can ...
Glenn Burns - WSB-TV Atlanta
Glenn Burns is the chief meteorologist for Channel 2 Action News' Severe Weather Team 2. He is an AMS certified meteorologist and appears on the 5, 6 and 11 p.m. newscasts Monday ...
Pinning down the Milky Way's spin - PhysOrg
Artist's impression of the local neighbourhood of the Sun and its setting within our galaxy, the Milky Way (see insert above). The figure shows the positions of some bright stars ...
Astronomers Discover Most Dark Matter-dominated Galaxy In Universe - Science Daily
ScienceDaily (Sep. 19, 2008) — A team led by a Yale University astronomer has discovered the least luminous, most dark matter-filled galaxy known to exist. The galaxy, called ...
Young Star Blasts Water To Pieces - Redorbit.com
Water is being blasted to pieces by a young star's laser-like jets, according to new observations from NASA's Spitzer Space Telescope. The discovery provides a better understanding ...
Liberty works in all areas, and that includes economy - Yuma Daily Sun
By all historical accounts the fully free society has never been tried, so arguing about it will always be to a large extent theoretical. But then nearly all of contemporary ...
Usain Bolt 'could have run 9.55 seconds in Olympic final' - Daily Telegraph
Usain Bolt lost precious time when he slowed down at the end of the race to celebrate - but still broke the world record Photo: Getty Images The Jamaican gold medallist broke the ...
Rock review: Queen and Paul Rodger, The Cosmos Rocks - Guardian Unlimited
Oh dear. Imagine Brian got his astrophysics PhD in '72, took that career path instead, and only formed a band now, aged 61. The result might be pub rock tosh with stadium reverb ...
Boffins calculate true speed of 'Lightning' Bolt - The Register
Physicists at the Institute of Theoretical Astrophysics at the University of Oslo have applied themselves to that most pressing of matters - how fast might Usain Bolt have run the ...
Rob's Westminster and Parliament day trip (and a pretty fun looking pub and some more pictures of everyone's favorite oversized clock).
Author: artifex85 Keywords: Westminster Parliament London astrophysicist Added: September 19, 2008
This is the first 'oddity' I encountered in the Space stage of Spore. When you visit it you get a post of your discovery in your trophy bin. I thought it was so cool looking that it had to be put in a video.
Author: bsgcylon86 Keywords: Spore Space Protoplanetary Disk disk outerspace game stars astronomy astrophysics Added: September 19, 2008
Heavenly Bodies (1920s)Visionary 1920s film containing imaginative astrophysical visualizations.Producer: UnknownAudio/Visual: Si, B&WKeywords: Astronomy; Physics
Author: CharacterControl Keywords: Heavenly Bodies 1920s Visionary imaginative astrophysical visualizations Astronomy Physics Physical Science Humanities Social Media Maths Computer Communications Added: September 19, 2008
Narration:The concept of a Star Tracker probably can be traced back to the early sailors who used to navigate the open seas. The concept is they use star field patterns in order to tell them where theyre pointed, while they are sailing from east to west or north to south, whatever direction they were going.The Star Tracker is a lot more complicated in that it uses the entire star field pattern to provide attitude knowledge or, in the laymens term, more of the direction in which the spacecraft is pointing while it is orbiting the Earth or doing wherever its science mission requires it to do. So, essentially, its an optical device to access the eyes of the spacecraft.The Star Tracker was built for the Lunar Reconnaissance Orbiter and the Solar Dynamics Observatory, both NASA missions in Florence, Italy by Galileo Avianica. They write their own software used to operate the star trackers, ground all of their optics, fabricate the structures, and assemble and test the electronics.Once the star trackers are assembled, Galileo Avionica works with NASA engineers in order to ensure that the star trackers are built to achieve their performance requirement as well as their environmental requirement. The LRO and SDO missions both use two star trackers for redundancy, so that if you get a fair unit in one, the second star tracker will be used as the backup.Also, the use of two star trackers provided added or increased performance accuracy so that the spacecraft will have a more accurate knowledge of where it's pointed while its orbiting either the moon, the Earth, or the Sun. NASA is an educational extension of the government.Through all the information we get from all our various missions, we learn things about our Earth, space, how space effects Earth, and our changing environment. All of these things are important to everyone in the world, whether we know it our not, and the importance of star tracker, is they act as the eyes of the satellite to let the satellite know where its going in order to get the information we need.For more visit us at www.figbranch.com
Author: FigBranchcom Keywords: astronomy stars space science astrophysics Added: September 19, 2008
Out-takes from recent trip to Namibia. Roo Ellis makes standing still and talking English look like Astro-Physics while the cattle behind him enjoy the moment too!
Author: TheHuntingAgency Keywords: cattle blooper out-take edit screwing cows Roo namibia africa mistake humour error Added: September 19, 2008
Interview with Professor Chris McKee, UC Berkeley
Author: opensourceteaching Keywords: opensourceteaching stars galaxies quasars black holes Added: September 18, 2008
Timothy Beers, professor of astronomy and physics at Michigan State University, discusses his research on the formation of the earliest stars in the universe. The first stars born out of the Big Bang were very massive with short lives and exploded. Low mass stars formed shortly after these massive stars. Their atmospheres contain elemental abundances produced from the massive stars. From this evidence, we are learning how elements heavier than hydrogen and helium formed. This helps us to understand the murkiest part of the universe's history, the story at the beginning. One star showed a strong signature of R-process elements that are found at the end of the periodic table. The abundance of Uranium-238 and Thorium-232 provides two atomic clocks. If you measure the rate of the ticking, then you can find when the ticking began.To find out more, please visit us at http://figbranch.com/index.php?option=com_content&task=view&id=475&Itemid=32Credit: NSCL
Author: FigBranchcom Keywords: space physics astrophysics sun stars astronomy Added: September 18, 2008
Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a rich galaxy cluster (10^15 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 5 Myr; total time of integration is 820 Myr. The box is 100 kpc in size: the central region of a rich glaxy cluster (e.g. A1795).The model is B2: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.001 (2). This is one of the best models: cooling rate are ~1-10% of the cooling flow standard model; the central temperature, density and SB profiles resembles the observational data (s. thesis); the evolution of the map (in the video) shows the typical X-bubbles and weak shocks (s. Perseus). For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press Watch in High Quality, bottom-right, for the proper film resolution]
Author: MaxGaspari Keywords: Astrophysics galaxy clusters cooling flow X-Rays simulation 3D Added: September 17, 2008
Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a rich galaxy cluster (10^15 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 10 Myr; total time of integration is 820 Myr. The box is 100 kpc in size: the central region of a rich glaxy cluster (e.g. A1795).The model is B2: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.1 (1). This is an extreme model (bad): cooling rate are ~1% of the cooling flow standard model; the central temperature (too high), density and SB profiles (too low) don't resemble the observational data (s. thesis); the evolution of the map (in the video) doesn't show the typical X-bubbles and weak shocks (s. Perseus). Instead the onedirectional channel of the outflow persists and cuts the system during all the simulation. For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press Watch in High Quality, bottom-right, for the proper film resolution]
Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a rich galaxy cluster (10^15 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 5 Myr; total time of integration is 820 Myr. The box is 100 kpc in size: the central region of a rich glaxy cluster (e.g. A1795).The model is B2: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.00001 (3). This is an extreme model (bad): cooling rate are ~80-90% of the cooling flow standard model; the central temperature (too low), density and SB profiles (too high) don't resemble the observational data (s. thesis); the evolution of the map (in the video) doesn't show the typical X-bubbles (s. Perseus). The cooling flow persists in time and only the nucleus of the cluster is slightly affected by heating of the outflow. For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press Watch in High Quality, bottom-right, for the proper film resolution]
Astro-Physics Inc.
Telescopes, mounts and accessories for observers and astrophotographers. ... Astro-Physics, Inc. 11250 Forest Hills Road, Machesney Park, IL 61115, U.S.A. ...
Astrophysics - Wikipedia, the free encyclopedia
Astrophysics is the branch of astronomy that deals with the physics of the ... as the basis for black hole (astro)physics and the study of gravitational waves. ...
Glossary of Astrophysics
Watch the creation of elements ... The Universe as a whole is the best labratory ... a b c d e f g h i j k l m n o p q r s t u v w x y z. Alpha-Carbon Reaction ...
What is Astrophysics? What is High Energy Astrophysics?
This site is intended for students age 14 and up, and for anyone interested in learning about our universe. ... I was just wondering exactly what astrophysics is? ...
Harvard Smithsonian - Center for Astrophysics Division of Optical and ...
... comprising the astronomy and astrophysics programs of two renowned scientific ... Laboratory Astrophysics. Extreme Astrophysics ...
ScienceDaily: Astrophysics News
Astrophysics and space science. From microquasars to dark matter, read all the ... Astrophysics. Extrasolar Planets. Beautiful Death: Halos Of Planetary ...
ScienceDaily: Astrophysics Articles
Astrophysics and space science. From microquasars to dark matter, read all the ... Astrophysics. Extrasolar Planets. Astronomy. Planetary nebula ...
Scientific American: Astrophysics
Find the latest Astrophysics articles, news, and information from the physics experts at Scientific American ... Topics: Astrophysics , Electrical Engineering , ...
Astrophysics - Simple English Wikipedia, the free encyclopedia
Astrophysics is the study of how stars and planets work, and how we can learn about them. ... Observational astrophysics is like astronomy. ...
Astrophysics at the NSSDC
National Space Science Data Center (NSSDC) Astrophysics Page ... HEASARC (High Energy Astrophysics Science Archive Research Center) ...
Greatest Physicists #9 - J.J Thomson [Built on Facts]
#9 - J.J. Thomson The entire edifice of chemistry is a theme and variation on the study of the properties of atomic electrons. Tremendous sections of physics, from solid state to quantum optics to AMO and beyond hings almost entirely on electron behavior. Astrophysics, spectroscopy, and large chunks of high energy physics rely on the understanding of the electron. And those are just the leading edge of what the electron means to modern science. More than anyone else, we owe J.J. Thomson for
Pinning down the Milky Way’s spin
Pinning down the Milky Way’s spin September 19th, 2008 New, very precise measurements have shown that the rotation of the Milky Way is simpler than previously thought. A remarkable result from the most successful ESO instrument HARPS, shows that a much debated, apparent ‘fall’ of neighbourhood Cepheid stars towards our Sun stems from an intrinsic property of the Cepheids themselves. Posted in Astrophysics
Sophmore year
Hallo everybody! ^_^ Man, I’m soo happy. Today, I finished my first week of the fisrt semester of my sophmore year (hope it stays sophmore and doesn’t become a suffer-more year :P) anyways, I’m just plain happy. I love all the courses I choose this semester… all.. except one: biology. But before I rattle on about why I dislike it, I shall first talk about the ones I do like! So this semester, we have to take Theoretical Mechanics and Electrodynamics, as well as Physics Lab as department r
Greatest Physicists #9 - J.J Thomson
Greatest Physicists #9 - J.J Thomson Category: Physical Science #9 - J.J. Thomson The entire edifice of chemistry is a theme and variation on the study of the properties of atomic electrons. Tremendous sections of physics, from solid state to quantum optics to AMO and beyond hings almost entirely on electron behavior. Astrophysics, spectroscopy, and large chunks of high energy physics rely on the understanding of the electron. And those are just the leading edge of what the electron means t
TATA INSTITUTE OF FUNDAMENTAL RESEARCH (TIFR) ADMISSION 2009-2010: Ph.D, INTEGRATED Ph.D, MSc in BIOLOGY [MATHS, PHYSICS, CHEMISTRY, BIOLOGY etc]
TATA INSTITUTE OF FUNDAMENTAL RESEARCH (TIFR)(A DEEMED UNIVERSITY)Homi Bhabha Road, Colaba, Mumbai 400005.Fax: (022) 2280 4555/4610/4611; Phone: (022) 2278 2875/2629/2241E-mail: gsch@tifr.res.in Website: http://univ.tifr.res.in; http://www.tifr.res.in/admissions Advertisement No. 8/2008PH.D. PROGRAMME IN MATHEMATICS, PHYSICS, CHEMISTRY, BIOLOGY, COMPUTER & SYSTEMS SCIENCES AND SCIENCE EDUCATIONINTEGRATED PH.D. PROGRAMME IN MATHEMATICS (BANGALORE) AND BIOLOGY;M.SC. PROGRAMME IN BIOLOGYThe Tata
09/17/08: XMM-Newton Discovers Periodic Signal in Black Hole.
XMM-Newton Discovers Periodic Signal in Black Hole. XMM-Newton has uncovered a well-tuned periodic signal from a super-massive black hole lodged at the centre of a galaxy, ending a long quest for such an object. The discovery provides scientists with a clearer picture on black hole accretion processes and an excellent tool to study active galactic nuclei (AGNs). These periodic signals originating from the black hole are emitted in X-rays, which are blocked out by the Earth's atmosphere.
Cepheids - Milky Way Motion Not So Complex
Cepheids - Milky Way Motion Not So Complex Submitted by News Staff on 19 September 2008 - 10:45am. Space Precise measurements by the ESO instrument HARPS now show that the rotation of the Milky Way is simpler than previously thought - the much debated, apparent 'fall' of neighborhood Cepheid stars towards our Sun stems from an intrinsic property of the Cepheids themselves, say a group of astrophysicists led by Nicolas Nardetto in a Astronomy & Astrophysics article. Since Henrietta Leavitt'
ASTROPHYSICS LIMITED
Registered Address: 7/8 EGHAMS COURT, BOSTON DRIVE, BOURNE END, BUCKS, SL8 5YS
Website: The owner of the business has not provided a URL to Topicala Business.
Telephone: The owner of the business has not provided a telephone number to Topicala Business.
ASTROPHYSICS INTERNATIONAL LIMITED
Oxford Astrophysics : information
Theoretical astrophysics, people, graduate study, and seminars.
Astrophysics
Astrophysics Group ... Chandra Arp220 xray image. Welcome to the web site of the Astrophysics group at Imperial College, London.
Astrophysics Group - Department of Physics - University of Cambridge
A wide-ranging program of research, including the Mullard Radio Astronomy Observatory, situated at Lord's Bridge. Group members, research interests, publications, surveys and ...
Astrophysics Research Institute - Liverpool John Moores University
The Astrophysics Research Institute at Liverpool John Moores University is one of the world's leading authorities in Astronomy and Astrophysics.
Astrophysics is the branch of astronomy that deals with the physics of the universe, including the physical properties (luminosity, density, temperature, and chemical composition ...
The University of Manchester Galactic Astrophysics & Astrochemistry ...
Galactic Astrophysics & Astrochemistry Group. Welcome to the home page of the Galactic Astrophysics & Astrochemistry Group, part of the Jodrell Bank Centre for Astrophysics in the ...
Centre for Astrophysics Research (University of Hertfordshire)
The Centre for Astrophysics Research (CAR) carries out research on a range of key science questions in astronomy. Research programmes include observations covering wavelengths ...
Astronomy and Astrophysics Group Welcome Page
astronomy and astrophysics at the university of glasgow ... University of Glasgow Glasgow G12 8QQ: Astronomy secretary Tel +44 (0) 141 330 4152
QUB Astrophysics Research Centre
Staff in the Astrophysics Research Centre (ARC) carry out research in a number of stellar, Galactic and solar system areas. We are an observational astronomy group employing both ...
Bristol University - Department of Physics - Astrophysics Group
Bristol Astrophysics home page ... The Astrophysics Group in the Department of Physics at Bristol is highly research-active.
White Dwarf
IMG_8400 Fun with Astronomy
Barred Spiral Galaxy
The Astro-Physics Building in 1939
Rough Trade Unsigned - Astrophysics
Superstrings
Listen......
Jodrell Bank
Keck Telescopes
"... And then I remember that I have a degree in astrophysics from Cal Tech; I must not be stupid" --Rock
Feelin sleepy, doing astrophysics hmwk, doing laundry, packing, looking cute?
Work microwave and coffeepot were blowing fuses. Today they're plugged into separate outlets. Took 25 astrophysics PhDs 18 months to solve.
@eldiblito_72 What's even more weird is that May's degree is in Astrophysics I believe.
who the hec cares about what I'm doing? ????
feeling pretty lost here
New York, London, Paris, Munich; everybody talk about experimental Dysonian astrophysics.
NASA Advisory Council Science Committee Astrophysics Subcommittee Meeting 6-9 Oct 2008 http://tinyurl.com/4e4xyq
learning about twitter
is up on a gorgeous fall morning. Astrophysics and hiking is up for today!
UK challenge to Big Bang machine
Scientists working from a laboratory at the bottom of Britain's deepest mine could beat a multibillion-pound Swiss project to crack the mystery of creation.
Cosmic crash unmasks dark matter
Striking evidence has been found for the enigmatic "stuff" called dark matter which makes up 23% of the Universe.
Black holes 'dodge middle ground'
For black holes, there appears to be very little room for mediocrity, astronomers have found.
Life from Venus blown to Earth?
Scientists suggest microbes from Venus could be blown to Earth by powerful winds.
Funding secured for observatory
Committed funds secure the future of Jodrell Bank, one of the world's leading radio astronomy centres.
Jodrell Bank future looks better
The future of eMerlin, an upgrade to the world-famous Jodrell Bank observatory, is starting to look brighter.
Trio of 'super-Earths' discovered
Astronomers have identified a trio of so-called "super-Earths" - rocky planets between two and 10 times the mass of Earth.
England v NZ Twenty20 as it happened
England win the Twenty20 international against New Zealand by nine wickets at Old Trafford.
Computer speeds up college work
Cardiff University hopes to put Wales on the research map with its new high performance computer.
Universe twice as bright as known
Scientists in St Andrews discover that dust particles are heavily blocking light from distant galaxies.
ScienceDaily Headlines: Space & Time
Astronomy Resources
Tribe.net: Quantum Physics
astra physics updates on arXiv.org
The Astronomer's Telegram: Top ATels
Category:Astrophysics - Wikipedia, the free encyclopedia
Astrophysics is the branch of astronomy that deals with the physics of the universe, including the physical properties (luminosity, density, temperature, chemical composition) of ...
Astronomy - Wikipedia, the free encyclopedia
An Introduction to Astronomy and Astrophysics. Berlin, New York: Springer. ISBN 3-540-67877-8. ^ a b B. Scharringhausen. Curions About Astronomy:
Astronomy and astrophysics - Wikipedia, the free encyclopedia
Astronomy and astrophysics may refer to: the physical science fields of study of astronomy and astrophysics; Astronomy and Astrophysics, a peer reviewed scientific journal
Harvard-Smithsonian Center for Astrophysics - Wikipedia, the free ...
The Harvard-Smithsonian Center for Astrophysics (CfA) is an astronomy research and education institution. The center was founded in 1973 by a joint venture between the Smithsonian ...
Nuclear astrophysics - Wikipedia, the free encyclopedia
Nuclear astrophysics is the branch of nuclear physics that deals with explaining the formation, via nuclear reactions, of all the naturally occurring chemical elements in the ...
Accretion (astrophysics) - Wikipedia, the free encyclopedia
In astrophysics, the term accretion is used for at least two distinct processes. The first and most common is the growth of a massive object by gravitationally attracting more ...
Astrophysics Data System - Wikipedia, the free encyclopedia
The NASA Astrophysics Data System (usually referred to as ADS) is an online database of over 5,000,000 astronomy and physics papers from both peer reviewed and non-peer reviewed ...
Astronomy and Astrophysics - Wikipedia, the free encyclopedia
Astronomy and Astrophysics (abbreviated as A&A in the astronomical literature, or else Astron. Astrophys.) is a European Journal, publishing papers on theoretical, observational ...
Indian Institute of Astrophysics - Wikipedia, the free encyclopedia
The Indian Institute of Astrophysics (IIA), with its headquarteres in Bangalore (Karnataka state), India, is a premier national institute of India for study of and research in ...
Spore- Space- Protoplanetary Disk
Spore- Space- Protoplanetary Diskbsgcylon8631 sec - 20 Sep 2008This is the first 'oddity' I encountered in the Space stage of Spore. When you visit it you get a post of your discovery in your trophy bin. I thought it was so cool looking that it had to be put in a video.
Star Trackers Lights the Way
Star Trackers Lights the WayFigBranchcom3 min - 19 Sep 2008Narration:The concept of a Star Tracker probably can be traced back to the early sailors who used to navigate the open seas. The concept is they use star field patterns in order to tell them where theyre pointed, while they are sailing from east to west or north to south, whatever direction they were going.The Star Tracker is a lot more complicated in that it uses the entire star field pattern to provide attitude knowledge or, in the laymens term, more of the direction in which the spacecraft is pointing while it is orbiting the Earth or doing wherever its science mission requires it to do. So, essentially, its an optical device to access the eyes of the spacecraft.The Star Tracker was built for the Lunar Reconnaissance Orbiter and the Solar Dynamics Observatory, both NASA missions in Florence, Italy by Galileo Avianica. They write their own software used to operate the star trackers, ground all of their optics, fabricate the structures, and assemble and test the electronics.Once the star trackers are assembled, Galileo Avionica works with NASA engineers in order to ensure that the star trackers are built to achieve their performance requirement as well as their environmental requirement. The LRO and SDO missions both use two star trackers for redundancy, so that if you get a fair unit in one, the second star tracker will be used as the backup.Also, the use of two star trackers provided added or increased performance accuracy so that the spacecraft will have a more accurate knowledge of where it's pointed while its orbiting either the moon, the Earth, or the Sun. NASA is an educational extension of the government.Through all the information we get from all our various missions, we learn things about our Earth, space, how space effects Earth, and our changing environment. All of these things are important to everyone in the world, whether we know it our not, and the importance of star tracker, is they act as the eyes of the satellite to let the satellite know where its going in order to get the information we need.For more visit us at www.figbranch.com
DrRiccardoDeSalvo.MPG
Matter Antimatter Wars
Matter Antimatter Warsartysci1013 min - 18 Sep 2008When particles collide. Written by SF Bay Area high school students for the 2008 BCCP Cosmology Workshop. After 6 days of learning about the history of the universe, students had to write a script of a cosmology concept. They wrote the script and music during the last 2 days of the workshop and we rehearsed and shot the video in an hour. http://bccp.lbl.gov/Academy/workshop2.htmlBCCP homepage:http://bccp.lbl.gov/
Archaeology of the Stars
Archaeology of the StarsFigBranchcom7 min - 18 Sep 2008Timothy Beers, professor of astronomy and physics at Michigan State University, discusses his research on the formation of the earliest stars in the universe. The first stars born out of the Big Bang were very massive with short lives and exploded. Low mass stars formed shortly after these massive stars. Their atmospheres contain elemental abundances produced from the massive stars. From this evidence, we are learning how elements heavier than hydrogen and helium formed. This helps us to understand the murkiest part of the universe's history, the story at the beginning. One star showed a strong signature of R-process elements that are found at the end of the periodic table. The abundance of Uranium-238 and Thorium-232 provides two atomic clocks. If you measure the rate of the ticking, then you can find when the ticking began.To find out more, please visit us at http://figbranch.com/index.php?option=com_content&task=view&id=475&Itemid=32Credit: NSCL
AGN Heating 3D Simulation (rich galaxy cluster; B2)
AGN Heating 3D Simulation (rich galaxy cluster; B2)MaxGaspari1 min - 17 Sep 2008Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a rich galaxy cluster (10^15 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 5 Myr; total time of integration is 820 Myr. The box is 100 kpc in size: the central region of a rich glaxy cluster (e.g. A1795).The model is B2: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.001 (2). This is one of the best models: cooling rate are ~1-10% of the cooling flow standard model; the central temperature, density and SB profiles resembles the observational data (s. thesis); the evolution of the map (in the video) shows the typical X-bubbles and weak shocks (s. Perseus). For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press "Watch in High Quality", bottom-right, for the proper film resolution]
AGN Heating 3D Simulation (rich galaxy cluster; B1)
AGN Heating 3D Simulation (rich galaxy cluster; B1)MaxGaspari31 sec - 17 Sep 2008Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a rich galaxy cluster (10^15 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 10 Myr; total time of integration is 820 Myr. The box is 100 kpc in size: the central region of a rich glaxy cluster (e.g. A1795).The model is B2: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.1 (1). This is an extreme model (bad): cooling rate are ~1% of the cooling flow standard model; the central temperature (too high), density and SB profiles (too low) don't resemble the observational data (s. thesis); the evolution of the map (in the video) doesn't show the typical X-bubbles and weak shocks (s. Perseus). Instead the onedirectional channel of the outflow persists and cuts the system during all the simulation. For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press "Watch in High Quality", bottom-right, for the proper film resolution]
AGN Heating 3D Simulation (rich galaxy cluster; B3)
AGN Heating 3D Simulation (rich galaxy cluster; B3)MaxGaspari31 sec - 17 Sep 2008Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a rich galaxy cluster (10^15 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 5 Myr; total time of integration is 820 Myr. The box is 100 kpc in size: the central region of a rich glaxy cluster (e.g. A1795).The model is B2: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.00001 (3). This is an extreme model (bad): cooling rate are ~80-90% of the cooling flow standard model; the central temperature (too low), density and SB profiles (too high) don't resemble the observational data (s. thesis); the evolution of the map (in the video) doesn't show the typical X-bubbles (s. Perseus). The cooling flow persists in time and only the nucleus of the cluster is slightly affected by heating of the outflow. For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press "Watch in High Quality", bottom-right, for the proper film resolution]
AGN Heating 3D Simulation (galaxy group; B3)
AGN Heating 3D Simulation (galaxy group; B3)MaxGaspari33 sec - 17 Sep 2008Advanced hydrodynamical and astrophysical 3D simulation of a jet outflow, generated from an active galactic nucleus at the center of a galaxy group (4x10^13 Msun). It was computed with YGUAZU'-A code (in FORTRAN language), in order to study the problem of cooling flow in these cosmological systems.The video refers to the specialistic thesis of Massimo Gaspari, entitled ''Cooling vs. Heating in galaxy clusters and groups & hydrodynamical 3D simulations with AGN outflow''. It shows an evolution of the density map (xz plane through center) with the temperature levels and velocity field superimposed. Each frame represents a timestep of 10 Myr; total time of evolution is 870 Myr. The box is 28 kpc in size: the central region of a galaxy group (e.g. NGC 5044).The model is B3: the feedback of the AGN outflow is self-regulated (B) by the accretion on the BH with an efficieny of 0.00001 (3). This is one of the best models for galaxy group: the central temperature, density and SB profiles resemble the observational data (s. thesis); the evolution of the map (in the video) shows very small X-bubbles and weak shocks (need more resolution). The cooling rate is not much reduced: ~70% of the cooling flow standard model; but it seems that galaxy groups don't need a strong heating (s. T and n profile of NGC 5044) like clusters. They are the most delicate system to compute.For further informations just contact me: gaspmax@hotmail.comMassimo Gaspari(Department of Astronomy, University of Bologna, Italy)[Press "Watch in High Quality", bottom-right, for the proper film resolution]
Elvis Presley Jailhouse Psychedelic Trance 1957
Elvis Presley Jailhouse Psychedelic Trance 1957thelabel3553 min - 17 Sep 2008Elvis Presley is alive & dancing Psychedelic TranceMusic By:Psychedelic Trance ExperienceTrack Name:AstrophysicsFrom the Album:The History Of Trance
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