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  1. Journey To The Interstellar Medium

  2. 17 Apr 2008 at 12:43am



    3 min - Apr 17, 2008

    Another poem I wrote quite awhile ago. Not sure if it's any good, but thought I'd share. :) Pulled into the sky. Out into space. Floating above the earth. Now accelerating, faster and faster, up to the interstellar medium. An invisible halo, surrounding distant shining stars. Where we were born. Where we return to when we die. Where we will be born again. The journey to the interstellar medium, is the journey towards a new beginning. A force of gravity, pulling me back to earth. Life flourishing, within a beautiful heaven, residing in the galaxy of the Milky Way.



  3. Solar wind interacting with interstellar medium

  4. 3 Apr 2008 at 1:38pm



    5 sec - Apr 3, 2008

    This animation illustrates how the constant outflow of particles from the sun, called the solar wind, interacts with the surrounding interstellar medium (ISM). Where the outflow first encounters the ISM, it forms a shockwave called the termination shock--the boundary that Voyager 2 just crossed. It is now in the intermediate zone, called the heliosheath, where the two regions interact. Within the next few years, it will cross another boundary, called the heliopause, where the sun's influence ends. More: MIT instrument finds surprises at solar system's edge Video animation / John Belcher and Mark Bessette, MIT Full Story - http://web.mit.edu/newsoffice/2007/voyager-1210.html Original posting on MIT TechTV - http://techtv.mit.edu/file/449/



  5. Propagation of Magnetized Neutron Stars Through the Interstellar Medium

  6. 19 Aug 2007 at 9:05am



    5 sec - Aug 19, 2007

    streamlines are shown. The background represents the density. [ avi, approx. 4.6 MBt) <br> Central region of simulations



  7. Solar system in Milky way

  8. 5 Jun 2006 at 1:28am



    21 sec - Jun 5, 2006

    Starting with a view of our Milky Way galaxy, the orange gas in the animation represents the interstellar medium. The bow shock is created because the heliosphere is moving through like a boat through the water, crashing through the interstellar gases. The bow shock in front of the moving heliosphere is similar to the one observed by the Hubble Space Telescope. Click for animation. Credit: NASA/Walt Feimer



  9. NIBIRU,.April 2008 Breaking News & 2012 ASCENSION.pt1/2...

  10. 27 Apr 2008 at 10:18am



    8 min - Apr 27, 2008

    Latest Sighting of Nibiru,.AKA,.PlanetX Also News about possible 2012 Rapture of Ascension... Gamma-Ray Emissions,.The Offical Report States,.. Physicists find evidence for highest energy photons ever detected from Milky Way's equator Physicists at nearly a dozen research institutions, including New York University, have discovered evidence for very high energy gamma rays emitting from the Milky Way, marking the highest energies ever detected from the galactic equator. Their findings, published in the Dec. 16 issue of the Physical Review of Letters, were obtained using the Milagro Gamma Ray Observatory, a new detector located near Los Alamos, N.M., that allows monitoring of the northern sky on a 24-hour, 7-day-per-week basis. Gamma rays are considered by scientists to be the best probe of cosmic rays outside the solar neighborhood. The research team, which includes nearly 40 physicists, reported that Milagro, positioned at an altitude of 8600 feet in the Jemez Mountains, detected a signal along the galactic equator region and interpreted it as arising from gamma rays with a median energy of 3.5 trillion electron-volts, or 3500 times the mass-energy of a proton. Previous satellite experiments have seen gamma-ray emissions along the galactic equator reaching up to energies of only 30 billion electron-volts. These emissions are understood to be produced by interactions of cosmic-ray particles with the abundant interstellar medium near the galactic equator. Previously, some researchers had speculated that additional mechanisms were needed to explain the large number of particles observed at high energies. However, the measurements by Milagro can be understood by assuming a cosmic ray energy spectrum near the galactic center similar to that in the solar system and the standard properties of particle interactions. The results presented in the Physical Review of Letters paper were gathered over a three-year period, beginning in July 2000. New York University



  11. IBEX | What are the Boundaries of our Solar System?

  12. 1 Aug 2008 at 1:22pm



    3 min - Aug 1, 2008

    For more info: http://www.nasa.gov/ibex IBEX is a new NASA mission that will study the interaction between the solar wind and the material beyond our Solar System called the interstellar medium. The solar wind flowing out of the sun inflates a bubble that we call the heliosphere. IBEX's job is to study those boundaries and understand how they really work and tell us how the heliosphere is able to do the important job of protecting us here on Earth as well as astronauts in space from the dangerous galactic cosmic rays.



  13. NASA | IBEX: Exploring The Edge Of Our Solar System

  14. 6 Jun 2008 at 11:58am



    3 min - Jun 6, 2008

    For more information: http://www.nasa.gov/ibex IBEX is a new NASA mission that will study the interaction between the solar wind and the material beyond our solar system called the interstellar medium. The solar wind flowing out from the sun inflates a bubble that we call the heliosphere. IBEX's job is to study those boundaries and understand how they really work and tell us how the heliosphere is able to do the important job of protecting us from the dangerous galactic cosmic rays.



  15. NASA - IBEX: Exploring The Edge Of Our Solar System

  16. 12 Jun 2008 at 12:38am



    Unknown length - Jun 12, 2008

    IBEX is a new NASA mission that will study the interaction between the solar wind and the material beyond our solar system called the interstellar medium. The solar wind flowing out from the sun inflates a bubble that we call the heliosphere. IBEX's job is to study those boundaries and understand how they really work and tell us how the heliosphere is able to do the important job of protecting us from the dangerous galactic cosmic rays.



  17. NASA | IBEX | What are the Boundaries of our Solar System?

  18. 1 Aug 2008 at 1:33pm



    3 min - Aug 1, 2008

    For more info: http://www.nasa.gov/ibex IBEX is a new NASA mission that will study the interaction between the solar wind and the material beyond our Solar System called the interstellar medium. The solar wind flowing out of the sun inflates a bubble that we call the heliosphere. IBEX's job is to study those boundaries and understand how they really work and tell us how the heliosphere is able to do the important job of protecting us here on Earth as well as astronauts in space from the dangerous galactic cosmic rays.



  19. MHD simulations of spherical accretion to a star in the propeller regime


  20. 22 sec

    Interaction of a magnetar rotating in the propeller regime with the interstellar medium at Mach number



  21. Exploring Physics Across the Universe

  22. 11 Aug 2008 at 7:03pm



    4 min - Aug 11, 2008

    The Cosmic Origins Spectrograph (COS) is a new instrument developed for the Hubble Space Telescope planned for installation during the next shuttle mission to the Hubble (SM4) in 2008. It is designed for high throughput, medium resolution (R=20,000) spectroscopy of point sources, allowing the efficient observation of numerous faint extragalactic and galactic ultraviolet (1150-3000 A) targets. The primary science objectives of the mission are the study of the origins of large-scale structure in the universe, the formation and evolution of galaxies, and the origin of stellar and planetary systems and the cold interstellar medium. The instrument has been designed with maximum effective area as the primary constraint, and will provide more than an order of magnitude gain in sensitivity over previous HST instruments in this wavelength region.



  23. Kaboom

  24. 4 Apr 2008 at 5:01pm



    3 min - Apr 4, 2008

    Fun song about exploding stars - how heavy elements seed the galaxy. Lyrics are posted here. Read on... Kaboom © David Bigelow and Peter Jedicke The stars go nova one by one KABOOM, KABOOM. Nucleosynthesis is done KABOOM, KABOOM The supernovas dissipate what fusion energy helped create And the stars go nova in the galaxy The heavy elements are born KABOOM, KABOOM And from their stellar cores are torn KABOOM, KABOOM Shells of gas are strewn through space, distributing matter all over the place And the stars go nova in the galaxy. As years go by the remnants spread KABOOM, KABOOM But the universe is far from dead KABOOM, KABOOM To eliminate the tedium of the interstellar medium come the molecules that make up you and me.



  25. VøKaB - Suitable Breaks - ?oKåß?0??¶S¶ON Mix II

  26. 30 Mar 2008 at 6:06pm



    4 min - Mar 30, 2008

    Science Goals The prime objective of ACE is to measure and compare the composition of several samples of matter, including the solar corona, the solar wind, and other interplanetary particle populations, the local interstellar medium (ISM), and galactic matter. While there has been great progress addressing these objectives, the changing conditions over the solar cycle present new opportunities. In addition, new observations and theoretical advances, new missions, and the evolving goals of NASA and the Sun-Solar- System Connection (S3C) Theme have introduced new challenges, including the goal of achieving the scientific understanding needed to forecast space weather in the coming years when humans will venture beyond Earths protective magnetosphere. The nine scientific instruments on ACE are performing: Comprehensive and coordinated composition determinations Elemental Isotopic Ionic charge state Observations spanning broad dynamic range Solar wind to galactic cosmic ray energies (~100 eV/nucleon to ~500 MeV/nucleon) Hydrogen to Zinc (Z = 1 to 30) Solar active and solar quiet periods Investigations of the origin and evolution of solar and galactic matter Elemental and isotopic composition of matter Origin of the elements and subsequent evolutionary processing o Formation of the solar corona and acceleration of the solar wind Particle acceleration and transport in nature Mission Status Last update: February, 2007 ACE has been at the L1 point for almost 10 years, and the spacecraft and instruments are still working very well, with the exception of the SEPICA instrument. Due to failure of the valves that control gas flow through the instrument, active control of the SEPICA proportional counter is no longer possible. At this time, we do not expect to deliver any SEPICA data beyond Feb 4 2005, unless one of the valves opens by itself, as has happened a few times in the past. A fuel use strategy has been implemented that will allow continued operations through the year 2022 ?oKåß?0??¶S¶ON...The Best Home ?oKåß?U?Lization & Use of the amazing and wonderful ALL NEW ?oKåß?U?Tron. Made In England - Under Strict Laboratory Conditions. (Deep Cleaned Using ?oKåß?U?Ology Products & Services) www.myspace.com/VKaB



  27. Supernovas

  28. 23 Oct 2007 at 10:39pm



    2 min - Oct 24, 2007

    a lyrics write about supernovas Remnants of an exploding star. Making up new creations like Earth and Mars. Replenishing the universe, goes to show ya. There would be no life without supernovas. Aglow brightly shining it's light. Surrounded by the dark of the everlasting night. Particles flying all about. To be recycled once more there is no doubt. Every new explosion sets a new cycle of life in motion. Remnants of an exploding star. Making up new creations like Earth and Mars. Replenishing the universe, goes to show ya. There would be no life without supernovas. Particles going back to the interstellar medium. Changing life like the seasons. Raw materials in the molecular clouds. Star formation, one of the most amazing things around. Every new explosion sets a new cycle of life in motion. Remnants of an exploding star. Making up new creations like Earth and Mars. Replenishing the universe, goes to show ya. There would be no life without supernovas. Evolving based on their mass. Ten billion years can seem to go by so fast. Spending the last of it's hydrogen fuel. Leaving interstellar remnants for later generations of stars to begin life anew. Every new explosion sets a new cycle of life in motion. Remnants of an exploding star. Making up new creations like Earth and Mars. Replenishing the universe, goes to show ya. There would be no life without supernovas. Every new explosion sets a new cycle of life in motion. Remnants of an exploding star. Making up new creations like Earth and Mars. Replenishing the universe, goes to show ya. There would be no life without supernovas. Just goes to show ya. There would be no life without supernovas.



  29. The heliosphere

  30. 13 May 2008 at 2:34pm



    35 sec - May 13, 2008

    The heliosphere is a bubble in space "blown" into the interstellar medium (the hydrogen and helium gas that permeates the galaxy) by the solar wind. Although electrically neutral atoms from interstellar space can penetrate this bubble, virtually all of the material in the heliosphere emanates from the Sun itself.



  31. primal glow

  32. 29 Apr 2008 at 8:42pm



    2 min - Apr 30, 2008

    extragalacticmicroquasar interstellar medium perlastron<
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