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Archaeology in the universe - 0 views

started by Sandra Flores on 30 Oct 14 no follow-up yet
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Why Are Quark Stars So Strange? : Discovery News - 1 views

  • First things first, neutron stars, quark stars and black holes are all born via the same mechanism: a supernova. But each of the three are progressively more massive, so they originate from supernovae produced by progressively more massive stars. So, what if a star exploded, producing something a little too massive to be called a neutron star? Well, neutron stars resist collapsing under their own gravitational pull by a characteristic of matter known as neutron degeneracy. This produces an outward force called neutron degeneracy pressure. What if the neutron star born after a supernova is too massive for this neutron degeneracy pressure to hold up against the neutron star's own gravity? In this case, it's up to the quarks that make up the neutrons to take over, preventing the body from collapsing any further. Single neutrons are composed of three quarks (two "down" quarks and one "up" quark). When quark degeneracy pressure kicks in, a quark star may be produced; the free "up" and "down" quarks get converted into "strange" quarks. Therefore, a quark star (also known as a "strange star") is made up of strange matter.
  • Using what we know from the Standard Model of particle physics, a massive quark star may have enough gravitational energy to start 'burning' strange matter. The quarks inside the core of the quark star may be abused so badly by gravitational pressure that the quarks will be converted into pure energy and neutrinos.
  • The fascinating thing with this scenario is that the quark star matter will be so dense that even the neutrinos cannot escape. However, this release of energy and generation of neutrinos creates an outward pressure countering the relentless inward gravitational pull.
  • ...2 more annotations...
  • Dai calls this extreme strange matter-burning quark star an "electroweak star"
  • Saving the best till last, the electroweak star's core would therefore be as extreme as the universe was only 10-10 seconds (that's 0.0000000001 seconds) after the Big Bang. These extreme objects would be like mini-Big Bang laboratories, maintaining a pressure where the electromagnetic and weak forces are so intertwined, they cannot be distinguished.

Star Formation - 0 views

started by Sandra Flores on 02 Nov 14 no follow-up yet
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Chrome Experiments - "100,000 Stars" by Google Data Arts Team - 3 views

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    100,000 Stars is an interactive visualization of the stellar neighborhood created for the Google Chrome web browser. It shows the real location of over 100,000 nearby stars. Zooming in reveals 87 major named stars and our solar system. The galaxy view is an artist's rendition.

Strange stars on the heel - 0 views

started by Sandra Flores on 05 Jan 15 no follow-up yet

Strange stars on the heel - 0 views

started by Sandra Flores on 09 Jan 15 no follow-up yet

REGULUS BINARY STAR SYSTEM - 1 views

started by Learn Astronomy on 20 Jan 21 no follow-up yet

Revealing pattern without planets - 0 views

started by Sandra Flores on 05 Jan 15 no follow-up yet
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Welcome to the NASA Star and Exoplanet Database - 1 views

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    he NASA Star and Exoplanet Database (NStED) collects and serves public data to support the search for and characterization of extra-solar planets (exoplanets) and their host stars. The data include published light curves, images, spectra and parameters, and time-series data from surveys that aim to discover transiting exoplanets. All data are validated by the NStED science staff and traced to their sources. NStED is the U.S. data portal for the CoRoT mission.

How big are neutron stars? - 0 views

started by Sandra Flores on 05 Jan 15 no follow-up yet

Planetary Nebulae - 0 views

started by Sandra Flores on 05 Jan 15 no follow-up yet

How big are neutron stars? - 0 views

started by Sandra Flores on 09 Jan 15 no follow-up yet

Planetary Nebulae - 0 views

started by Sandra Flores on 09 Jan 15 no follow-up yet
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Star Shadows Remote Observatory Home Page - 1 views

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    Located at New Mexico Skies and CTIO, Star Shadows Remote Observatory (SSRO) is a cooperative astro-imaging venture operated by Lewis Garrett, Jacob Gerritsen, Rick Gilbert,  Jack Harvey, Steve Mazlin, Michael Smith, Teri Smoot, and Daniel Verschatse.
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Astronomers Crowdsource the Definition of a Galaxy - Technology Review - 2 views

  • So what to do? Today, Duncan Forbes at Swinburne University in Australia and Pavel Kroup at the University of Bonn in Germany put forward a novel solution. They outline the various characteristics that astronomers think about when classifying galaxies. These include factors such as the presence of stars, so gas clouds can't be defined as galaxies; being gravitationally bound, so materials that has been stripped away by another galaxy wouldn't count; whether the system is stable or not; whether it hosts a good variety of different types of star, which excludes globular clusters which contain only similar stars; and whether it is held together by dark matter, which many galaxies seem to be. There are other factors too, of course. (Although they do not include the presence of a black hole at the centre of a galaxy as a defining characteristic , which is odd given the growing interest in the link between galactic evolutoin and black holes.) Forbes and Kroup go on to suggest that the best way to achieve consensus is to crowdsource the problem. In other works, they want to use the wisdom of the crowd to determine what factors are important what aren't.
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