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First Cosmological Results From MAP

riptalon writes "The Wilkinson Microwave Anisotropy Probe, a NASA Explorer mission has announced the first results based on a year of observations from the L2 Lagrangian point. MAP carries two back-to-back microwave telescopes to study variations in the cosmic microwave background, to much greater accuracy than the COBE satellite. The excruciating details of the results on the age, geometry and composition of the universe can be found in this paper. Executive summary: 13.7 billion years old, flat, 4.4% baryons, 22% dark matter and 73% dark energy."

24 of 291 comments (clear)

  1. courtesy of Wikipedia by goatasaur · · Score: 4, Informative

    Baryons

    Dark Energy

    Dark Matter

    Hope this helps you out a little. :)

    --
    ~D:
    1. Re:courtesy of Wikipedia by jaoswald · · Score: 5, Informative

      In this case "vacuum" is physicists' name for "empty space," meaning "as empty as possible." On earth, "empty" means "much less matter than in the atmosphere."

      When that empty space is surrounded by the earth's atmosphere, the atmosphere presses on the container that encloses the empty space. Open a hole in the container, and the atmosphere rushes in---that's the sucking part. (Indirectly, it is Earth's gravity that creates the pressure, but you could also imagine the Earth is in a big closed box.)

      Intergalactic space is presumably much emptier than any vacuum that we can achieve on earth. When the "empty space" in question is simply surrounded by more empty space, there isn't any sucking of matter. (Pressure is practically zero.)

      It turns out that space itself can contain energy; that is, "empty" is not the same as "nothing." General relativity predicts that there is energy in the curvature of space, which is roughly equivalent to the energy in Newton's gravitational fields. (Not exactly equivalent for strong fields, however.) Also, quantum mechanically, there is always the possibility of a particle or field being present in the empty space. That possibility provides a "zero-point" energy, even when the matter or fields are not there. If we really knew all the possible particles and fields, we could calculate what this would be. There might be particles and fields that we haven't discovered yet, or other additions to quantum mechanics that we haven't discovered yet, which is why we have to look to astronomers to determine the properties of empty space.

      The energy in otherwise empty space is the dark energy. That energy can cause dynamic behavior in the framework of space, causing it to expand and contract.

  2. Re:0.6% regular stuff by mph · · Score: 2, Informative
    So only 0.6% of the universe is the "normal" matter and energy that we observe and of which we are composed?
    I don't know about you, but I'm mostly made of baryons.
  3. More information by Anonymous Coward · · Score: 5, Informative

    More information can be found at (including a cosmology tutorial):

    http://www.astro.ucla.edu/~wright/cosmolog.htm#New s

    This press release was mentioned in a post in the previous slashdot story yesterday.

  4. Other links by riptalon · · Score: 5, Informative

    Mass media coverage can be found at CNN and the BBC. A list of all the MAP papers can be found here.

  5. Re:huh? by JoeBuck · · Score: 5, Informative

    A baryon is a particle such as a neutron or proton. It's one of the two main classes of ordinary matter particles, the other is the lepton (e.g. an electron or neutrino). Baryons "feel" the strong nuclear force, leptons do not.

    Dark matter refers to exotic forms of matter that are "ordinary" from a gravitational point of view, that isn't made up of baryons or leptons. This stuff either interacts weakly with ordinary matter, or doesn't interact at all (other than via gravity).

    Dark energy has positive energy but negative pressure, so it causes a gravitational repulsion. Einstein's "cosmological constant" one possible example of dark energy. It can be thought of as a property of space.

  6. Re:0.6% regular stuff by DeepBlueDiver · · Score: 2, Informative
    So only 0.6% of the universe is the "normal" matter and energy that we observe and of which we are composed?

    The 4.4% baryons are the "normal" matter.
  7. Dark Energy/Dark Matter/Negative Energy by monk · · Score: 5, Informative

    Confused by "Dark Energy," "Vacuum Energy," "Dark Matter," and "Exotic Matter?" Here's a great collection of papers. (Mostly from the SNAP project)

    --
    [-- Trust the Monkey --]
  8. Re:0.6% regular stuff by mph · · Score: 2, Informative
    Remaining 0.6% probably antimatter but not 100% sure. Correct me if I'm wrong...
    You're wrong. Antimatter is baryonic (well, at least to the same extent that normal matter is; some of it is leptons, but very little by mass).

    I suspect that all of the percentages given have been rounded to two significant figures, and that you folks shouldn't be concluding that 0.4% has been unspecified.

    There are contributions to Omega from electrons and neutrinos, for example, but this is a tiny amount compared even to the 4.4% from baryons.

  9. Re:huh? by (void*) · · Score: 4, Informative

    In astronomy, "baryons" can also include "leptons", simply because leptons are included in the mass that one measures using a galaxy rotation curve.

  10. Re:Expansion rate? by riptalon · · Score: 3, Informative

    Mpc = Mega parsecs, i.e. millions of parsecs, where parsec stands for parallax arcsecond and equals about 3.26 light years.

  11. Answers here, dammit. by Decimal · · Score: 3, Informative

    Does Dark Energy suck or blow?

    Blow... sort of. It acts the opposite of gravity, pushing everything apart.

    http://www.lbl.gov/Science-Articles/Archive/dark-e nergy.html

    --

    Remember "Bring 'em on"? *sigh
  12. Re:Expansion rate? by Gruturo · · Score: 2, Informative

    What does the Mpc stand for?

    Megaparsec (a parsec is 3.26 light years, or 3.08*10^16 meters).

    Basically, it means that an object 1 megaparsec away from you is moving away by 71km/second (since the whole universe is expanding like a 4-dimensional balloon, all points are moving away from all other points, and this speed increases with their relative distances)

    --

    Vacuum cleaners suck. Kings rule.
  13. Nothing of the sort by rufusdufus · · Score: 2, Informative

    Time has not been proven to continue into infinity. Go read 'A Brief History of Time' for a good laymens introduction to cosmology.

    Space and time are concepts deeply intertwined with energy and matter; they is not distinct from them. Thus, there is no 'before' the universe began, there is no time there, there is no there there either.

  14. Re:Why is the probe at the L2 point? by anubi · · Score: 2, Informative
    Try Eddington's Site .

    But, given this, let me add a little nota bene...

    I found this by opening up a window to Google and typing the words +"L2" +"orbit" +"space". For me, it was the first entry returned.

    "Give a man a fish and you have fed him for a day, but *teach* a man to fish and you have fed him forever". That is what makes sharing the 'tricks of the trade' so special.

    --
    "Prove all things; hold fast that which is good." [KJV: I Thessalonians 5:21]

  15. Re:Why is the probe at the L2 point? by djcinsb · · Score: 5, Informative

    L2 is nice for several reasons. The instrument on MAP needs to be kept cold. Sitting at L2, the spacecraft can keep the instrument pointing away from the Sun, and still measuring data, without ever needing to worry about interference from the Earth or Moon, and there is this nice big dish (the solar array) shielding the instrumentation from direct sunlight. In addition, NASA has lots of experience with spacecraft at the collinear Lagrange points (L1 and L2), so the orbits and communications are very well understood there. And L2 is far enough away from the Earth-Moon system to avoid complicated orbit perturbations, but close enough for relatively easy communications (that is, the radio doesn't have to be too big).

    Hope that helps!

    --
    A signature always reveals a man's character - and sometimes even his name. -- Evan Esar
  16. Re:How can you see so close to the big bang? by Anonymous Coward · · Score: 1, Informative
    There is no "universal point of origin". The Big Bang was not a concentrated lump of stuff somewhere out in the middle of empty space, which subsequently exploded (with a spherical wavefront marking the "outer edge of the explosion"). Rather, all of space was compressed into a point, and space expanded (instead of matter exploding), like the surface of an inflating balloon. Think of an ants crawling randomly all over across the surface of such a balloon. At any given time, ants which were crawling on the surface when the balloon was small are still crawling past any given point --- that's like why we still see photons.



    This FAQ may help.

  17. Umm.... by Anonymous Coward · · Score: 2, Informative

    Do you have any idea about how NASA really operates?

    NASA's budget and operations are firmly divided into unmanned and manned areas. Almost none of the unmanned science missions are launched by the Shuttle fleet... most are launched on corporate expendable launch vehicles.

    Science in NASA is almost totally disengaged from launch vehicle & station planning & operations. This is a problem, not a cure.

  18. Re:huh? by Peter+T+Ermit · · Score: 3, Informative
    First, he said baryons, not baryonic matter -- you will never hear any astronomer call a lepton a baryon.

    Second, technically, even in astronomy, baryonic matter is only the nuclei -- the leptons are counted separately, though they're unimportant masswise, as you mentioned. Here's why.

    There are several ways of computing the amount of and types of matter in the universe. One of the most important is examining primordial gas clouds and looking at the relative abundances of hydrogen, helium, and lithium and their various isotopes. This tells us about the era of nucleosynthesis -- the time 3 seconds to 3 minutes after the big bang when the temperature and pressure of the universe was enough to induce nuclear fusion. After 3 minutes, this process ended and froze the ratios of primordial elements.

    By looking at those ratios, scientists could figure out the abundance of those nuclei -- the nuclei, not the leptons, which don't affect the ratios at all. From this, they can figure out the density of nuclear matter in the universe, which is related to a quantity known as omega sub b. This number is thought to be about 4.5% from measurements of the elements in those gas clouds -- and MAP confirmed this by a different method. But this baryonic fraction does not have anything to do with the leptonic component of matter... including electrons and neutrinos.

    So, when astronomers say that they have shown that 4.4% of the universe is made up of baryonic matter, they really mean baryons. It just so happens that there are pesky leptons hanging around the baryonic matter, too.

  19. Re:Universe Flat? Please explain... by Bruce+Losis · · Score: 2, Informative

    Flatness/curvedness refers to whether parallel lines meet and by extension what sum of angles there are in a polygon:

    In a flat space (or plane as an example of a 2D space) angles in a triangle sum to 180 degree, always. Parallel lines never meet. This is a falt desk in 2D.

    In positively curved space (or plane) internal angles of a triangle sum to >= 180 degrees (sum approaches 180 as size of triangle side lengths approach 0). Parallel lines cross twice. This is the surface of a globe.

    In negatively curved space (or plane) internal angles of a triangle sum to <= 180 degrees (again sum approaches 180 as size approaches 0). Parallel lines diverge. This is a saddle.

    It's easy to see the way this are if you think of the space as a 2D object since the curvature requires (to visualise) an extra dimension, but the principles are the same in higher dimensionalities

    --
    Don't believe the nonsense, unless you hear it from me directly.
  20. Re:huh? by efuseekay · · Score: 4, Informative

    nope.

    Astronomy/astophysics pays my bills, and I can tell you that 4.4% of baryons from WMAP really means anything that is known in particle physics as quarks, leptons, blah blah blah.

    A rule of thumb is that 'baryons' in astronomy/astrophysics is anything that is in the standard model (sans the higgs.)But that's not the whole story.

    "baryons" (in the 4.4% of WMAP) is classified as matter that is not "dark". "Non-dark" means it interacts with other stuff and itself beyond just pure gravitation. That includes "radiation", which is stuff that behaves relativistically, and include things like photons, neutrinos,a nd perhaps other relics.

    To summarize, there is no difference between "baryons" and "baryonic matter" in astronomy.

    I will not call a lepton a baryon, but I will definetely lump leptons in when I say 4.4% of ther universe is made out of baryons. it's just a matter of context, and people in the field will udnerstand that.

    Really, astrophysicists are sloppy when it comes to naming stuff. So you have to be careful not to read too much into nomenclature like this, even in the era of "precision cosmology".

    --
    Mode (3) smart-aleck mode. Press * to return to main menu.
  21. Re:Expansion rate? by efuseekay · · Score: 2, Informative

    The further away the object is from us, the greater the velocity it seems to be expanding away from us. So H=71km/s /Mpc means that for every Mpc the objet is away from us, it is flying away from us at the velocity of 71 km/s.

    --
    Mode (3) smart-aleck mode. Press * to return to main menu.
  22. Re:Universe Flat? Please explain... by murky.waters · · Score: 2, Informative

    A way to visualize what flat (and open & closed) mean is to think of a plot of how two dimensions are shaped at very large distances. That is, if you had some ordinary (flat, straight lines are straight lines) reference and observed the path of a bunch of photons sent of at right angles (only two directions) to form a grid and plot that in 3D. Then if there is no curvature (=flat), you'll get a plot that looks like a sheet of paper or the surface of a desk. If the universe was curved (open or closed) then you'll get a hyperpolic saddle or sphere respectively.

    In short, flat means space like we ordinary envision it; it has absolutely nothing to do with the whole universe only expanding in 2 dimensions (like flat earth vs. round) as some of the earlier posters seem to think.

    Mathematically, flat is the most unlikely result since even the slightest deviation would translate into one of the other two states. Physically, it means that the universe's geometry is euclidean, that its volume is infinite, and that it expands FOREVER (yes sure, the expansion rate approaches zero, but you know how asymptotes are supposed to work).

    Incidentally, it means that we won't be able to eat at Milliway's. Shit.

    --
    Imagine the Creator as a stand up commedian - and at once the world becomes explicable. -Mencken
  23. Re:speed of light constant? by Mr.+Slippery · · Score: 2, Informative
    If the speed of light is constant, then why does it vary as it goes through different things? For example: when light goes through glass, it slows through the glass then speeds back up again.

    You're correct. What's constant for all observers is the speed of light in a vacuum.

    --
    Tom Swiss | the infamous tms | my blog
    You cannot wash away blood with blood