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Largest Ever Digital Survey of the Milky Way Released

Several readers have written to tell us that an international team of over fifty astronomers from around the globe have created the largest ever digital survey of the Milky Way. IPHAS (INT/WFC Photometric H-alpha Survey of the Northern Galactic Plane) is an image survey designed to show large-scale structure within our galaxy. IPHAS data is being released by utilizing technology from the UK government funded open source project Astrogrid. Some of the images are quite spectacular.

2 of 75 comments (clear)

  1. Why do some so love staring into space? by TheLazySci-FiAuthor · · Score: 4, Interesting

    I am always amazed at the large-scale structures of the universe. Especially the way that these structures are almost always analogous to physical phenomenon on earth (perhaps no surprise or coincidence if you adhere to the anthropic principle ;)

    I was showing my wife the computer-generated 3D maps of the uneven, filamentous distribution of galaxies in the known universe and she commented on how it reminded her of the fingers and tendrils of water being thrown from a bucket - but thrown out in all directions. I suddenly saw gravity as a sort of surface tension, trying to bring everything back together into a nice, neutral sphere. I also suddenly saw the dark energy as the momentum of the thrower and the dark energy as the buffeted air through which the splash disperses.

    It's amazing how an analogy can take something so intangiable and make it immediately accessable. I feel, however, that sometimes a simple analogy can have a negative effect as well.

    Without a true appreciation of the reality of astronomical images, comparisons to clouds and swirling water can diminish the wonder.

    For me, in this image I see a stunning display of incomprehensible size and volume. I see the very heart and soul of our universe laid bare; the very stuff from which everything is made - amazing!

    But for someone more lay in the ways of science and astronomy (and less enthused) this simply looks like a puff of smoke.

    How is it that some of us wonder and wander and some of us do not?

  2. Re:My God! by Jugalator · · Score: 2, Interesting
    You're joking, but dyson spheres have actually crossed the mind of astronomers.
    None found yet however. :-)

    According to Wikipedia:

    Given the amount of energy available per square meter at a distance of 1 AU from the Sun, it is possible to calculate that most known substances would be re-radiating energy in the infrared part of the electromagnetic spectrum. Thus, a Dyson Sphere, constructed by life forms not dissimilar to humans, who dwelled in proximity to a Sun like star, made with materials similar to those available to humans, would most likely cause an increase in the amount of infrared radiation in the star system's emitted spectrum. Hence, Dyson selected the title "Search for Artificial Stellar Sources of Infrared Radiation" for his published paper.

    SETI has adopted these assumptions in their search, looking for such "infrared heavy" spectra from solar analogs. As of 2005 Fermilab has an ongoing survey for such spectra by analyzing data from the Infrared Astronomical Satellite (IRAS). And from the SETI Institute:

    DATE: 1980
    OBSERVER(S): WITTEBORN
    SITE: NASA - U OF A, MT. LEMMON
    INSTR. SIZE (M): 1.5
    SEARCH FREQ.(MHz): 8.5 microns - 13.5 microns
    FREQUENCY RESOL.(Hz): 1 micron
    OBJECTS: 20 STARS
    FLUX LIMITS (W/m**2): N MAGNITUDE EXCESS < 1.7
    TOTAL HOURS: 50
    REFERENCE:
    COMMENTS: Search for IR excess due to Dyson spheres around solar
    type stars. Target stars were
    chosen because too faint for spectral type.
     
    DATE: 1984
    OBSERVER(S): SLYSH
    SITE: SATELLITE
    INSTR. SIZE (M): RADIOMETER
    SEARCH FREQ.(MHz): 37x10**3
    FREQUENCY RESOL.(Hz): 4x10**8
    OBJECTS: ALL SKY 3K BB
    FLUX LIMITS (W/m**2): T/T =< .01
    TOTAL HOURS: 6000
    REFERENCE: 27
    COMMENTS: Lack of fluctuations in 3K background radiation on
    angular scales of 10**-2 Strd. rules
    out optically thick Dyson spheres radiating more than 1 solar
    luminosity within 100 pc.
     
    DATE: 1987
    OBSERVER(S): TARTER, KARDASHEV & SLYSH
    SITE: VLA
    INSTR. SIZE (M): 26 (9 ANTENNAS)
    SEARCH FREQ.(MHz): 1612.231
    FREQUENCY RESOL.(Hz): 6105
    OBJECTS: G357.3-1.3
    FLUX LIMITS (W/m**2):
    TOTAL HOURS: 1
    REFERENCE:
    COMMENTS: Remote observation (by VLA staff) of IRAS source near
    galactic center to determine if
    source could be nearby Dyson sphere. Source confirmed as OH/IR
    star.
    --
    Beware: In C++, your friends can see your privates!