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Chi Cygni expands and dims, and then contracts and brightens over 408 days

SpaceRef Reps SpaceRef Reps·265 videos
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Uploaded on Dec 15, 2009

This movie combines infrared images of the surface of Chi Cygni, obtained with IOTA, with visual brightness measurements provided by the American Association of Variable Star Observers (AAVSO). Chi Cygni demonstrates a 408-day-period of expanding and dimming, followed by contracting and brightening. Credit: Sylvestre Lacour, Observatoire de Paris

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Top Comments

  • bsm117532

    It works, bitches.

    · 13

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    in reply to bigdonthedj (Show the comment)
  • bigdonthedj

    Science!

    · 9

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All Comments (41)

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  • aaa821999

    Question is this normal for it to dim and contract like this cuz it looks like its going red giant and then back to normal size is it normal .Also what does infrared detect

    ·

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  • CookieMonzta1995

    How come at night I can see bright non-moving objects in the sky which pulsate and change colors? I know they are not aviation vehicles as they are in the same place each time I go to bed.

    ·

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  • 1787dude

    its having moodswings XDDDDD

    ·

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  • Geminii27

    Great, some Ascended species is using it as a doof-doof speaker.

    ·

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  • webhead84

    with the generally accepted fact of the big bang it means that fundamentally that no matter where your origins are in this universe , we're all connected on the basic fundamental level of physics and since most life would have an energy basis we're all energy expressions of the universe @ hand and unique unto ourselves

    ·

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    in reply to hurricanefloyd1 (Show the comment)
  • webhead84

    i was thinking due to stellar closeness

    if the debris shed would pass near us

    even a weak wave would possibly cause some sorta effect ....but there are a lot of variables to take into account.

    ·

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    in reply to Hilariousity (Show the comment)
  • siderespector

    Chi Cygni is not very unique. It is however the Mira star with greatest brightness variation (amplitude), and the apparently brightest S-type star in the sky.

    ·

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    in reply to siderespector (Show the comment)
  • siderespector

    It's an S-type Mira variable. It's half way becoming a carbon star up on the unstable AGB-branch. It will end as a planetary nebula, not as a supernova. SN:s, type II, belong to the supergiant classes, I think lum classes Ia and Ib. This is a lum class III ordinary giant. When being an advanced AGB-branch carbon star, it will finally shed off its own atmosphere, which becomes a planetary nebula, while the core contracts and finally ends as a white dwarf.

    ·

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  • Michael Miller

    I'm very curious about that as well. Gravity should be a pretty universal contracting force, but a star at this stage might be hella unstable as well.

    ·

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    in reply to Christian Treber (Show the comment)
  • Michael Miller

    Nah, it probably happened right around the time Constantinople fell.

    ·

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    in reply to SARGAMESH (Show the comment)
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