Hubble Captures Birth, Annihilation of Young Solar Systems in Orion Nebula

Article written: 14 Dec , 2009
Updated: 24 Dec , 2015
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Looking deep inside the Orion Nebula, the Hubble Space Telescope has captured a stunning collection of protoplanetary disks – or proplyds – which are embryonic solar systems in the making. Using Hubble’s Advanced Camera for Surveys (ACS), researchers have discovered 42 protoplanetary blobs, which are being illuminated by a bright star cluster. These disks, which sometimes appear like boomerangs, arrows, or space jellyfish, surround baby stars and are shedding light on the mechanism behind planet formation.

One of 42 new proplyds discovered in the Orion Nebula, 181-825 is one of the bright proplyds that lies relatively close to the nebula’s brightest star, Theta 1 Orionis C. Resembling a tiny jellyfish, this proplyd is surrounded by a shock wave that is caused by stellar wind from the massive Theta 1 Orionis C interacting with gas in the nebula.  Credit: NASA/ESA and L. Ricci (ESO)

One of 42 new proplyds discovered in the Orion Nebula, 181-825 is one of the bright proplyds that lies relatively close to the nebula’s brightest star, Theta 1 Orionis C. It resembles a tiny jellyfish. Credit: NASA/ESA and L. Ricci (ESO)

As newborn stars emerge from the nebula’s mixture of gas and dust, proplyds form around them. The center of the spinning disc heats up and becomes a new star, but remnants around the outskirts of the disc attract other bits of dust and clump together. This is the beginning of a solar system.

But not all proplyds face a bright and happy future, even in these beautiful images.

Bright star that illuminates some of the proplyds is both a blessing and a curse. The disks that lie close to the brightest star in the cluster (Theta 1 Orionis C) are being zapped by the star’s powerful emissions. The radiation that lights them up and makes them visible also threatens their very existence. As the disk material begins to heat, it is very likely to dissipate and dissolve, destroying the potential for planets to form. Some of these proplyds will be torn apart; however others will survive and perhaps evolve into planetary systems.

One of 42 new proplyds discovered in the Orion Nebula, 321-602 is one of the dark proplyds that lies relatively far from the nebula’s brightest star, Theta 1 Orionis C.  Credit: NASA/ESA and L. Ricci (ESO)

One of 42 new proplyds discovered in the Orion Nebula, 321-602 is one of the dark proplyds that lies relatively far from the nebula’s brightest star, Theta 1 Orionis C. Credit: NASA/ESA and L. Ricci (ESO)

Discs that are farther away do not receive enough energetic radiation from the star to heat up the gas and so they can only be detected as dark silhouettes against the background of the bright nebula, as the dust that surrounds these discs absorbs background visible light. By studying these silhouetted discs, astronomers are better able to characterize the properties of the dust grains that are thought to bind together and possibly form planets like our own.

A montage of 30 proplyds in the Orion Nebula.  Credit: NASA/ESA and L. Ricci (ESO

A montage of 30 proplyds in the Orion Nebula. Credit: NASA/ESA and L. Ricci (ESO


The brighter discs are indicated by a glowing cusp in the excited material and facing the bright star, but which we see at a random orientation within the nebula, so some appear edge on, and others face on, for instance. Other interesting features enhance the look of these captivating objects, such as emerging jets of matter and shock waves.

It is rare to see proplyds in visible light, but the astronomers were able to use Hubble for this ambitious survey of the familiar and photogenic Orion Nebula.

Source: ESA

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5 Responses

  1. Lawrence B. Crowell says

    We always knew stars and solar systems were being formed there. Fascinating to see it this close.

    LC

  2. 2stepbay says

    The images from Hubble and other space devices over the past few weeks have astounded me. That we can see, appreciate and experience such wonder is truly a gift of a higher frequency.

  3. Dark Gnat says

    Amazing!

    Some of them have a sort of donut shape. I also wonder how radiation from other stars affects the clumping and eventual orbits of the future planets. That might help explain the wide variety of systems we’ve seen.

    I hope NASA re-images the Eagle Nebula. I’m sure theres some interesting stuff going on there as well.

  4. Torbjorn Larsson OM says

    Aahhhwesome, and illuminating [sic]!

    Isn’t it shocking what a supernovae can do (if such a one started to collapse this particular nebula cloud)? That is a high exchange rate of new stars for one dead. Since the Sun started in the same way Earth doesn’t seem quite as special anymore.

    And these proplyds look just like they “should”. Another aha moment.

  5. DrFlimmer says

    @ Torbjorn Larsson OM

    I disagree here. Earth is still unique, or in other words: it was really lucky! It was at the right time at the right spot, crashed with another body, barely survived, got a moon stabilizing it. The sun itself went away from its nursery before a nearby supernova could’ve destroyed the proto-planetary disk.
    And finally there was enough crap on earth to form life. Well, that is what I call lucky 😉 .

    Of course, there could be stars and planets in M42 with equaling luck, but the Orion nebula is really dense. Maybe too unstable?

    ———————————-

    Two planets meet:
    “Hey! How do you do?”
    “Oh, I feel terrible. I have homo sapiens!”
    “I know what you’re going through. But that will pass!”

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