Ten previously discovered circumstellar debris systems, plus MP Mus (a mature protoplanetary disk of age comparable to the youngest of the debris disks), were studied.
Hubble's sharp view uncovers an unexpected diversity and complexity in the structures. The disk-like structures are vast, many times larger than the planetary distribution in our solar system.
Some disks are tilted edge-on to our view, others nearly face-on.
Asymmetries and warping in the disks might be caused by the host star's passage though interstellar space.
Alternatively, the disks may be affected by the action of unseen planets. In particular, the asymmetry in HD 181327 looks like a spray of material that is very distant from its host star.
It might be the aftermath of a collision between two small bodies, suggesting that the unseen planetary system may be chaotic.
The stars surveyed may be as young as 10 million years old and as mature as more than 1 billion years old.
The visible-light survey was done with the Space Telescope Imaging Spectrograph (STIS).
The STIS coronagraph blocks out the light from the host star so that the very faint reflected light from the dust structures can be seen.
The images have been artificially coloured to enhance detail.
Credit: NASA, ESA, G. Schneider (University of Arizona), and the HST/GO 12228 Team
Astronomers using NASA's Hubble Space Telescope have completed the largest and most sensitive visible-light imaging survey of dusty debris disks around other stars.
These dusty disks, likely created by collisions between leftover objects from planet formation, were imaged around stars as young as 10 million years old and as mature as more than 1 billion years old.
The survey's results appeared in the Oct. 1, 2014, issue of The Astronomical Journal.
Once thought to be simply pancake-like structures, the unexpected diversity and complexity of these dusty debris structures strongly suggest they are being gravitationally affected by unseen planets orbiting the star.
Alternatively, these effects could result from the stars' passing through interstellar space.
The researchers discovered that no two "disks" of material surrounding stars look the same. "We find that the systems are not simply flat with uniform surfaces," Schneider said.
"These are actually pretty complicated three-dimensional debris systems, often with embedded smaller structures. Some of the substructures could be signposts of unseen planets."
The astronomers used Hubble's Space Telescope Imaging Spectrograph (STIS) to study 10 previously discovered circumstellar debris systems, plus MP Mus, a mature protoplanetary disk of age comparable to the youngest of the debris disks.
Irregularities observed in one ring-like system in particular, around a star called HD 181327, resemble the ejection of a huge spray of debris into the outer part of the system from the recent collision of two bodies.
"Catastrophically destroying an object that massive at such a large distance is difficult to explain, and it should be very rare."
"If we are in fact seeing the recent aftermath of a massive collision, the unseen planetary system may be quite chaotic."
Another interpretation for the irregularities is that the disk has been mysteriously warped by the star's passage through interstellar space, directly interacting with unseen interstellar material. "Either way, the answer is exciting," Schneider said.
"Our team is currently analyzing follow-up observations that will help reveal the true cause of the irregularity."
More information: "Probing for Exoplanets Hiding in Dusty Debris Disks: Disk Imaging, Characterization, and Exploration with HST/STIS Multi-Roll Coronagraphy," Glenn Schneider et al., 2014, Astronomical Journal, Vol. 148, No. 4, Art. 59 dx.doi.org/10.1088/0004-6256/148/4/59 , On Arxiv: arxiv.org/abs/1406.7303
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