If astronomers initially miss something in their review of data, they can make new discoveries by revisiting earlier data with new image-processing techniques, thanks to the wealth of information stored in the Hubble data archive. This is what Rémi Soummer of the Space Telescope Science Institute (STScI) in Baltimore and his team recently did while on a hunt for hidden Hubble treasures.
The stars in question initially were targeted with Hubble’s Near Infrared Camera and Multi-Object Spectrometer (NICMOS) based on unusual heat signatures obtained from NASA’s Spitzer Space Telescope and the Infrared Astronomical Satellite that flew in 1983. The previous data provided interesting clues that dusty disks could exist around these stars. Small dust particles in the disks might scatter light and therefore make the disks visible, but when Hubble first viewed the stars between 1999 and 2006, no disks were detected in the NICMOS pictures.
Recently, with improvements in image processing, including algorithms used for face-recognition software, Soummer and his team reanalyzed the archived images. This time, they could unequivocally see the debris disks and even determine their shapes.
The NICMOS instrument, which began collecting data in 1997, has been so cutting-edge that ground-based technology only now is beginning to match its power. Because Hubble has been in operation for almost 24 years, it provides a long baseline of high-quality archival observations.
“Now, with such new technologies in image processing, we can go back to the archive and conduct research more precisely than previously possible with NICMOS data,” said Dean Hines of STScI.
“These findings increase the number of debris disks seen in scattered light from 18 to 23. By significantly adding to the known population and by showing the variety of shapes in these new disks, Hubble can help astronomers learn more about how planetary systems form and evolve,” said Soummer.
The dust in the disks is hypothesized to be produced by collisions between small planetary bodies such as asteroids. The debris disks are composed of dust particles formed from these grinding collisions. The tiniest particles are constantly blown outward by radiation pressure from the star. This means they must be replenished continuously through more collisions. This game of bumper cars was common in the solar system 4.5 billion years ago. Earth’s Moon and the satellite system around Pluto are considered to be collisional byproducts.
“One star that is particularly interesting is HD 141943,” said Christine Chen, debris disk expert and team member from STScI. “It is an exact twin of our Sun during the epoch of terrestrial planet formation in our own solar system.”
Hubble found that the star exhibits an asymmetrical, edge-on disk. This asymmetry could be evidence that the disk is being gravitationally sculpted by the tug of one or more unseen planets.
“Being able to see these disks now also has let us plan further observations to study them in even more detail using other Hubble instruments and large telescopes on the ground,” said Marshall Perrin of STScI.
“We also are working to implement the same techniques as a standard processing method for NASA’s upcoming James Webb Space Telescope,” said Laurent Pueyo from STScI. “These disks will also be prime targets for the Webb telescope.”
Soummer’s team has just begun its work. They next will search for structures in the disks that suggest the presence of planets.
