Tonight's Sky
Sun
Sun
Moon
Moon
Mercury
Mercury
Venus
Venus
Mars
Mars
Jupiter
Jupiter
Saturn
Saturn

Tonight's Sky — Change location

OR

Searching...

Tonight's Sky — Select location

Tonight's Sky — Enter coordinates

° '
° '

Sharpest-ever ground-based images of Pluto and Charon

The data from Gemini North verified and refined previous orbital characteristics for the dwarf planet and its largest moon while revealing the pair’s precise diameters.
PlutoCharon
Speckle image reconstruction of Pluto and Charon obtained in visible light at 692 nanometers (red) with the Gemini North 8-meter telescope using the Differential Speckle Survey Instrument (DSSI). Resolution of the image is about 20 milliarcseconds rms (root mean square). This is the first speckle reconstructed image for Pluto and Charon from which astronomers obtained not only the separation and position angle for Charon, but also the diameters of the two bodies. North is up, east is to the left, and the image section shown here is 1.39 arcseconds across. // Credit: Gemini Observatory/NSF/NASA/AURA
Despite being infamously demoted from its status as a major planet, Pluto (and its largest companion, Charon) recently posed as a surrogate extrasolar planetary system to help astronomers produce exceptionally high-resolution images with the 8-meter Gemini North Telescope. Using a method called reconstructive speckle imaging, the researchers took the sharpest ground-based snapshots ever obtained of Pluto and Charon in visible light, which hint at the exoplanet verification power of a large state-of-the-art telescope when combined with speckle imaging techniques. The data also verified and refined previous orbital characteristics for Pluto and Charon while revealing the pair’s precise diameters.

“The Pluto-Charon result is of timely interest to those of us wanting to understand the orbital dynamics of this pair for the 2015 encounter by NASA’s New Horizons spacecraft,” said Steve Howell from the NASA Ames Research Center in Moffett Field, California. In addition, Howell notes that NASA’s Kepler mission, which has already proven a powerful exoplanet discovery tool, will benefit greatly from this technique.

Kepler identifies planet candidates by repeatedly measuring the change in brightness of more than 150,000 stars to detect when a planet passes in front of, or affects the brightness of, its host star. Speckle imaging with the Gemini Telescope will provide Kepler’s follow-up program with a doubling in its ability to resolve objects and validate Earth-like planets. It also offers a 3- to 4-magnitude sensitivity increase for the sources observed by the team. That’s about a 50-fold increase in sensitivity in the observations Howell and his team made at Gemini. “This is an enormous gain in the effort underway to confirm small Earth-size planets,” Howell said.

To institute this effort, Howell and his team, which included Elliott Horch from Southern Connecticut State University, New Haven; Mark Everett from the National Optical Astronomy Observatory; and David Ciardi from NASA’s Exoplanet Science Institute/Caltech in Pasadena, California, temporarily installed a camera called the Differential Speckle Survey Instrument (DSSI) among the suite of instruments mounted on the Gemini Telescope.

“This was a fantastic opportunity to bring DSSI to Gemini North this past July,” said Horch. “In just a little over half an hour of Pluto observations, collecting light with the large Gemini mirror, we obtained the best resolution ever with the DSSI instrument — it was stunning!”

The resolution obtained in the observations, about 20 milliarcseconds, easily corresponds to separating a pair of automobile headlights in Providence, Rhode Island, from San Francisco, California. To achieve this level of definition, Gemini obtained a large number of quick “snapshots” of Pluto and Charon. The researchers then reconstructed them into a single image after subtracting the blurring effects and ever-changing speckled artifacts caused by turbulence in the atmosphere and other optical aberrations. With enough snapshots — each image was exposed for only 60 milliseconds, or about 1/20 of a second — only the light from the actual objects remains constant, and the artifacts reveal their transient nature, eventually canceling each other out.

DSSI was built at SCSU between 2007–2008 as a part of a United States National Science Foundation Astronomical Instrumentation grant and mounted on the Gemini North Telescope for a limited observing run. The instrument is likely to return to Gemini North for observations in mid-2013 for general user programs from across the international Gemini partnership.

0

JOIN THE DISCUSSION

Read and share your comments on this article
Comment on this article
Want to leave a comment?
Only registered members of Astronomy.com are allowed to comment on this article. Registration is FREE and only takes a couple minutes.

Login or Register now.
0 comments
ADVERTISEMENT

FREE EMAIL NEWSLETTER

Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter.

ADVERTISEMENT
ADVERTISEMENT
BoxProductcovernov

Click here to receive a FREE e-Guide exclusively from Astronomy magazine.

Find us on Facebook

Loading...