MESSENGER Captures Images of Comets Encke and ISON
MESSENGER’s cameras have been acquiring targeted observations of Encke since October 28 and ISON since October 26, although the first faint detections didn’t come until early November. During the closest approach of each comet to Mercury, the Mercury Atmospheric and Surface Composition Spectrometer (MASCS) and X-Ray Spectrometer (XRS) instruments also targeted the comets. Observations of ISON conclude on November 26, when the comet passes too close to the Sun, but MESSENGER will continue to monitor Encke with both the imagers and spectrometers through early December.
In contrast, ISON did not pass as close to Mercury, but the comet was between the Earth and Mercury when it passed closest to MESSENGER. “We saw the side opposite to that visible from Earth,” says Vervack, “so our images and spectra are complementary to observations from Earth made at the same time and could aid in understanding the variable activity of the comet as it approached the Sun.”
On the day that Encke was closest to Mercury, the MDIS wide-angle camera scanned the comet with all of its 12 filters while the instrument’s narrow-angle camera (NAC) snapped images of the rotating comet every 10 minutes to capture a full 360° view. The imaging campaign for ISON was similar, with the NAC capturing a series of stills every 30 minutes.
Several ground- and space-based NASA observatories, as well as many other observatories around the world, are collecting data on the comets. However, none will be able to collect simultaneous images and spectra from X-ray through near-infrared wavelengths when the comets are so close to the Sun, as will MESSENGER. Vervack expects MESSENGER to gather 15 hours worth of data on Encke and another 25 hours on ISON. “These observations of Encke and ISON fill a gap in heliocentric coverage to which most other observatories don’t have access,” Vervack says.
Scientists are still combing through the data collected by MASCS, but there are already confirmed detections of several molecules and atoms, including OH, NH, CS, oxygen, carbon, sulfur, and hydrogen. “Far-ultraviolet observations can’t be made from ground-based observatories, and only a few instruments in space have been able to look at the comets in the ultraviolet,” says Vervack. “The MASCS observations are therefore of great interest.”
Taken together, the MESSENGER observations offer a varied science investigation of the comets. “Whereas the MDIS images will provide a global picture of the comet coma morphology, MASCS observations will inform us about the composition of the cometary ices and XRS may be able to tell us what the dust is made of,” Vervack says.
“Comet encounters were not considered when the MESSENGER mission was designed,” adds MESSENGER Principal Investigator Sean Solomon of Columbia University. “If Encke and ISON share a few of their secrets on the formation and evolution of the solar system, the MESSENGER team will be delighted with the scientific bonus.”
Publication of press-releases or other out-sourced content does not signify endorsement or affiliation of any kind.