SETI Institute Projects and Programs (Listed Chronologically)

Precision Pointing Reconstruction and Backplanes in Support of Cassini Remote Sensing Science

Thursday, November 06 2014 - 9:11 am, PST
The objective of this proposal is to generate several higher-order data products that will substantially reduce the level of effort required to analyze Cassini's optical remote sensing data sets (ISS, VIMS, CIRS and UVIS), by eliminating the need for most scientists to perform their own navigation and geometric reconstruction.

Initial Analysis of Pluto's Tiniest Moon

Thursday, November 06 2014 - 9:08 am, PST
This is an unsolicited proposal to perform the initial scientific analysis of Pluto’s tiniest moons, the recently-discovered “P4” (S/2011 (134340) 1; Showalter et al. 2011) and “P5” (S/2012 (134340) 1; Showalter et al. 2012b). It will enable the P.I. to determine the bodies’ orbits, shapes and sizes based on all of the available Hubble data, using established measurement and modeling techniques. The results of this analysis will be published promptly and will be presented at a scientific workshop about the Pluto system in July 2013.

Orbital Evolution and Stability of the Inner Uranian Moons

Thursday, November 06 2014 - 9:06 am, PST
Orbital Evolution and Stability of the Inner Uranian Moons

CIRS Investigations of Planetary Rings

Thursday, November 06 2014 - 9:04 am, PST
This is a new, five-year proposal to support the work of CIRS co-investigator Dr. Mark Showalter on behalf of the Cassini Project. It is a successor to our current cooperative agreement, NNX06AC85A. The predecessor agreement has supported the Cassini-related activities of Dr. Showalter and his SETI Institute colleagues Dr. Stu Pilorz, Robert French and, briefly, Dr. Nicolas Altobelli. This report provides a brief summary of our accomplishments during the previous agreement and outlines our plans for the years ahead. The Cassini Mission is now expected to continue into 2017, so this proposal describes our planned work for most of the remainder of the Cassini tour. Our activities encompass conducting fundamental scientific research with the CIRS data, plus meeting a large and continuing set of responsibilities for mission operations and planning.

Orbital Evolution and Stability of the Inner Uranian Moons

Thursday, November 06 2014 - 9:02 am, PST
Orbital Evolution and Stability of the Inner Uranian Moons

New Horizons Mission Planning Support: A Deep Search for Faint Rings of Pluto

Thursday, November 06 2014 - 9:01 am, PST
New Horizons Mission Planning Support: A Deep Search for Faint Rings of Pluto

Preserving Voyager's Legacy: Image Calibration and Geometry Reconstruction

Thursday, November 06 2014 - 8:59 am, PST
The Voyager flybys remain our best source of data for the Uranus and Neptune systems, and provide key reference points for continuing studies of Jupiter and Saturn. However, because the Voyager mission pre-dates NASA's focus on archiving, the data sets remain difficult to use. We propose to modernize the Voyager data sets by (a) producing calibrated and geometrically corrected versions of all the images; (b) generating accurate, continuous "C kernels" describing the pointing of the instruments during each Voyager flyby; and (c) using this information to generate detailed geometric indices describing the contents of the Voyager images and spectra. The resulting volumes of derived products will be delivered to the Planetary Data System. This work will ensure that the Voyager data sets remain easily usable by the scientific community for many decades to come.

Orbital Evolution and Stability of the Inner Uranian Moons

Thursday, November 06 2014 - 8:57 am, PST
Orbital Evolution and Stability of the Inner Uranian Moons

Big Picture Science Radio Show

Wednesday, November 05 2014 - 9:38 pm, PST
Monies from the grant will be used to augment the “on-site” feel and appeal of our programming in several ways.

Astrobiology Education and Outreach Projects at the SETI Institute

Wednesday, November 05 2014 - 9:34 pm, PST
A proposal seeking funding for the continued production of one-hour science radio show, travel expenses for guests, and the development of a database on societal impacts of astrobiology.

Pages