EVLA Observations of Pluto, Charon, Makemake, Quaoar, and 2002 TC302 at 0.9 cm Wavelength

Details EVLA Observations of Pluto, Charon, Makemake, Quaoar, and 2002 TC302 at 0.9 cm Wavelength EVLA Observations of Pluto, Charon, Makemake, Quaoar, and 2002 TC302 at 0.9 cm Wavelength

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1670b&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1670

Computer Science

Scientific paper

Observations of the Trans-Neptunian Objects (TNOs) Pluto, Charon, Makemake, Quaoar, and 2002 TC302 were made with the Expanded Very Large Array at a wavelength of 0.9 cm. These observations can be used to constrain the properties of the surfaces and subsurfaces (down to ~10 cm) of these bodies, including temperature, composition, and structure. We have detected Pluto and Charon, with the emission separated on the sky; the longest wavelength detection of either of these bodies to date. We have only upper limit non-detections for Makemake and 2002 TC302, but more data remain to be reduced, and we have not reduced any Quaoar data yet.

Affiliated with

Also associated with

No associations

Rating

EVLA Observations of Pluto, Charon, Makemake, Quaoar, and 2002 TC302 at 0.9 cm Wavelength does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with EVLA Observations of Pluto, Charon, Makemake, Quaoar, and 2002 TC302 at 0.9 cm Wavelength, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and EVLA Observations of Pluto, Charon, Makemake, Quaoar, and 2002 TC302 at 0.9 cm Wavelength will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1487560