Title: Stellar Occultation by Charon as Observed from Chile
1Stellar Occultation by Charon as Observed from
Chile
- Taavi Tuvikene
- Vrije Universiteit Brussel
- Contact Group Meeting, 19 May 2006
2Cerro Armazones, Chile
3Observatorio Cerro Armazones
442 cm
84 cm
5Rotating the Dome
6Stellar Occultation by Charon
- Occultation Charon passes in front of a star
- The highest spatial resolution available from the
Earth - Stellar occultation in 1980
- 2 years after discovery
- one observation (in South Africa)
- lower limit to Charons radius 600 km
- 25 years later ...
711 July 2005 (prediction)
- Geocentric mid-time11-7-2005 033701 (UT)
- Shadow diameter1200 km
- Shadow velocity on the ground 21.3 km/s
- C313.2 magnitudeR 14.8
- Distance of Pluto30.06 AU
http//occult.mit.edu/research/occultations/Charon
/C313.2.html
8Observatories / Research Groups
San Pedro
- Massachusetts Institute of Technology (MIT)
Williams College - Group led by Paris Observatory
- Southwest Research Institute (SwRI) Wellesley
College
Paranal
Cerro Armazones
Las Campanas (du Pont, Clay)
Cerro Pachon (Gemini)
Cerro Pachon (SOAR)
El Leoncito
9Telescopes Instrumentsused by MIT team
- Chile
- Observatório Cerro Armazones 84 cm POETS
- Las Campanas
- Du Pont 2.5 m POETS
- Clay 6.5 m POETS
- Cerro Pachón
- Gemini South 8 m Acquisition Camera
(R-filter) - Brasil
- Observatório Pico dos Dias, Itajubá 0.6 m
POETS no observations due to clouds
10Stellar Occultation (video)
http//occult.mit.edu/research/occultations/Charon
/C313.2/C313OccMovie.html
11Light-curves
See Figure 2 in Gulbis, A. A. S. et al. Nature
439, 4851
12Occultation Chords
See Figure 1 in Gulbis, A. A. S. et al. Nature
439, 4851
13Charons Atmospheric Models
See Figure 3 in Gulbis, A. A. S. et al. Nature
439, 4851
Clay light-curve
14Results (Gulbis et al. 2006)
- Charons mean radius 606 8 km
- Bulk density 1.72 0.15 g/cm3
- Rock-ice mass fraction 0.63 0.05
- Smaller than Plutos impact formation scenario
- No significant atmosphere
15Results
Nature, 5 January 2006