
********* CALL FOR SMALL TELESCOPES IN SOUTHEAST ASIA *********
Most of our work today is logistical, trying to find places that are in the new Pluto and Charon shadows. For Pluto, we’ve made contact at a larger telescope in Japan.
To catch the Hydra track in Hawaii, we’ll be spreading ourselves to more sites rather than trying to compare lightcurves from two telescopes at the same sites. We’re looking into adding a telescope at one of the islands in the Kwajalein atoll. This is not trivial, because you can only get there by helicopter.
As you read here, we got the June 23 Pluto and Charon occultation, and we were able to update our prediction for the Hydra shadow. The new prediction for the Hydra path is now crossing areas in Southeast Asia. Are there any telescopes that can help with this observation?
We’re looking for 11-inch or larger telescopes in Indonesia, Thailand, and Malaysia too. Our host in Cebu City, Christopher Go, knows many of the amateur groups there, and we’re making good contacts. Anyone who is interested in helping out can contact me at layoung@boulder.swri.edu.
SCIENCE GOALS
Pluto has one large moon, Charon, and two small moons, Nix and Hydra. Nix and Hydra were only discovered six years ago, and very little is known about their physical properties. An occultation would give us the first measurement of the size of Hydra. Also, because the four bodies pull on each other in subtle ways that depend on their masses, improving the orbit will help us measure the mass. Finally, we hope to measure the cross-section of Hydra from two different angles, one from occultations and one from the New Horizons spacecraft.
IMPORTANCE OF SOUTHEAST ASIA
he newest prediction—good to maybe 300 kilometers—is here:
See in particular:
WHAT IS NEEDED TO ATTEMPT TO THE HYDRA OCCULTATION
* located anywhere within 300 kilometers of the predicted shadow
* 20 minutes of continuous images taken June 27, 14:42 to 15:02 UT
* 11-inch or larger telescope
* camera with low dead time (less than 0.1 seconds between exposures)
Best is:
* larger telescopes, which will give higher signal
* pairs or clusters of sites where telescopes are spaced 2 to 50 kilometers apart (25 kilometers is ideal)
* wide field-of-view (20 arcseconds), to make finding this crowded field easier
* integrating CCDs that can observe at 0.5 seconds with little time between exposures
* some way of telling the time of the observations
* an additional 20 minutes of continuous images taken June 27, 14:08 to 14:28 UT, in case Pluto’s shadow is actually over Malaysia
FOR MORE INFO
Our planning pages (finder charts, stars for star hopping, etc) are at:
Our planning pages (finder charts, stars for star hopping, etc) are at:
Read full news coverage on National Geographic:

Leslie Young
layoung@boulder.swri.edu
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