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Dwarf Planet Eris in Cetus

 Please wait for all
 3 animation frames
 to load.

 Eris is in the lower-right
 quarter of the image
 and moving further to the
 lower-right.

These 3 images were taken about 24 hours apart.
Each image is a stack of 400 video frames. The 9 to 11 day old Moon was high in the sky at the time. The listed magnitude for Eris was 18.9 visual and 18.7 photographic. The video is pretty sensitive in the IR part of the spectrum so with Eris being fairly bright in the IR is why it shows up well through a bright sky. The distance to Eris is about 97 AU which is nearly 3 times more distant than Pluto.

Positions for images:
Date__(UT)__HR:MN   R.A._(ICRF/J2000.0)_DEC APmag
********************************************************
2006-Oct-02 00:00 * 01 38 25.81  -05 17 21.1  18.72
2006-Oct-03 00:00 * 01 38 23.68  -05 17 33.7  18.72
2006-Oct-04 00:00 * 01 38 21.54  -05 17 46.3  18.71

Found this table on a paper on 2003 UB313 giving brightness and reflectance at each wavelength.



Another set of images,
 this time taken in a dark sky.
 
Each frame of the animation
 is a stack of 400 video frames.
 
 
Please wait for
all 3 animation
frames to load.
 
 
The 3rd frame was taken ahead
of a weather front and the
seeing was pretty bad.

  


 Image Info

- Imaged on 20061002-04
- 31.5 cm f/4.5
  Newtonian Reflector
- 400 video frames
  no filter for each image
 
Formally known as 2003 UB313

 JPL Horizons 
 generate ephemerides for 
 solar-system bodies. 

 


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