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  • Roger Bagula
    Subject: Gemini Observatory Shows That 10th Planet Has a Pluto-Like Surface From: baalke@earthlink.net Date: 1 Aug 2005 09:03:10 -0700 Newsgroups:
    Message 1 of 1 , Aug 2, 2005
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      Subject:
      Gemini Observatory Shows That '10th Planet' Has a Pluto-Like Surface
      From:
      baalke@...
      Date:
      1 Aug 2005 09:03:10 -0700
      Newsgroups:
      sci.astro,alt.sci.planetary

      http://www.gemini.edu/index.php?option=content&task=view&id=142
      
      Gemini Observatory Shows That "10th Planet" Has a Pluto-Like Surface
      Gemini Observatory
      29 July 2005
      
      Gemini Observatory has obtained a preliminary spectrum of 2003 UB313,
      the so-called "10th planet". These observations were obtained on
      January
      25, 2005 by Chad Trujillo, a Gemini staff member who is also on the
      discovery team for 2003 UB313, the existence of which was formally
      announced by the Minor Planet Center in Cambridge, MA on July 29, 2005.
      The discovery team (Mike Brown of Caltech, Chad Trujillo of Gemini and
      David Rabinowitz of Yale) are still uncertain of the exact size of the
      body, but report that it must be Pluto-sized or larger. The body is the
      most distant solar system body known to orbit the sun at 97 AU from the
      sun, over 3 times farther away than planet Pluto. The "planet" was
      originally discovered in late December 2004 with data collected from
      the
      Samuel Oschin 1.2 meter telescope at Palomar Mountain, CA.
      
      To better characterize the surface of the object the team obtained
      spectra with NIRI (the near-infrared spectrograph) on the much larger 8
      meter Gemini North telescope on Mauna Kea, Hawaii. The NIRI spectra
      shows strong signatures of methane ice, remarkably similar to the
      spectrum of Pluto, which is also dominated by methane ice in
      near-infrared observations. Figure 2 shows the spectra of Pluto and
      2003
      UB313, with arrows marking the "dips" that correspond to methane
      features. The same features are readily apparent in both the Pluto and
      the 2003 UB313 spectra.
      
      Figure 2: 2003 UB313 spectrum (red, obtained at Gemini Observatory by
      Trujillo, Brown and Rabinowitz) and Pluto (black, from Rudy et al.
      2003). The "dips" characteristic of methane ice are indicated by red
      arrows and are present in both 2003 UB313 and Pluto.
      
      Trujillo states, "We still do not know much about this object, however,
      it is clear that it is very similar to Pluto in both size and
      composition, at least upon first glance." The presence of methane ice
      is
      unusual in that it indicates a primitive surface that has not likely
      been heated significantly since the solar system formed 4.5 billion
      years ago. "If 2003 UB313 ever got close to the sun, all the methane
      ice
      would have boiled off immediately," Trujillo continued. "To date, no
      one
      has seen methane on any other Kuiper Belt Object, only on Pluto and
      Neptune's moon Triton." The distant Kuiper Belt is a collection of
      bodies orbiting the sun beyond Neptune, and is likely the parent
      population to the comets.
      
      The team have also obtained spectra of the smaller mini-planet 2003
      EL61, which was reported on July 28, 2005 by two independent teams: one
      from the Sierra Nevada Observatory in Spain and the Brown, Trujillo and
      Rabinowitz team. This object is smaller than Pluto, but shows strong
      water-ice features, similar to what is seen on the surface of Pluto's
      moon Charon.
      
      Results will be reported in detail at the 37th annual meeting of the
      Division for Planetary Sciences of the American Astronomical Society in
      September 2005 at the University of Cambridge, UK.
      
      
      -- 
      Roger L. Bagula { email: rlbagula@...  or  rlbagulatftn@... }                             
      11759 Waterhill Road,                               
      Lakeside, Ca. 92040    telephone: 619-561-0814
      
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