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Hello, I'm BracketBot. I have automatically detected that your edit to Amorphous ice may have broken the syntax by modifying 4 "{}"s. If you have, don't worry: just edit the page again to fix it. If I misunderstood what happened, or if you have any questions, you can leave a message on my operator's talk page.
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of high-density amorphous ice is also created during vapor deposition of water on low-temperature (< 30 K) surfaces such as interstellar grains. The water molecules do not fully align to create the
With radiation equilibrium temperatures of 40-50 K, <ref>{{cite journal|title=Colors and Spectra of Kuiper Belt Objects|author=Jewitt, David C.; Luu, Jane X.|
are expected have amorphous water ice. While water ice has been observed on several objects, <ref>{{cite journal|title=Water Ice on Kuiper Belt Object 1996 TO_66|author=Brown, Robert H.; Cruikshank,
The Astrophysical Journal|volume=519|page=L101|year=1999|bibcode=1999ApJ...519L.101B}</ref><ref>{{cite journal|title=Water ice on the surface of the large TNO 2004 DW|author=Fornasier, S.; Dotto,
on (5000) Quaoar, perhaps due to resurfacing events such as impacts or cryovolcanicism. <ref>{{cite journal|title=Crystalline water ice on the Kuiper belt object (50000) Quaoar|author=Jewitt,
Europa, Ganymede, and Callisto. The temperatures of these moons range from 90-160 K, <ref>{{cite journal|title=Temperatures on Europa from Galileo Photopolarimeter-Radiometer: Nighttime
ice, Ganymede has both amorphous and crystalline ice, and Callisto is primarily crystalline. <ref>{{cite journal|title=Amorphous and crystalline ice on the Galilean satellites: A balance between
the charged particles to higher latitudes and protect the lower latitudes from irradiation. <ref>{{cite journal|title=Amorphous and crystalline ice on the Galilean satellites: A balance between
Hello, I'm BracketBot. I have automatically detected that your edit to Amorphous ice may have broken the syntax by modifying 3 "{}"s. If you have, don't worry: just edit the page again to fix it. If I misunderstood what happened, or if you have any questions, you can leave a message on my operator's talk page.
List of unpaired brackets remaining on the page(Click show ⇨)
of high-density amorphous ice is also created during vapor deposition of water on low-temperature (< 30 K) surfaces such as interstellar grains. The water molecules do not fully align to create the
With radiation equilibrium temperatures of 40-50 K, <ref>{{cite journal|title=Colors and Spectra of Kuiper Belt Objects|author=Jewitt, David C.; Luu, Jane X.|
are expected have amorphous water ice. While water ice has been observed on several objects, <ref>{{cite journal|title=Water Ice on Kuiper Belt Object 1996 TO_66|author=Brown, Robert H.; Cruikshank,
The Astrophysical Journal|volume=519|page=L101|year=1999|bibcode=1999ApJ...519L.101B}</ref><ref>{{cite journal|title=Water ice on the surface of the large TNO 2004 DW|author=Fornasier, S.; Dotto,
on (5000) Quaoar, perhaps due to resurfacing events such as impacts or cryovolcanicism. <ref>{{cite journal|title=Crystalline water ice on the Kuiper belt object (50000) Quaoar|author=Jewitt,
Europa, Ganymede, and Callisto. The temperatures of these moons range from 90-160 K, <ref>{{cite journal|title=Temperatures on Europa from Galileo Photopolarimeter-Radiometer: Nighttime
ice, Ganymede has both amorphous and crystalline ice, and Callisto is primarily crystalline. <ref>{{cite journal|title=Amorphous and crystalline ice on the Galilean satellites: A balance between
the charged particles to higher latitudes and protect the lower latitudes from irradiation. <ref>{{cite journal|title=Amorphous and crystalline ice on the Galilean satellites: A balance between
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Hello, I'm BracketBot. I have automatically detected that your edit to Amorphous ice may have broken the syntax by modifying 4 "{}"s. If you have, don't worry: just edit the page again to fix it. If I misunderstood what happened, or if you have any questions, you can leave a message on my operator's talk page.
