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???????? - ????????? ??????????IAEA???????????????????? ... ???????????. ???????????????????? ... ?? 19 ??????????????????????????? JRR-3 ????. ?????????????. 2. ????????????????????????? JRR-4 ... ??????????????(?)??????????????????????????? 20 ? 9. ?. (? 1.16-2) ????????????????????????? 19 ?????. ?????? ... ?? ?? - ?????????3?4??????????????????????. ???????????????????????????????????????????????????. ????????????????????????? ????? ...???????????????????????????????? 2050 ??? ... ?????????????????????????. ????????? ... ??????????????????? ????? ... - ?????????. ?????????????????????????? ... ??????????????????????????HEAF????????. ?????????????????????????????19?20?? ???????????????????????????. ? ?. ? ????. 1? ????????????????. ?62????????????? ??3 - ?????????????????????6?? ??. ???????????????????. ???A?????????????. ??????????????. The scientific potential of orbital missions to Uranus and NeptuneThis limited timespan makes the mission sensitive to short-period planets only. Only a handful of K2 exoplanets with periods longer than 40 days (half the ... Liquid methane at extreme temperature and pressure - JETP LettersTESS TPF of TOI-815 created with tpfplotter (Aller et al. 2020). The orange pixels define the aperture mask used for extract- ing the photometry. Additionally, ... Formation of Super-EarthsWe could also investigate planet compositions in or near the habitable zone of Sun-like stars. Another interesting feature to study would be the planet radius. UC Santa Cruz - eScholarshipStandard structure models of the planets consist of three layers: a rocky core, an 'icy' shell (water, ammonia, methane, etc.), and a gaseous envelope composed ...
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