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Another way to study this class of disruption events is to separately calculate the cross sections for fly-by encounters to ionize the solar system, and combine these results with the rate of stellar encounters to determine an optical depth, τs, for scattering (Adams and Laughlin, 2001; Li ...
一、选择括号中的词填空1. The Sun is a ___(star/planet).2. Mr Li's class is very ___(lovely/liv
And M-dwarf protostellar nebulae–the natal origins of these small red stars–have proven relevant to the search for liquid water on the surfaces of these worlds, and vital to the discussion of whether M-dwarf planets as a class are expected to be water rich....
density distribution of young stellar objects (YSOs) in nearby (\(<500\)pc) regions shows a smooth distribution [27], implying that there is no bimodal distribution to star formation, e.g., ‘clustered’ versus ‘isolated,’ but rather that star formation results from a continuum of ...
Gordon-Levitt stated that he was attracted to the role because "it's a Disney animated movie and Disney animated movies are in a class by themselves," and that "to be part of that tradition is unbelievable to me". Musker mentioned that Gordon-Levitt "combined enough vulnerability and ...
PLANET MESSI; THE GREATEST FOOTBALLER EVER? Cruyff: Barca Star in a World Class of His OwnByline: NEIL McLEMAN JOHAN CRUYFF has hailed Lionel Messi as a world footballing treasure...The Mirror (London, England)
Finally, multiple 30-m class telescopes (extremely large telescopes; ELTs) are under construction with first light expected at the end of the decade. The transformative sensitivity and angular resolution ELTs provide the first resolved observations of individual objects in regions too distant for ...
Class O stars evaporate their surroundings quickly. The article said, "This means that younger disks have a lot more raw material from which planets could form," Tobin said in the statement. "Possibly, bigger planets already start to form around very young stars." Four of the young stars ...