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Ю.Е.Навроцкий, Ю. Е.; Черниговский национальный педагогический университет имени Т.Г.Шевченко (2016)
Publisher: Національний Авиаційний Університет
Languages: Ukrainian
Types: Article
Subjects: remote estimation of porosity; remote asteroid surface., УДК 523.3, дистанционное определение пористости; поверхность астероида.
It has been suggestedthat the surface of the asteroid scattering function is the same as that of the Moon, and using phase depending shinesome asteroids at phase angles <5◦, porosities were estimated in the range 0,469<p<0,894. В предположении, что индикатриса рассеяния поверхности астероидов такая же, как и у Луны, и используя фазовые зависимости блеска некоторых астероидов при фазовых углах <5◦, получили значения пористостив пределах 0,469<p<0,894. Зробивши припущення, що iндикатриса розсiювання поверхнi астероїдiв така ж сама, як i у Мiсяця, i використовуючи фазову залежнiсть блиску для кутiв <5◦ для деяких астероїдiв отримали значення пористостi в межах0,469<p<0,894.
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