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Ый

Ый диэн Сир соҕотох уонна Күн систематын улаханынан бэhис аргыhа.

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  1. ↑ 1 2 3 4 5 6 7 Цитата сыыһата: Сыыһа <ref> тиэк (тег); W06 диэн хос быһаарыыларга аналлаах тиэкис суох
  2. ↑ The maximum value is given based on scaling of the brightness from the value of -12.74 given for an equator to Moon-centre distance of 378 000 km in the NASA factsheet reference to the minimum Earth-Moon distance given there, after the latter is corrected for the Earth's equatorial radius of 6 378 km, giving 350 600 km. The minimum value (for a distant new moon) is based on a similar scaling using the maximum Earth-Moon distance of 407 000 km (given in the factsheet) and by calculating the brightness of the earthshine onto such a new moon. The brightness of the earthshine is [ Earth albedo × (Earth radius / Radius of Moon's orbit)² ] relative to the direct solar illumination that occurs for a full moon. ({{{1}}}; {{{1}}} radius × equatorial {{{1}}}).
  3. ↑ 1 2 Williams, D.R. Moon Fact Sheet. NASA (10 Олунньу 2006). Сигэнии күнэ: 12 Алтынньы 2007.
  4. ↑ The range of angular size values given are based on simple scaling of the following values given in the fact sheet reference: at an Earth-equator to Moon-centre distance of 378 000 km, the angular size is 1896 arcseconds. The same fact sheet gives extreme Earth-Moon distances of 407 000 km and 357 000 km. For the maximum angular size, the minimum distance has to be corrected for the Earth's equatorial radius of 6 378 km, giving 350 600 km.
  5. ↑ A.R. Vasavada, D.A. Paige, and S.E. Wood (1999). «Near-Surface Temperatures on Mercury and the Moon and the Stability of Polar Ice Deposits». Icarus 141: 179. DOI:10.1006/icar.1999.6175.

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