ИСТИНА

Astronomers AO KNUSH (Churyumov, Ponomarenko, and Baransky) from 2008 to 2011, observed the spectra of the Moon with a 2-m Zeiss telescope at the Terskol to find the resonance lines of the luminosity Na (5890-5896ÅÅ) and K (7699 Å), which were detected earlier in the lunar atmosphere. The most successful were observing the spectra of the lunar atmosphere on 12-13 August 2009. In these spectra were found bright luminosity of the sodium doublet DI and DII spectral lines. Spectra of a temporary lunar atmosphere, which is formed during the bombardment of the Moon reholit by meteoroids of Perseid’s meteor streams observed on 12/13.08.09 and 13/13.08.09 with the 2-m Zeiss telescope at pick Terskol. Obtained 6 eshelle spectra at a distance of 50", 150" and 250" arcsec from the Moon’s limb (on the north pole). Observations were carried out in probable area bombing by meteoroids of meteor shower Perseids. Spectral resolution - λ / Δλ = 15 000 or 0,2 Ǻ / pixel. Processing of the spectra showed the existence of a noticeable luminosity of sodium doublet DI and DII a little stronger on 13 August during the peak of the meteor shower Perseids of bombardment of the Moon than Aug. 12, 2009. The spectra of of the Moon’s temporary atmosphere were also observed 15/16 May (during the full lunar eclipse) and 16/17 May 2011. Noticeable glow of sodium in the background of continuous solar spectrum in the spectrum of the atmosphere of the Moon is not found, due to the absence in this period of active meteor showers bombarding the Moon regolith.