ꯊꯥꯅꯤꯜ

ꯊꯥꯅꯤꯜ ꯍꯥꯏꯕꯁꯤ ꯊꯥꯒꯤ ꯃꯃꯥꯏ ꯑꯃꯅꯤ ꯃꯂꯦꯝ ꯁꯤꯗꯒꯤ ꯌꯦꯡꯕ ꯃꯇꯝꯗ ꯊꯥ ꯅꯥ ꯃꯄꯨꯡ ꯐꯥꯅꯥ ꯆꯥꯎꯅꯥ ꯀꯣꯏꯅꯥ ꯄꯥꯛꯅꯥ ꯎꯕ ꯃꯇꯝꯅꯤ ꯫ ꯃꯁꯤ ꯃꯂꯦꯝ ꯑꯄꯥꯛꯉꯥ ꯁꯤ ꯅꯥ ꯅꯨꯃꯤꯠ ꯑꯃꯁꯨꯡ ꯊ ꯒꯤ ꯃꯔꯛꯇꯥ ꯆꯞ ꯆꯥꯅꯥ ꯂꯩꯕ ꯃꯇꯝꯗ ꯊꯣꯛ ꯏ ꯫ ꯊꯥꯁꯤ ꯅꯠꯇ꯭ꯔꯒ ꯊꯥꯅꯤꯜ ꯑꯅꯤꯁꯤꯒꯤ ꯃꯔꯛꯁꯤ ꯑꯃꯨꯛ ꯑꯣꯏꯅꯕ ꯌꯥꯡꯆꯠꯇꯥ ꯅꯨꯃꯤꯠ ꯲꯹.꯵꯳ ꯆꯪꯉꯤ ꯫ ꯃꯁꯤꯅꯥ ꯃꯔꯝ ꯑꯣꯏꯔꯒ ꯊꯥꯅꯤꯜ ꯁꯤ ꯊꯥ ꯑꯗꯨꯒꯤ ꯱꯴ ꯄꯥꯟꯕ ꯅꯠꯇꯔꯒ ꯱꯵ ꯄꯥꯟꯕ ꯅꯨꯃꯤꯠꯁꯤꯡꯗ ꯑꯣꯏ ꯫ ꯃꯔꯝꯗꯤ ꯊꯄꯥꯂꯣꯟ ꯒꯤ ꯆꯩꯆꯠ ꯇꯥ ꯊꯥ ꯑꯃꯥꯁꯤ ꯅꯨꯃꯤꯠ ꯲꯹ ꯅꯠꯇꯔꯒ ꯅꯨꯃꯤꯠ ꯳꯰ ꯑꯣꯏꯕꯒꯤꯅꯤ ꯫

ꯊꯥꯕꯜ ꯌꯥꯝꯅ ꯐꯕ ꯅꯨꯃꯤꯠ ꯲꯳꯵ ꯃꯤm (꯹.꯲꯵ in) Schmidt-Cassegrain telescopeꯇꯒꯤ ꯎꯕ ꯁꯛꯇꯝ ꯫ The Moon was near its northernmost ecliptic latitude, so the southern craters are especially prominent

ꯐꯨꯡꯒꯥ ꯋꯥꯔꯤ ꯑꯃꯁꯨꯡ ꯆꯠꯕꯤꯗ

Full moon rising, seen through the Belt of Venus

ꯂꯧ ꯂꯣꯛꯄꯥ ꯑꯃꯁꯨꯡ ꯁꯥꯇꯥꯟꯕ ꯊꯥ

A harvest moon. Its orange color is due to its closeness to the horizon, rather than being unique to harvest moons.^[꯱]

ꯂꯧꯔꯛꯐꯝꯁꯤꯡ

↑ cite web|url=https://web.archive.org/web/20160303230520/http://www.research.utoronto.ca/harvest-moon/ |title=Why is the harvest moon so big and orange? |date=27 September 2010 |publisher=University of Toronto |last=Percy |first=John

[1] te web|url=https://web.archive.org/web/20160303230520/http://www.research.utoronto.ca/harvest-moon/ |title=Why is the harvest moon so big and orange? |date=27 September 2010 |publisher=University of Toronto |last=Percy |first=John

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