2- waning gibbous

3- 3,72,280 km

4- calvious crator , Grimaldi basin

5- The Grimaldi impact basin's basalt-flooded center is surrounded by an inner wall that is about 124 miles (200 km) in diameter and a partial, 248-mile-long (400 km) outer wall. The outer wall is almost as long as the Grand Canyon.

6- Grimaldi basin

2- warning gibbous

3- 4,02,637 km

4- tycho crater , Kepler crater

5- Rays of material ejected by the impact that created this crater extend over 185 miles (300 km) ― almost 10 times farther than the crater's diameter. This impact event was energetic enough to excavate material from great depth and distribute it around the crater. Surface material is ejected the furthest, while the deepest material has just enough energy to land on the crater rim

6-Mare Crisium

2.Waning crescent

3.3,69,164 km

4.Rises in afternoon and sets before sunrise.

5. The "Sea of Cold" is located in the outer rings of the huge, flat region called Oceanus Procellarum

6.Mare firogoris

Waxing crescent

2,46,375 miles

Mare crisium and Endymion crater

The "Sea of Crises" covers over 109,000 square miles (176,000 sq km) of the lunar surface ― about the size of Nevada.

Endymion crater

1. 10 june

2. Waxing crescent

3. 394843

4. Mare crisium. Mare facundatatis

5. Waxing crescent

6. This phase occurs when the illuminated half of the Moon faces mostly away from Earth, with only a tiny sliver visible to us from our planet. As the Moon's orbit carries the Moon's dayside farther into view, the sunlit crescent appears to grow. A waxing crescent rises shortly after sunrise and sets shortly after sunset, rising a little later each day. It is easiest to find in the evening when the sky grows darker