Mare Crisium
Sketch and details by Dale Holt
Mare Crisium (the “sea of crises”) is a lunar crater located in the Moon’s Crisium basin, just northeast of Mare Tranquillitatis. This basin is of the Pre-Imbrian period, 4.55 to 3.85 billion years ago. This mare is 376 miles (605 km) in diameter, and 176,000 km2 in area. It has a very flat floor, with a ring of wrinkled ridge toward its outer boundaries. Ghost craters, craters that have largely been buried under deposits of other material, are located to the south.
The crater has many notable features in and around it. The cape-like feature protruding into the southeast of the mare is Promontorium Agarum. On the western rim of the mare is the palimpsest Yerkes. The crater Picard is located just to the east of Yerkes, and northwest of Picard is the crater Peirce. Mare Anguis can be seen northeast of Mare Crisium. Mare Crisium is the site of the Luna 15 crash in 1969.
I used my 150mm F9 Triplet refractor and Denkmeier binoviewer fitted with 32mm Plossl eyepieces to view this Mare.
I captured the image on black art paper approx 125mm x 125mm using a white Conte pastel, white ‘Derwent’ watercolour pencil, white ‘Derwent’ pastel pencil, black ink pen & blending stump.
The image was scanned and reorientated hopefully to match the description above description lifted from Wikipedia.
Date of Sketch 15-Sept-2008 20.15 UT
Seeing Ant III
Mag 98x
Moon phase 99.6%
Location: Chippingdale observatory, Chipping, Hertfordshire, England
Dale,
A most impressive sketch of the Sea of Crisis and the many craters surrounding it. With the terminator just West of the mare as the full moon begins to wane, you have beautifully captured the deep shadowed craters there. Wonderful sketching.
Frank 🙂
Dear Frank,
I thank you for being too generous with your comments towards me as usual.
Warmest regards, Dale ;¬)