Where would we be without the Moon? It has served as a light source, timekeeper, navigation tool, inspiration for poets, a nearby neighbor to draw us off the planet, and most importantly, it stabilizes our orbital tilt to allow life to flourish on the Earth.
The latest benefit we’ve derived from our weatherless and stable friend is understanding how often space rocks, big and small, cross our orbital path. Recently, NASA’s Lunar Reconnaissance Orbiter photos, which covers 6.6% of the lunar surface, revealed 222 new small craters (2- to 43-meters diameter) created over a period of 7 years1. More ominous, according to a University of Toronto study, “The production rate of large lunar craters (more than 10 kilometers in diameter) increased by a factor of two to three in the past ~300 million years.”2 This is the time-frame of the Cretaceous-Paleogene mass extinction that eliminated T. Rex and friends.
We dedicate this week’s blog to the study of our life-long friend, the Moon, as seen from the surface of the Earth.
This image is of a waning Moon, after being full the day before. At the bottom right of the lunar disc is the famous rayed crater Tyco. Depending on the lighting, you can trace some of these rays far across the visible surface of the Moon. Due to their brightness, the impact was believed to have taken place just 108 million years ago. The dark areas of the moon are the iron-rich maria (Latin for sea). These are lava plains created by volcanic activity due to asteroid impacts on the far side of the Moon. The bright areas are the lunar highlands and mountains formed by asteroid impact debris.
Montes Appenninus is the dramatic 3.9 billion-year-old mountain range running through the center of the image with the shadowed crater Eratosthenes anchoring the left side of the range. These mountains form the border of Mare Imbrium on the upper left, Mare Vaporum on the bottom-left, and Mare Serenitatis on the lower right. The largest of the trio of craters at the top-right is Archimedes (81 km) showing a flat lava interior. The next largest is Aristillus showing multiple central peaks and the smallest is Autolycus.
Apollo 15 Landing Site
The Montes Appenninus image also contains a historic landing site. If you follow the smooth lava plain that borders Archimedes to where it meets Montes Appenninus, you’ll see the squiggle of Hadley Rille bisected by a small crater named Hadley C. Apollo 15 landed on the far right side of Hadley Rille as seen from the perspective of the image.
Archimedes to Aristoteles
This image continues where the above images leave off. Archimedes, Aristillus, and Autolycus are at lower left on this frame. On the extreme opposite side are two large craters Aristoteles (the larger at 87 km) and Eudoxus. Between these sets of craters, is the thin ring of the weathered crater Cassini that encloses two smaller craters. The mountain range at the bottom, below Cassini, is the Montes Caucasus range. The mountains above Cassini are the Montes Alpes. Toward the top-right of center is a cut that runs across Alpes range. This is the famous Vallis Alpes.
This image is a mosaic of the lunar surface. The region in the central part was explored in the prior two photos, with Montes Appenninus, the major mountain range to the left of the center, and the Montes Alpes, with the cut of Vallis Alpes, to the right of center. To the left of Montes Appenninus is Mare Vaporium. The prominent crater Manilius is at the bottom of the image about a third of the way from the left edge. Near the bottom-left are craters Godin and Agrippa (the larger) with notable central peaks. Above Agrippa is crater Triesnecker in the lava plane of Sinus Medii next to Mare Vaporium. On the right of the Montes Alpes is Mare Frigoris and the northern highlands around the polar region.
Remaining Lunar Events for 2022
Super and Micromoons
Due to the elliptical shape of the lunar orbit, the distance from the Earth to the Moon can vary by 50,200 km (31,200 mi). The term “Supermoon” describes a Full Moon that occurs near the Moon’s closest approach to Earth while “Micromoon” describes a Full Moon near the point furthest from the Earth. A Supermoon can be 14% bigger than a Micromoon. There is no agreed-upon definition of how close and far a Moon needs to be to qualify for any of these “Moon” titles. That said, August 12 will have the largest remaining Full Moon of the year and December 7 is the remaining smallest Full Moon of the year. They will differ by 38,900 km (24,200 mi) in distance from the Earth. This should be notable when comparing images taken of the Full Moon on those days with the same focal length lens.
November 8 will feature a total lunar eclipse centered on the Pacific Ocean. The total phase will be visible from eastern North America to Central America and northwestern South America. China, Japan, Eastern India, Southeast Asia, and areas down to Australia will also see totality. Totality will miss Scandinavia, Europe, the Arabian Peninsula, and Africa.
On October 25 the Moon will partially eclipse the Sun. You will need a solar filter to view this type of eclipse. The skies from the arctic to India and through much of Europe, the Middle East, and the northern part of Africa to the horn will darken. The deepest part of the eclipse will be in eastern Russia and Kazakhstan. They will see about 80% of the Sun covered.
Moon and Planet Pairings
The Moon will pose with all the bright planets and Uranus this month. Here is a table of when each planet is nearest the Moon for the month.
|Separation and Moon Phase
|12 August 2022
|<4° to Full Moon
|15 August 2022
|<2° to Waning Gibbous Moon
|18 August 2022
|~½° to Waning Gibbous Moon
|19 August 2022
|<2¾° to 3rd Quarter Moon
|25 August 2022
|~4¼° to Waning Crescent Moon
|29 August 2022
|~6½° to Waxing Crescent Moon
Plato to the Pole
Mare Imbrium dominates the lower-left of the frame with lava-filled, major crater Plato (101 km) near the center. Vallis Alpes is toward the lower-right of Plato as it cuts through to Montes Alpes. The sea above Plato is Mare Frigoris with the northern highlands and the lunar north pole beyond. At the very top of frame is deeply shadowed crater Anaxagoras, with its young, high-albedo rim walls just catching enough light to be identifiable.
We started out with the Moon just past full and we end with the Moon just past New. The allure of the crescent phase is the faintly glowing Earthshine — “the young moon in the old moon’s arms” near the horizon. Leonardo da Vinci was the first to explain, in the 16th century, that light reflecting off the Earth was illuminating the night-side of the Moon.
Tele Vue Refractors
Observing the Moon with any Tele Vue refractor is a striking sight! Whether you are using high power to study the smallest resolvable features, taking advantage of their rich-field capabilities for lunar-planetary conjunctions, or imaging the Moon, these versatile APO refractors cover all bases. Every Tele Vue refractor, from the Tele Vue-60 to the 5″ Tele Vue-NP127is, can give at least a 4° field with our low power eyepieces. With such rich-field capability, the scope are practically their own finder. Our unit-power StarBeam (mobile site) with flip-mirror is the perfect complement to easily aim the scope at the Moon or in the vicinity of the Messier object you are searching for.
From the powder-coated tubes and anodized aluminum finishes to the silky-smooth, lash-free focuser, these scopes are rugged and easily transported to dark-sky locations by land, sea, or sky. Tele Vue telescopes are engineered and built to be your life-long observing companions; and someday, your kids’ as well. All Tele Vue telescopes come with a 5-year Limited Warranty.
Did you observe, sketch, or image with Tele Vue gear? We’ll like your social media post on that if you tag it #televue and the gear used. Example:
#televue #tv85 #ethos #moon
Do you want your Tele Vue images re-posted on Tele Vue Optics’ Social Media accounts? Use this hashtag for consideration:
- 1Witze, Alexandra. “Incoming! Space Rocks Strike the Moon More Than Expected.” Scientific America, 13 Oct. 2016, www.scientificamerican.com/article/incoming-space-rocks-strike-the-moon-more-than-expected.
- 2Mazrouei, Sara. “What the moon’s craters reveal about the Earth’s history: U of T expert and lead author of new study.” University of Toronto, 18 Jan 2019, www.utoronto.ca/news/what-moon-s-craters-reveal-about-earth-s-history-u-t-expert-and-lead-author-new-study.
- Tele Vue and the Moon Men from Philly! blog post.
- Return to the Moon with Michel Deconinck blog post.
- The Art of Sketching the Moon at the Eyepiece blog post.