Showing posts with label Moon. Show all posts
Showing posts with label Moon. Show all posts

Tuesday, April 1, 2025

Eyepiece cheat codes: Becoming a Lunatic

Most of us probably live in light polluted urban or semi-urban areas. My home usually exhibits a Bortle 8 sky at best (no hope of seeing the Milky Way and only the brighter constellations visible on a good clear night). We eagerly await the period around new moon so we can get somewhere darker and do some deep sky observing: galaxies, clusters, nebulae, hoping that we might have some clear nights.

We've all probably observed the Moon when it was up. But have we really observed it?

I am by no means an accomplished lunar observer, primarily because for many years, like many of us, I waited for new moon to do my observing. Now that I'm unable to get out to a darker sky as often, I have developed a new attitude toward our little rocky satellite, and I've discovered that lunar observing is pretty damn B A D A S S.

Having a 6-inch reflector as my current "go to" scope, I can't see many of the smaller features that someone with a 12-inch with consistently excellent seeing might see. Yet, given my limitations, I've found lunar observing to be something I look forward to as much, and sometimes more, than deep sky observing. 

[Want some Pink Floyd on YouTube to accompany you while you read this post? Click here.]

Pink Floyd - Dark Side of the Moon album art

Catch the excitement

When I was much younger, the race between the U.S. and the Soviet Union to put spacecraft and eventually people on the Moon was exciting for the general population, and even more so for space nerds like myself, whose favorite movie then (and now) was 2001: A Space Odyssey. Say hello again to HAL 9000.

Apollo 11 landing site from orbit
Now, with spacecraft once again landing on the Moon, some of that excitement is returning. Where are the landing sites? Where did the Apollo astronauts land? What are the various features visible in small telescopes? Can I see the flag on the Moon? (No, a flag is much too small to see in a backyard telescope. Buzz Aldrin saw the Apollo 11 flag blown over upon ascent from the lunar surface, but the other five flags planted in the Apollo program are still standing, although they may be quite faded and deteriorated from the ultraviolet light and temperature extremes. See this LROC explanation and this NASA evaluation for further discussion of the flags on the Moon.)

Above: The Apollo 11 landing site viewed by the Lunar Reconaissance Orbiter Camera showing the Lunar Module (LM) just left of center and several instruments left by the astronauts. The image is roughly 225 meters across, or about 738 feet. In comparison, an 8" telescope will only resolve details as small as about seven times the width of the image, or about a mile across, or half an arc second in perfect seeing. With a good Moon map, however, you can identify the general location of the various spacecraft landing sites. (NASA/GSFC/Arizona State University)


Get started being a lunatic

I recommend starting your lunar observing by simply perusing the surface, especially along or near the terminator—the line demarcating sunrise or sunset, where the shadows highlight the relief of the various features. Don't worry about names until you get curious. What is that crater with the long bright rays? How about that one with the straight radial line inside it? What is that U-shaped valley by that bright crater? What is that long cliff-like feature? How about that gap in that huge mountain range? Discovering these features on your own and then looking them up on a Moon map is part of the fun.


The ever-changing shadows

One of the many great things about lunar observing is that the view is continuously changing as the Sun's light marches across the Moon, with the terminator highlighting new vistas every night. One rule of thumb is that the period between new moon and full moon, centered on first quarter, will place the Moon best for observing in the evening sky, and the nights centered on last quarter will place the Moon best in the morning sky. First quarter in the first part of the night, last quarter in the last part of the night. In the evening, you'll be seeing sunrise marching across the Moon. In the morning, sunset.

You can look up the rise/set times and current phase of the Moon on many websites, including Time and Date. There are also many apps available, such as Moon Phase Calendar.



The importance of good seeing

With lunar observing, we really want to see detail as sharply as possible, with little to no blurring by the atmosphere. A night with steady air, or good "seeing," will yield more detail than a night of poor seeing when the Moon looks like it is rippling, undulating, or just plain fuzzed out. How do you know when the seeing will be good? Well, if you're like me and live under the jet stream, it won't happen very often that you get excellent seeing. But usable seeing can often be had. 

Check apps or sites like Astrospheric or Clear Dark Sky (R.I.P, Attilla Danko) for seeing predictions for your location, understanding that they are just predictions. Other factors can affect seeing, especially from urban locations where heat rising from streets, driveways, and roofs can turn an otherwise good night of seeing into churning soup. If your telescope needs some cool down time, typical for reflectors or SCTs, try to set it outside for at least 30 to 60 minutes and use a fan or insulation to reduce internal tube currents.


Charts and Moon map apps

While my favorite charting app, Sky Safari Pro, shows lunar features when zoomed in, I find it difficult to see in night mode, with the features just too dim. Since I do most of my observing of the Moon from home, I can hop indoors and check out the excellent (and free) Virtual Moon Atlas, which I highly recommend if you have a Windows or Linux operating system.  Once you set it up, it will show you where the terminator is currently, you can turn labels on or off, zoom in to an astonishing level of detail (thanks to Lunar Reconaissance Orbiter Camera imaging), look up information about various features, and even orient the view to match your telescope's. There are other apps available that you may prefer. Try Moon Globe for iPad, or the online Real Time Map of the Moon

Entire Moon view in the Virtual Moon Atlas
Left: Virtual Moon Atlas showing the phase on a particular date and time and set up for a 180 degree rotated image with south up and astronomical west to the left, as seen in a reflector. The Moon is about 31 arc minutes in diameter, or half a degree as seen from Earth. On the other hand, the Earth is about 2 degrees in diameter as seen from the Moon.



Note that when describing directions on the Moon, we use the convention of east being toward Mare Crisium, the circular dark plain just below center near the left limb in the image. This conforms with how terrestrial maps work, and is opposite from directions described for the night sky and deep sky objects. The idea was that lunar explorers would not get confused by "backwards" maps of the surface, compared to terrestrial maps. The crater Copernicus is on the terminator just below center.


Crater Copernicus from the Virtual Moon Atlas
Right: Zooming in on the crater Copernicus, which is about 58 miles in diameter. 37 mile-wide Eratosthenes is the crater in the lower left. The image is about 3.5 arc minutes wide.









Close up of Copernicus from the Virtual Moon Atlas
Left: Zooming in further into the interior of Copernicus. This image scale and detail is beyond the capability of most backyard telescopes. The image is about 25 arc seconds across.

The central peaks are almost 4,000 feet high, ,while the crater wall at left is about 13,500 feet high. The detached part of the central peak just to the right of center is about 9 miles wide, or about 7 arc seconds in the telescope.




Lunar features and naming conventions

Features on the Moon are labeled in Latin (and you thought it was a "dead" language!). These are based on names first proposed by Giovanni Battista Riccioli, an Italian astronomer and Catholic priest (hence the Latin) who lived in the 1600s. His Moon maps were drawn by Francesco Maria Grimaldi, his colleague and fellow scientist/priest. They both have large walled plains, close to each other on the western limb, named after them. Many features, mostly craters, have been named since then. For more on naming, see the Smithsonian Magazine's How are Places on the Moon Named?


Some of the main types of features include:

Mare Crisium
Mare ("sea"):
the expansive darker, smoother basaltic plains formed from molten rock that can be seen with the unaided eye. Examples: Mare Tranquilitatis (where the Apollo 11 astronauts landed), Mare Crisium, and Mare Imbrium.

Left: Mare Crisium (Virtual Moon Atlas. South is up.)
Sinus Aestuum
Sinus ("bay"):
A smaller plain similar to a mare. Similar smaller "maria" include Lacus ("lake") and Palus ("marsh"). Examples: Sinus Aestuum, Sinus Iridum, Lacus Lenitatis. 

Left: Sinus Aestuum, with craters Eratosthenes below center and Copernicus at right edge (Virtual Moon Atlas. South is up.)
Clavius
Crater:
95% of named features on the Moon are craters, almost all of which were caused by the impact of meteors or asteroids. They are named after dead scientists and explorers. Examples: Copernicus, Tycho, Clavius.

Left: Clavius, amid many other craters in the lunar southern hemisphere. This was the home of the fictitious moon base in the movie 2001: A Space Odyssey (Virtual Moon Atlas. South is up.)


Montes Apenninus
Mons/Montes ("mountain/mountain range"):
 These can be individual mountains or massive mountain ranges. Examples: Montes Apenninus (named after the Apennines on Earth), Montes Alpes (named after the Alps on Earth), Mons Piton (named after a peak in the Canary Islands).

Left: Montes Apenninus (Virtual Moon Atlas. South is up.)
Vallis Schröteri
Vallis ("Valley"):
Usually, but not always, named after a nearby crater. Examples: Vallis Schröteri, Vallis Alpes, Vallis Rheita.

Left: Vallis Schröteri. The deep crater to the left is Aristarchus. The valley's end points to the crater Herodotus. (Virtual Moon Atlas. South is up.)
Rima Hyginus
Rima/Rimae ("rille/rilles" or narrow channels):
These were mostly formed by lava flows, collapsed lava tubes, or grabens caused by the sinking of the surface between faults. Examples: Rima Hyginus, Rima Cauchy, Rimae Ariadaeus.

Left: Rima Hyginus. Crater Agrippa is in the upper left. (Virtual Moon Atlas. South is up.)
Rupes Recta
Rupes ("scarp" as defined by the IAU, but actually a fault looking like a huge cliff):
 Examples: Rupes Altai, Rupes Recta, Rupes Cauchy.

Left: Rupes Recta, the "Straight Wall,"  on the southeast edge of Mare Nubium (Virtual Moon Atlas. South is up.)

Dorsa Smirnov
Dorsum/Dorsa ("ridge/ridges"):
Tectonic features found in maria, these "wrinkle ridges" are long, thin folds formed by the cooled and solidified edges of lava flows. Examples: Dorsum Heim, Dorsa Smirnov, Dorsum Zirkel.

Left: Dorsa Smirnov, curving vertically down the center. The crater Posidonius is at bottom left. (Virtual Moon Atlas. South is up.)




Advanced lunacy

If you really want to get into all the details of the Moon's orbit, phases, libration, etc., check out NASA's Scientific Visualization Studio

For more ideas on lunar observing, and what others are looking at, see The Association of Lunar and Planetary Observers (ALPO) Lunar Section.

If you don't mind logging your observations in detail, you might consider joining the Astronomical League and trying out their Lunar Observing Program, which contains features to view with the unaided eye, binoculars, and a small telescope. Even if you don't log your observations to get the certificate, this gives you a list of prominent lunar features to observe.

Welcome to the lunatic asylum!

Man in the Moon


Saturday, October 12, 2024

3D Moon flyover

Full Moon with 3D label
I'm a big 3D fan, especially of stereogram pairs that require no special equipment to see. 

Here is a variety of images featuring different formations on the Moon in 3D. Seeing these from a new perspective adds to our understanding of what we observe in our telescopes. In this case, we are seeing them closer than we ever could from Earth, at differing angles, and in simulated 3D. 

These are stereoscopic pairs using the parallel viewing method. See the instructions for my 3D constellations for details on how to view these. With practice, almost everyone can learn to do it. It's worth the effort!

These images were taken by the Lunar Reconnaissance Orbiter Camera, which has been orbiting the Moon on the LRO since 2009. It has taken some spectacular images of the lunar surface, a few of which are reproduced here in 3D. All images are courtesy NASA/GSFC/Arizona State University. I created the 3D versions using Owl3D and created the location maps with Virtual Moon Atlas. Definitely check out the links to details of the images and browse the other incredible images on the LROC web site. If you have those cardboard anaglyph glasses, they have quite a few images in anaglyph 3D, although the 3D depth tends to be unrealistically exaggerated in some cases.

Many of these features can be observed with small backyard telescopes. The Moon's phase is critical, because features at or near the terminator, the line between night and day, are highlighted with long shadows and can be seen easier. Features near the limb, such as the crater Stevinus, can also be seen better when the Moon's wobble, or libration, presents it a little more favorably towards us. A steady atmosphere and a telescope adjusted to the ambient temperature is also very important. Of course, if a feature is on the far side, we won't be seeing it from Earth. 

Check out this cool NASA simulation to see how much the Moon varies in phase and libration throughout a year. You can also check out how the Moon will look now or at another time for the remainder of this year using NASA's visualization tool.


Unnamed crater between Lowell W and Mare Orientale

This 2.8 mile wide crater sits at the edge of the crater Lowell W and Mare Orientale on the Moon's far side. This was taken when the LRO was at an altitude of 47 miles, facing west. Not visible from Earth. See details about this image.

Stereoscopic pair of Unnamed crater between Lowell W and Mare Orientale









Location of the unnamed crater near Mare Orientale
Mare Orientale on the lunar far side. The arrow just below crater Lowell W points to the unnamed crater in the image above.













Aristarchus central peak

Aristarchus is visible in small telescopes, binoculars, and even with the unaided eye. It is often one of the brightest features visible because it is a young crater, 450 million years old, that hasn't had time for its ejecta material to darken. Here is a closeup crop of the central peak of the crater, taken by LROC from an altitude of 60 miles, facing west. The central peak is about 1,300 feet tall and 9,800 feet wide. The crater is over 2 miles deep. The best time to view Aristarchus is four days after First Quarter or three days after Last Quarter, but try for it around Full Moon and you'll see how bright it appears. See details about this image. 

Stereoscopic pair of Aristarchus central peak






Aristarchus is 25 miles in diameter. Here's another view. See details about this image.

Stereoscopic pair of Aristarchus










Location of Aristarchus
Location of crater Aristarchus in Oceanus Procellarum. South is up.













Messier crater

About 8.7 miles across, Messier is located in Mare Fecunditatis and may have been formed by a low angle impact, causing it's oblong shape. With an apparent size of nearly 7 arcseconds, Messier and its companion crater, Messier A, as well as the two small rays pointing east from Messier A, can be seen in small telescopes. The best time to view Messier is four days after New Moon or three days after Full Moon. See details about this image.

Stereoscopic pair of Messier crater

















Location of Messier crater
Location of Messier crater in Mare Fecunditatis. South is up.















Komarov crater floor (detail)

Located on the far side of the Moon, the floor of 53-mile-wide Komarov crater is covered with deep fractures created when magma rose from the mantle more than 2.6 billion years ago. The largest fractures are about 1,600 feet deep and 8,000 feet wide. Not visible from Earth. See details about this image.


Stereoscopic pair of floor of Komarov crater















Location of Komarov crater

Lunar Orbiter image of Mare Moscoviense with Komarov crater in the left foreground.















Mare Tranquillitatis pit

Pits are relatively small features that may have formed due to the collapse above a lava tube. They were first discovered in 2009 and over 200 have now been identified. The sharp edge of the opening of this pit is about 330 feet across, and the depth is estimated to be about the same. Computer modeling suggests the temperature in the shaded part of the pit may be relatively stable at about 63 degrees F, and there may be a more extensive cave or cave network. The pit is too small to be seen in backyard telescopes. See this article for details.

Stereoscopic pair of Mare Tranquillitatis pit






Location of Mare Tranquillitatis pit
Mare Tranquillitatis pit location. South is up.









Mound in Stevinus crater


A fractured mound inside Stevinus crater. This may have resulted from squeeze-up of molten rock in the impact that formed the crater. The mound is about 2 miles wide. Stevinus can be seen in small telescopes, although our view is at an angle, Stevinus being near the Moon's southwestern limb. The central peak can be spotted. The mound is only about 1.6 arcseconds in diameter and may just barely be detected in some amateur images. The best time to observe Stevinus is three days after New Moon or two days after Full Moon, with a favorable libration. See details about this image.

Stereoscopic pair of Stevinus mound


















Location of Stevinus crater
Location of Stevinus crater. South is up.







Location of Stevinus dome
Location of the dome within Stevinus crater. North is up.













Wallach crater

Wallach is located in Mare Tranquillitatis. The asteroid or comet that hit the basaltic surface stirred up brighter material from underneath. Wallach is about three miles in diameter. This image was taken from an altitude of about 58 miles. A small telescope with good seeing can pick it out from the mostly flat floor of the mare using higher powers. The best time to observe Wallach is five days after New Moon or four days after Full Moon. See details about this image.


Stereoscopic pair of Wallach crater

















Location of Wallach crater
Wallach's location in Mare Tranquillitatis. South is up.













Hell Q crater


One of the many satellite craters (smaller craters near a named crater) named after Hungarian astronomer Maximilian Hell, Hell Q is a very young crater only about 2 miles in diameter. At only 1.8 arcseconds in apparent size, Hell Q requires a 6-inch or larger scope with higher power. The best time to observe it is one day after First Quarter or Last Quarter. See details about this image.


Stereoscopic pair of Hell Q crater

















Location of Hell Q crater
Hell Q location. The crater Tycho is just above  center on the right, near the Terminator. South is up.











Tycho

The 53-mile-wide crater Tycho has a large and prominent ray system. This oblique image was taken from an altitude of about 37 miles. The west wall on the far side in the image is more than 14,000 feet high. Tycho is an easy target in any telescope, best observed one day after First Quarter or Last Quarter. The bright rays are most prominent around Full Moon, however. See details about this image.

Stereoscopic pair of Tycho crater











The central peak of Tycho. The image is about 3/4 of a mile wide. The boulder on top is about 100 yards wide. See details about this image.

Stereoscopic pair of central peak of Tycho crater


















Lichtenberg B

Lichtenberg B is a young three-mile-wide crater located in Oceanus Procellarum. The ejecta darkens over time, so the presence of bright ejecta is an indicator that the crater is relatively young. Lichtenberg B can be spotted with small telescopes. Being very close to the northeastern limb, it is best observed six days after First Quarter or five days after Last Quarter using higher powers. See details about this image.

Stereoscopic pair of Lichtenberg B crater








Location of Lichtenberg B crater
Lichtenberg B location in Oceanus Procellarum













Earth over Compton Crater

Taken at 83 miles altitude, the Earth appears over the far side crater Compton. See details about this image.

Stereoscopic pair of Earth over Compton crater