Sky Events

2022: Year-End Events!

In the northern hemisphere, rapidly lengthening night at the expense of daylight is a clear reminder that the year is drawing to a close. However, 2022 still has some noteworthy astronomical events in its final two months.

Sun and Moon

Lunar Eclipse
On November 8th, there will be a total lunar eclipse when the Full Moon travels through the Earth’s shadow. First, it passes through the faint shadow of the Penumbra, then through the dense Umbra (see illustration below) where the darkened Moon can appear with reddish hues. This coloration has given rise in recent years to the phrase blood moon which is used to describe totality while in the Umbra. In reality, the reddish color comes from the sunlight that passes through Earth’s atmosphere at a low angle and gets refracted into the Umbra. In other words, it is the deep-red light we see during sunrise and sunset hitting the shadowed lunar disk.

Lunar Eclipse diagram showing the Moon passing through penumbra and umbra shadows cast by the Earth. The red wavy lines are deep-red rays refracted by Earth’s atmosphere into the Umbra and onto the lunar disk. Credit: NASA.

This lunar eclipse is centered on the vast Pacific Ocean. The total phase will be visible from eastern North America to Central America through to 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.

The most dramatic eclipse phases are when the Moon enters, resides in, and exits the Umbra. The diagram below maps the visibility of each phase of the eclipse to the geography of the Earth. For example, in the central dark area no eclipse is visible. In the white areas, on the extreme left and right of the diagram, all phases of the event are visible. Shaded regions indicate geographic visibility of phases. Phases begin and end at moonset (left of the dark zone) and moonrise (right of the dark zone). For example, the line “U3” that runs through Central America, the tip of Florida, the coast of the mid-Atlantic states, New England, and eastern Canada indicates that anyone on that line will not see the Moon exit the Umbral shadow because that phase happens at moonset. On the other side of the world, the same “U3” line that runs through India, Western China, Kazakhstan, and Russia indicates that anyone along that line will see the Moon exiting the Umbra at moonrise.

Total Lunar Eclipse 2022 Nov 08 visibility. P1/P4 = first/last contact of Earth’s Penumbra with Moon (this is barely visible). U1/U4 = first/last contact of Earth’s Umbra with Moon (a “bite” is taken out of Moon). U2/U3 = begin/end of Total Eclipse (the blood moon).

Eclipse Fireballs
As a bonus, look out for fireballs in the sky during the lunar eclipse on November 8th. Meteor researchers say that the normally languid Southern Taurid Meteor shower perks up periodically and produces a swarm of meteors and bright fireballs. (Since the Moon will not be bright enough to blot these out, you can look for fireballs nightly on either side of the November 5th peak). During the umbral (totality) phase of the November 8th lunar eclipse, the sky will darken enough to show dimmer meteors from the shower as well as the fireballs. But don’t forsake the Moon for the fireballs: Taurids may hit the Moon and produce a flash. You’ll want to make a video record of the Moon while observing it through a telescope to confirm the impact. For lunar impact detection software to analyze your video, see this article on the Sky & Telescope website. For more information on the Taurid shower and fireball predictions, see this page on the International Meteor Organization website.

The last “Micromoon” of the year, when the Moon becomes full near the point of its orbit furthest from Earth (Apogee), will be on December 7th (8th UTC). If you photographed a “Supermoon,” a Full Moon near its closest point to Earth (Perigee), earlier in the year (June 14, July 13, or August 12) this will be your last chance to take a comparison photo to show the size difference.

A “supermoon” looks bigger than a “micromoon” (when the full moon is at apogee) because it’s about 40,000 kilometers closer to Earth on average. Credit: NASA/JPL-Caltech

Tele Vue Refractors for Astronomical Events

A scope you can quickly set up and take down, without having to install and align accessories, gives you more time for observing the events on this page. 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. This eliminates the need for installing a finder. Instead, use our unit-power StarBeam (mobile site) with flip-mirror to comfortably aim the scope in the vicinity of the object you are searching for.  

From the powder-coated tubes and anodized aluminum finishes to the silky-smooth, lash-free focusing, these scopes are rugged and easily transported to dark-sky locations. Tele Vue telescopes are engineered and built to be your lifelong observing companions; and someday, your kids’ as well.  All Tele Vue telescopes come with a 5-year Limited Warranty.


At Opposition, Earth and a planet are on the same side of the Sun. Courtesy NASA/JPL-Caltech.

Planets in opposition are in the sky opposite the Sun when viewed from Earth. They rise at sunset and are in the sky all night. Around opposition, the planets are closest to Earth and at their brightest. This makes opposition an opportune time to view and image a planet. Note that only planets further away from the Sun than Earth can be in opposition (diagram right). Opposition season started in August with Saturn and continued in September with Neptune and Jupiter. After a break in October, we’ll see Uranus enter opposition on November 9th and Mars on December 8th.

As an inner planet, Mercury will never be in opposition. It stays near the Sun and is often hidden by the solar glare. However, there are times when it is better placed for viewing. These are called “elongations.” December 21st finds the elusive planet Mercury a little over 20° east from the Sun at sundown. This is known as “greatest eastern elongation” and is a good time to view the planet. Beware: the bright magnitude -3.9 object that emerges in twilight that evening is actually Venus. It will appear closer to the Sun than Mercury. Mercury will be the dimmer, but still bright magnitude -0.45 that follows the path of Venus toward the Sun.

Nagler 3-6 Planetary Zoom.

Your Opposition and Elongation Eyepiece!

The Nagler Zoom was conceived as the ideal planetary eyepiece.  Like all Tele Vue eyepieces, it’s designed for full-field sharpness in any speed telescope, as well as high contrast and transmission with natural color rendition, low scatter, and comfortable eye relief. Use it to fine-tune magnification for the seeing conditions — no need to swap eyepieces to find the highest usable power. It’s parfocal through the zoom range, maintains its eye relief and has click-stops for each focal length.  Its constant 50° apparent field of view makes it more appropriate for scopes on tracking mounts. Read more about it on our website Nagler 3-6-mm and (mobile site).

It is excellent for turning up the power to confirm that you’ve sighted an ice-giant planet like Uranus or Neptune and not a field star. With just a flick of the finger, you can continuously vary the focal length from 6mm down to 3mm with click-stops along the way at 5mm and 4mm focal length settings.  

Images from the Recent Jupiter Opposition
The Jupiter Opposition in the last week of September had many imagers working the planet as Pierre Gilet did with his capture of Jupiter with Great Red Spot during the transit of the moon Io across the face of the planet (left below). This was also the best time to see details on the major Jovian moons. In Pierre’s image, below at right, contrasting topography and color is visible on the four major Jovian moons. Amazingly, this image was shot when the Earth was 591 million km from the targets! With diameters ranging from 3122 km for Europa to 5268 km for Ganymede, Earth’s Moon, at 3475 km in diameter, would be between Europa and Io in size. If our Moon was transported to the Jovian system it would appear very grey and boring to us compared to the other major moons.

Left: Jupiter and Io Transit on 18 October 2022 and Right: Galilean Moons of Jupiter. Both images by Instagram user Pierre Gilet. All rights reserved. Used by permission. Skywatcher 254mm / 1200 PDS Newtonian with Tele Vue 5x Powermate amplifier, Baader IR/UV cut filter, and Omegon Atmospheric Dispersion Corrector into ZWO ASI385MC camera all carried on EQ6-R Pro Mount.

Tele Vue’s Powermate Amplifiers for Planetary Oppositions

Powermates come in 1¼” (2.5x & 5x) and 2″ (2x, & 4x).

Attempting to image a planet at opposition? Just sticking a camera at the end of your longest focal length scope will likely produce tiny images. In order to capture detail on planets at Opposition you’ll need at least 3- to 6-meters of effective focal length. That’s where Tele Vue’s line of Powermate™ image amplifiers can give your telescope a boost.

Tele Vue’s Powermate line has some distinct advantages over simpler Barlows for visual and imaging. Powermate™ photo / visual amplifiers increase the focal length of your scope with reduced aberrations, greater magnification potential, and compact size compared to typical Barlow lenses. Also, Powermates™ can be stacked with no adverse impact. Powermates are available in different barrel sizes and powers to meet your mission needs: 1¼” (2.5x & 5x) and 2″ (2x, & 4x) formats.

Imaging with Powermates is easy: either put a camera nosepiece into the visual barrel or unscrew the visual top to attach an optional Tele Vue Powermate T-Ring Adapter accessory to allow camera attachment with T-threads.

Read more on our Powermate page (mobile site).

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 #jupiter

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