Tele Vue Optics has been the key to unlocking the limits of magnification.
In the last installment, our scientific path went from “polar to solar.” (If you missed it, please go back and read Tele Vue Scientific Part 1.) In Part 2 of this multi-part blog post on the use of Tele Vue gear in science, we reveal Sneakey research with Tele Vue Powermates and how a compact Tele Vue-NP101is telescope proved once again that lights are “all askew in the heavens.” All this research was done using our standard gear with products bought off-the-shelf — the same as you would receive from Tele Vue.
Sunspots 25 Nov 2020 by flickr user Antonio Agnesi. All rights reserved. Used by permission. The image was captured through a Tele Vue Ranger refractor with Celestron Ultima 2x Barlow and Lunt Herschel wedge with Baader Solar Continuum filter. The camera used was a ZWO ASI 120MM. All gear was carried on a Skywatcher AZ-EQ6 mount. Exposures 5ms and the best 120 frames were stacked. macOS software used was ASICap, Lynkeos, and Photoshop CC.
According to a recent Solar Activity Update by the National Oceanic and Atmospheric Administration (NOAA) Space Weather Prediction Center, “Solar activity picked up at the end of November into early December, 2020, as several sunspot groups emerged or rotated onto the visible disk”. The update continues: “Solar activity is anticipated to slowly increase over the upcoming years towards the predicted solar maximum peak around July, 2025.” This is great news for observers of our nearest star! At times this year, there had been month-long sunspot “droughts” with no or few sunspots on the solar disk.
The return of Sun as a target of interest has led to a sudden uptick in Solar image postings to social media these past few weeks.
A detailed look at sunspots 2785 and 2786 by Instagram user Michael Harriff. All rights reserved. Used by permission. Taken on 29 November 2020 in Hydrogen-alpha light ─ “This was the only clear shooting day in several weeks! 😩”. A Tele Vue 4x Powermate on a Lunt 80mm MT refractor allowed the system to reach 2,240mm effective focal length for this close-up shot. The camera used was the ZWO ASI174MM (mono).
Proms Mono by flickr user Paul Andrew. All rights reserved. Used by permission. Lunt LS152 Solar Telescope (obj: 152mm / fl: 900mm) with Tele Vue 2.5x Powermate and imaged with ZWO ASI290MM monochrome camera (1936px x 1096px, color added in post-processing). Taken 20th May 2020 from Kent, UK. Solar prominences dance along magnetic field lines on the limb of the active Sun while fibrils of super-heated plasma fill the foreground.
Paul Andrew has been an amateur astronomer since the age of 11. He is the founder and Honorable President of the South East Kent Astronomical Society in the UK. He’s had a number of his astrophotographs published — in particular, his solar images — in national newspapers and on websites as far afield as Russia. He’s been short-listed for the prestigious Insight Astronomy Photographer of the Year competition four times now. We’ve noted his high-quality solar images and discovered that many were made with our Tele Vue 2.5x Powermate in the imaging train. So, we present a selection of his work in this week’s blog.
Mercury Transit 2019-11-11 Time 10-03-50-0631 by flickr user Photon_chaser. Copyright Frank Tornyai. Mercury is about to leave the face of our Sun. Hα image through Wollensak 153/1200 achromat using Quark Chromo with Tele Vue 4x Powermate™ using Lunt double stacked etalons, and ASI174 mono camera. Software used was Genika Astro capture, PIPP, AS!3 , Images Plus and Photoshop.
Images from the 2019 Mercury Transit made with Tele Vue gear have now been posted to social media. We present here the best (with permission) and note that Tele Vue Powermate™ amplifiers “shone” in the creation of most. Not only does Powermate™ help fast, modern scopes achieve a focal length suitable for imaging the tiny planet, but some high-end, drawtube-side, narrow-band filters requires a Powermate’s telecentric operation to create parallel rays for best image contrast. (See Daystar application of Rear-Mounted Filter page).
Uranus and moons. Celestron Edge 11 with 2.5x Tele Vue Powermate and ZWO ASI224MC color camera. Image credit and copyright by Anis Abdul.
Anis Abdul’s composite image of Uranus and moons is from the October 2017 opposition and was posted to his Facebook page. The imaging gear used was a Celestron Edge 11 telescope, riding on on AP900 mount, that was “amplified” with our Tele Vue 2.5x Powermate to achieve 7,000 mm focal length. Imaging was done with a ZWO ASI224MC color camera . The best 50% of frames from 20-minutes of video were processed for the image. Software used was Pixinsight and Registax.
“One of the closer moon (Miranda) is actually visible in my stacks but is lost in the planet glow ,” says Anis.
The “ice giant” planet Uranus was in opposition on October 28th. That means that the Sun, Earth, and Uranus all lined up together at an instant in time on that date. Uranus is on the same side of the Sun as the Earth, so the planet was closest to Earth and brightest for the year and in the sky all night long. If you missed it: don’t worry. The slow-moving planet will remain at least 3.7″ of arc in diameter and at magnitude 5.7 for the next month.
protuberancias y superficie solares – 18/11/2017 by flickr user Jordi Sesé. All rights reserved. Used by permission. In this impressive image, a massive solar prominence erupts above the limb of the Sun. Furry spicules are visible along the entire edge of the disk. The roiling surface appearance of the Sun is caused by filaments and fibrils (prominence and spicules away from the limb — see blog text for details). All these solar features are usually invisible in ordinary white light. These phenomena are only revealed through narrow-band hydrogen-α light filters. Tele Vue 2.5x Powermate™ into ZWO ASI174MM monochrome camera using 100mm f/10 achromatic scope with modified Coronado PST Hα and BF10 blocking filter.
If you’re suffering from the cold northern winter like we are at Tele Vue headquarters in upstate New York, you’ll instantly be “warmed” by these “hot” solar images made by Jordi Sesé Puértolas from his balcony in Barcelona, Spain. These photos appear to show a blazing inferno on the “surface” of the Sun. However, science tells us this is not fire we are seeing but hot plasma (ionized gas) and gas in the wavelength of Hydrogen-α light.
Uranus by Instagram user astrobobo. Copyright astrobobo. Used by permission. Imaged with Tele Vue 2.5x Powermate™ on Celestron EdgeHD 8″ SCT (effective focal length = 5080-mm) and ZWO ASI290MC camera.
On the 23rd, the “ice giant” Uranus will be visible all night, as it rises when the sun sets (hence it is opposite the sun). It will also be at its largest for the year: a diminutive 3.73″ of arc. Due to its distance and close-to-circular orbit, Uranus doesn’t vary that much in brightness over time. It will reach magnitude 5.7 from mid-October through early November before slightly fading to magnitude 5.9 in late March 2019. This makes it a naked-eye target in dark skies and easy to locate in a binocular or finderscope.
Air China A332 crossing the Moon (crop) by Instagram user Kacper Lechwar. Copright Kacper Lechwar. Used by permission. Air China Airbus A330-243 is captured poking its nose into the Sea of Serenity as it crosses the face of the Moon. Imaged using 254mm / 1200mm Dobsonian telescope with Tele Vue 2x Powermate™ and Canon 1200D / EOS Rebel T5 (18.1-megapixel) camera. Shot at cruising altitude (30,000+ feet). With this Powermate™ setup, Kacper takes a series of images in quick succession of each plane. He then reviews them on a computer before processing the best ones. Click to see full image.
We’ve noticed a proliferation of close-up plane images on Instagram made using Tele Vue Powermate™ image amplifiers. What is amazing about these images? They are taken from the ground with the plane at jet-aircraft cruising altitude. This is the imaging side of the hobby of “plane spotting.” It is sort of like bird watching — but the “bird” is much bigger and potentially much further away: in the stratosphere!
While imaging a bird can be serendipitous, the modern plane spotter has the advantage of free online flight-tracking software, such as FlightRadar 24 and FlightAware, to predict what aircraft are approaching their location. Aircraft identification, route, speed, altitude, and heading are just a click away. This software has also made its way to the ubiquitous smartphone. Thus, unlike birding, plane spotters can anticipate targets to observe in advance. This gives the spotter time to prepare for encounters with common and rare aircraft — like the Antonov An-225.
Saturn is in opposition tonight: it glides above the horizon around sunset and will be over 18-arc-seconds in diameter for a few weeks. At about magnitude 0.0, it will pair well with the full moon that accompanies it across the sky this evening.
Galileo’s telescopic sketches of the moon from “Sidereus Nuncius” published in March 1610. Animation created from public domain images obtained from Wikimedia Commons.
The changing face of the moon has long been documented by artists. In the early 1600s, the introduction of the telescope allowed for detailed sketching of lunar features at the eyepiece. The most celebrated early telescope sketcher was Galileo Galilei. His artistic training allowed him to understand that the jagged appearance of the lunar terminator (day/night line) seen in the eyepiece was due to the topography of craters, mountain, and ridges on the moon. These irregular shadows on the moon had puzzled earlier observers that considered the moon to be a flat disk with markings on it.
Copernicus Crater by AstroBin user Tanglebones. Copyright by the artist. Used by permission. Tele Vue Panoptic 35mm eyepice with Tele Vue 2x Powermate using Sky-Watcher Mak 180 Pro scope.
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