Our monthly meetings are free and open to the public. You can attend in person or online
This month’s speaker will be Larry McHenry, giving a presentation on “The Local Group of Galaxies (What are they, and How to Observe Them)”.
Larry will discuss what he’s learned during his observing ‘journey’ among the Local Group. He’ll review what are galaxies in general and what is the Local Group and its place in the universe, along with some of the people, both historical and modern, behind these objects, and how to go about observing them.
Larry has been active in amateur astronomy for over 40 years, and is a member of the Kiski Astronomers, and the Oil Region Astronomical Society (ORAS) in Western Pennsylvania.
Directions: Our meeting in a condo association club house. The street address is 10748 Independence Dr, North Royalton, OH. Drive all the way to the end of the drive, about a half mile from the street. You can park next to the club house or on the street.
CAA member Frank Shoemaker, despite challenging seeing conditions and the early hour, captured a fine image of the September 14 conjunction of Earth’s Moon and planet Venus. As luck would have it, the conjunction occurred in constellation Cancer home of the lovely open cluster M44, the “Beehive”. The technical info.: Canon EOS 6D Mark 2, 100mm, f/4.5, 19 seconds, 5:29 a.m. Eastern Daylight Time.
Saturn is truly the lord of the rings in this latest portrait from NASA’s Hubble Space Telescope, captured on July 4, 2020, when the opulent giant world was 839 million miles from Earth. This new Saturn image was taken during summer in the planet’s northern hemisphere.
Hubble found a number of small atmospheric storms. These are transient features that appear to come and go with each yearly Hubble observation. The banding in the northern hemisphere remains pronounced as seen in Hubble’s 2019 observations, with several bands slightly changing color from year to year. The ringed planet’s atmosphere is mostly hydrogen and helium with traces of ammonia, methane, water vapor, and hydrocarbons that give it a yellowish-brown color.
Hubble photographed a slight reddish haze over the northern hemisphere in this color composite. This may be due to heating from increased sunlight, which could either change the atmospheric circulation or perhaps remove ices from aerosols in the atmosphere. Another theory is that the increased sunlight in the summer months is changing the amounts of photochemical haze produced. “It’s amazing that even over a few years, we’re seeing seasonal changes on Saturn,” said lead investigator Amy Simon of NASA’s Goddard Space Flight Center in Greenbelt, Maryland. Conversely, the just-now-visible south pole has a blue hue, reflecting changes in Saturn’s winter hemisphere.
Hubble’s sharp view resolves the finely etched concentric ring structure. The rings are mostly made of pieces of ice, with sizes ranging from tiny grains to giant boulders. Just how and when the rings formed remains one of our solar system’s biggest mysteries. Conventional wisdom is that they are as old as the planet, over 4 billion years. But because the rings are so bright – like freshly fallen snow – a competing theory is that they may have formed during the age of the dinosaurs. Many astronomers agree that there is no satisfactory theory that explains how rings could have formed within just the past few hundred million years. “However, NASA’s Cassini spacecraft measurements of tiny grains raining into Saturn’s atmosphere suggest the rings can only last for 300 million more years, which is one of the arguments for a young age of the ring system,” said team member Michael Wong of the University of California, Berkeley.
Two of Saturn’s icy moons are clearly visible in this exposure: Mimas at right, and Enceladus at bottom.
This image is taken as part of the Outer Planets Atmospheres Legacy (OPAL) project. OPAL is helping scientists understand the atmospheric dynamics and evolution of our solar system’s gas giant planets. In Saturn’s case, astronomers continue tracking shifting weather patterns and storms.
Comet C/2020 F3 (NEOWISE) was the finest comet to grace the skies of the Northern Hemisphere in quite some years. Amateur astronomers and photographers the world over made fascinating observations and beautiful images of the comet and its surprisingly long tail. By July 5, NASA’s Parker Solar Probe had captured an image of the comet, from which astronomers also estimated the diameter of the comet nucleus at approximately 5 km. or about three miles; that’s a reasonably large size but around average for a comet. The large nucleus offered plenty of volatile materials for the Sun to stir into tail formation.
On July 23 the comet reached perigee with Earth and is now speeding toward the outer Solar System, not to revisit the inner planetary neighborhood for several thousands of years. So, though relatively near Earth the object is fading fast. Lately astronomers and astrophotographers have been grabbing the last views they will have of C/2020 F3 before it fades to obscurity.
Here are some photos made by members of the Cuyahoga Astronomical Association (CAA) as a cometary farewell of sorts:
Alan Studt’s lovely portrait of the comet shows its tails remain, if faded, long and expansive. He wrote, “Beautiful night by the lake last night. Took these at Veteran’s Memorial Park in Avon Lake just before 11 p.m. Pretty large group of people hanging out. The comet was definitely much dimmer than the previous Friday.”
Technical Information: Tamron 70-200mm f/2.8 lens, on a Nikon D850. The comet image is made from 14 shots (2.5 seconds, ISO 10,000, at 200mm, f/2.8). Stacked in Deep Sky Stacker & post processed in Lightroom and Photoshop. Seventy-five shots but got the best star field alignment using only 14 shots. Also used dark & flat frames.
James Guilford was at Letha House Park, July 24, attempting to record detailed images of the comet nucleus and close tail. The green coloration of the comet was a surprise to him, even after reading the observations of others. “All of my comet shots Friday night show a green nucleus,” Guilford said, “and it grew brighter as I processed the images later. I’d have liked to have picked up more of the tail but, given the circumstances, I’m pretty happy with what I got.” Both he and other Letha House Park observers could see a green tint by eye through telescopes. He and others also report the comet was barely within the range of eyesight but only at its highest above the horizon and only via averted vision.
Technical Information: Canon EOS 6D Mk. 2, at prime focus of 1800mm FL Cassegrain telescope, eight light exposures plus darks, ISO 1250, 15 seconds per exposure, stacked in Starry Sky Stacker, processed in Photoshop.
Jon Salontay also photographed the comet that Friday. Above we see how it is nearly lost, even to the camera, amongst the stars. Technical Info.: Time – 11:32 p.m., Canon T5i with 18-75mm zoom lens at 18 mm, exposure 30 seconds at F/5.6, ISO 800. Brightness & Contrast adjusted.
Salontay then turned his telescope on the “dirty snowball.” Technical Info.: Time – 12:13 a.m., July 25. Celestron 8-inch SCT on Advanced VX Mount, Canon T5i, 15 seconds, ISO 1600. No out-of-camera adjustment.
He wrote, “Although I’ll try to follow it telescopically over the next month, how about another comet before the year is out? It’s a lot of fun.”