Webb’s Wreath: Asterism In Hercules

Posted July 17, 2025 by rogerivester
Categories: Uncategorized

Posted July 17th 2025

From “Deep-Sky Wonder’s” By Sue French:

“Moving back to Omicron and dropping 2.7º south-southwest takes you to a golden 7th magnitude star. It ornaments the eastern side of Webb’s Wreath, a little-known asterism first mentioned in the 4th edition (1881) of Thomas Webb’s observing guide “Celestial Objects for Common Telescopes.”

My 105mm scope at 68x reveals 13 additional stars, magnitudes 11 and 12, outlining 11′ x 7′ oval leans northeast and is dented inwards at the bright star.”

RA: 18h 02m Dec. +26 18m

6-09-01: Telescope 105 mm Apochromatic refractor; 610 mm focal length, and a 9 mm Nagler eyepiece for a magnification of 68x.

Pencil Sketch by Sue French as following: The following sketch was made using my 105 mm refractor with the employ of a diagonal.

Images by Mario Motta:

Using my 32-inch telescope, I imaged Webb’s Wreath in RGB and Lum, subtle colors. The images as following present the Wreath with north is at the top and west to the right.

The following image identifies very faint galaxies inside and around the wreath.

Can you still spot the galaxies in the following image?

Observer’s: Keith Rivich and Larry Mitchell

Location: ~10 miles SE of Leakey, Texas

Telescope:  25-inch f/5 Newtonian

SQM-L:   21.3

Seeing:  4 of 10  (Seeing pretty much was limited to around 300x, however, could occasionally go higher.)

Transparency:   10 of 10   

Webb’s Wreath itself is a worthy target. My 20 mm Nagler eyepiece framed the wreath quite nicely looking a bit like a lop-sided potato. Larry was going to check GAIA to see if any of these stars may be related. Except for the 7th mag star the rest look suspiciously similar. 

UGC 11097: 

This galaxy was just out of the frame in the (Mario Motta’s image) but I used it as my star hop base, so I will go ahead and mention the observation. Easy to see at mag. 14.5 with a pretty high surface brightness. Its 1.2′ x .3′ nearly N-S elongation was obvious being brighter in the center and tapering off towards the ends of the arms. A couple of 15th mag stars bracket the galaxy.

PGC 61289 (MCG +4-42-22)

This is the brightest of the galaxies in the Motta image. As suspected at mag 14.6 it was quite easy to see, appearing as a very small oval glow. A mag 14 star sits just off the galaxies northern edge.

2MFGC 14178 (in the image as PGC 1768412)

As suspected this one was tough and fun. When the field first slid into view I strongly suspected I could see some elongation at the right spot. Looking at images there is a 15th mag star just 20″ east of the core of the galaxy, which is depicted as a 14th magnitude “non-star” in Megastar. These two “stars” could easily mimic the elongation I was seeing. I bumped up power to 650x and during moments of good seeing I could distinctly see the arm of the galaxy opposite the 15th mag field star. I called Larry over to take a look and he was seeing what I was seeing. As a bonus he knew nothing about the galaxy before looking. 

For the fun part of the observation we put Larry’s NVD into the scope. He had it mated to a 27mm eyepiece so the magnification was quite low. We suspected the NVD devise should work as the galaxy is infrared bright, and we were right. The 15th mag field star was dramatically reduced in brightness so the galaxy, though tiny, was just visible as a complete edge on spiral. The dark lane visible in high res images was not visible to us. 

LEDA 1772537 (in the image is listed as a PGC):

As suspected nothing. Nada. Not even a sparkle!

UN-NAMED FACE ON SPIRAL:

We couldn’t see anything of the galaxy, no surprise there, but we could see the 17.5 mag star that sits on the NE edge of the spiral. 

Observer: Roger Ivester (North Carolina)

The following pencil sketch was made using a 10-inch f/4.5 EQ Newtonian with an 11mm eyepiece, apparent field of 82º. Magnification: 104x and field-of-view of 0.79º which was a perfect framing for the asterism.

As a follow-up on the four galaxies in and about Webb’s Wreath, they were partially featured in Stephen O’Meara’s column in the May issue of Sky & Telescope (p. 12).  Keith’s and Larry Mitchell’s earlier observations of PGC 61289 and PGC 1768412 with Keith’s 25″ were discussed in the article.  O’Meara also mentioned the two fainter galaxies within the Wreath itself “most likely require even larger apertures to detect.”  One of these is PGC 1772537, an E- or S0-type, and the other is a spiral not catalogued in LEDA (PGC).

Webb's Wreath.jpg

The following is a Cloudy Nights post by expert big scope “visual” observer, Steve Gottlieb

Larry Mitchell also included Webb’s Wreath and its galaxies in the Texas Star Party’s “Advanced Observing” list, just a week ago.  When Larry came over last Thursday to observe on Jimi Lowrey’s 48″ f/4.0, he requested to look at Webb’s Wreath again to search for the two dim galaxies within the Wreath.  Also observing with Jimi and I were Stephen O’Meara, Brent Archinal (from Lowell Observatory), and Doug McCormick (from Houston).

When we observed these galaxies at the end of the observing session, the background sky was jet black in the eyepiece (excellent contrast) and the stars pinpoint at 610x. The unnamed face-on spiral (NED lists the infrared designation WISEA J180231.28+262057.6) was immediately seen as a faint, very small glow, perhaps 10″ in diameter.  Although it was fairly easy to see, the visibility may have been enhanced by a faint star at the NE edge.

PGC or LEDA 1772537 was easy to pinpoint, as it lies at the midpoint of a mag 10.8 star 40″ SW and a similar star 40″ NE (two of the main stars in the Wreath).  At 610x it was very faint and quite small, perhaps 5″ diameter, but definitely non-stellar. I may have just been seeing the core region of this galaxy.  Checking later, I noticed that HyperLeda lists a B magnitude of 17.93 ± 0.50 and NED list a single redshift at z = 0.192.

So, there’s two things interesting about LEDA 1772537.  It lies precisely along the Wreath, and if the redshift is accurate, the light of this E or S0-type galaxy has been traveling for 2.4 billion years! (using H0 = 70).  

Steve Gottlieb

Galaxy NGC 5958 In Corona Borealis: Visible With A 10-Inch Telescope, But What About From A~4.7 NELM Suburban Backyard? June 17th 2025

Posted June 7, 2025 by rogerivester
Categories: Roger's Articles

For the past few months while watching T Corona Borealis, I didn’t realize there was a potential “observable galaxy” using a 10-inch telescope” and fairly close to the novae star:  But, what about a 10-inch from a magnitude ~4.7 NELM location. (?)  However, due to the “high-surface brightness” it just might be possible, but very doubtful.  

The following information from the “Observing Handbook and Catalog of Deep-Sky Objects” by Christian Luginbuhl and Brian Skiff:  

“…galaxy is very small and unconcentrated, but of high surface brightness.  In 25 cm it is circular, about 35 arc second diameter, with a faintly granular texture.” L&S

Interesting to note: This galaxy is not listed in either the Herschel-400 or the H-2 lists.  I’m wondering if it would be more difficult than galaxy NGC 6118: Which is considered by “most all” amateurs to be the most difficult object in the Herschel-400 list. This galaxy (NGC 6118) was “very, very difficult” for me from my suburban backyard, taking me several observing sessions over a couple years.

Note: For those with a 12-inch telescope, galaxy NGC 5961 can be observed using a 12-inch telescope. This is the second of only two deep-sky objects listed in the Luginbuhl and Skiff Observing Handbook.

Galaxy NGC 5961: “Though it is a small moderately faint object for 30 cm, this galaxy has a high surface brightness.” L&S

If I have a very clear night with excellent transparency, I might give NGC 5958 a try with my 10-inch f/4.5 EQ Newtonian. A clear and transparent night during the summer months is very rare for me, observing from the foothills of North Carolina. Due to increasing light pollution and glow on my best nights I can hardly achieve ~4.7 in a winter sky!

What is a magnitude ~4.7 NELM (naked eye limiting magnitude) and how was it derived?

This is the longtime system used by many “mostly” visual observers, using the stars of the little dipper to determine the faintest star that can be seen naked eye.

I learned this from an Edmund Scientific (Sam Brown books) many years ago, and have been using the NELM system for more than 40 years. However, since the sky glow from the horizons is growing from light pollution, I sometimes (on nights) for reasons might add 1/2 magnitude to my NELM near the zenith.

My backyard Bortle scale number is ~6.5-7.0 which has increased over the past 40 years, as most all backyards in America.

The Bortle scale puts my (NELM) naked eye limiting magnitude at about 4.7-4.8 on a good night, which corresponds pretty close to the Bortle scale.

However, during the summer months, with high-humidity, heat and haze, my NELM sometimes will hover around 4.0 or even less! Defintely not good nights to attempt faint galaxies or nebulae, but can be excellent nights for viewing double and multiple stars.

I’ll never forget the days of growing up in the country and seeing the Milky Way glowing overhead, and extending “seemingly” almost to the southern horizon.

A 6-Inch f/6 Newtonian Just Might Be The Perfect Telescope For Visual Observing With 2x The Light Gathering Power Of A 4-Inch Refractor But Still Very Portable

Posted April 26, 2025 by rogerivester
Categories: Uncategorized

Yes, the 6-inch f/6 Newtonian in my opinion, just might be the perfect telescope for the dedicated visual observer. It’s both compact and lightweight, and even with an equatorial mount is easily manageable, and has twice the light gathering power of a 4-inch refractor.

I had a 6-inch Criterion RV-6 almost 50 years ago, but life got busy and sold it. However, I have always regretted selling that telescope. So, in 2018, I bought another 6-inch, but this time with an f/6 focal ratio. The Criterion RV-6 was an f/8. I like the f/6 much better as the optical tube is not as long, and the shorter focal length allows for wider fields of view. When emplying a 2x Barlow, the f/6 becomes an f/12 focal ratio.

I also have a 4.5-inch f/8 Newtonian that was given to me last year (March 2025) by a friend. I like this telescope as when using, reminds me of my 4.25-inch f/10 EQ Edmund reflector. This was my first “very own” telescope, which opened the world of (serious) amateur astronomy to me in the spring of 1977.

After being a serious “visual” observer for at least 40 years and having had more than 12 telescopes, I’ve come to the conclusion:  A 6-inch f/6 Newtonian just might just be the perfect amateur telescope by offering enough aperture to see thousands of deep-sky objects and with reasonable portability.

The Train of Life By James S. Tippett (1885-1958)

Posted April 20, 2025 by rogerivester
Categories: Roger's Articles

Recently, we had a good friend to lose their father. I wanted to say something meaningful and not just “I’m very sorry” and nothing more. So, quite a few years ago, I had read a poem by James S. Tippett, and thought it would be very good to share with anyone who had just lost a loved one. This poem also has great meaning for all of us…to think about and contemplate from time to time.

The train photo from Public Domain: Strasburg Railroad of Lancaster, Pennsylvania. And “The Train of Life” by James S. Tippett

At birth, we board the train and meet our parents, and we believe they will always travel by our side.

As time goes by, other people will board the train; and they will be significant i.e. our siblings, friends, children, and even the love of your life.

However, at some station our parents will step down from the train, leaving us on this journey alone.

Others will step down over time and leave a permanent vacuum. Some, however, will go so unnoticed that we don’t realize they vacated their seats.

This train ride will be full of joy, sorrow, fantasy, expectations, hellos, goodbyes, and farewells.

Success consists of having a good relationship with all passengers requiring that we give the best of ourselves.

The mystery to everyone is: We do not know at which station we ourselves will step down.

So, we must live in the best way, love, forgive, and offer the best of who we are.

It is important to do this because when the time comes for us to step down and leave our seat empty, we should leave behind beautiful memories for those who will continue to travel on the train of life.

This poem was written “again” by James S. Tippett, but you might find a similar poem with variations via online.

April (2025) photo

Recurrent Novae Star T CrB: Now Is The Time To Be Watching For The Predicted Outburst

Posted April 3, 2025 by rogerivester
Categories: T Corona Borealis

Tags: , , ,

For those waiting and watching for the predicted outburst of recurrent novae star, T Corona Borealis, the excitement is building, but no one knows when the event will happen.

I’ve been making photos of the constellation Corona Borealis as often as possible since March (2025) using my cellphone with 3-second exposures. When the outburst “finally” occurs, there will be the appearance of a “new star” in the constellation and visible without optical aid. The outburst could become the brightest star in the constellation, possibly reach a magnitude of 2.0 or even brighter.

For the location of T, see the (X) inside the box, which at current or before the outburst is shinning at ~10, which is much fainter than can be seen without optical aid. Image as following and credit to wikisky.org

The following photo was made this morning…Saturday February 7th 2026 @ 2:56 AM: Corona Borealis is in perfect sky position, high in the east.  The bright moon made the constellation difficult to see without optical aid.   

In his book Starlight Nights,Peltier writes:

“I alone am to blame for being remiss in my duties, nevertheless, I still have the feeling that T could have shown me more consideration. We had been friends for many years; on thousands of nights I had watched over it as it slept, and then it arose in my hour of weakness as I nodded at my post. I still am watching it but now it is with a wary eye. There is no warmth between us any more.” Leslie Peltier

The following picture is provided just for reference as to the location of T, however, not likely will it be this bright as related to other stars in the constellation, but lets keep watch.

The following excerpts are from a “Sky & Telescope” online article.

Take T Coronae Borealis (T CrB). It’s one of only about 10 stars in the entire sky classified as a recurrent nova, with two recorded outbursts to its name. Normally, the star slumbers at 10th magnitude, but on May 12, 1866, it hit the roof, reaching magnitude +2.0 and outshining every star in Corona Borealis before quickly fading back to obscurity. Eighty years later, on February 9, 1946, it sprang back to life, topping out at magnitude +3.0.

“I alone am to blame for being remiss in my duties, nevertheless, I still have the feeling that T could have shown me more consideration. We had been friends for many years; on thousands of nights I had watched over it as it slept, and then it arose in my hour of weakness as I nodded at my post. I still am watching it but now it is with a wary eye. There is no warmth between us any more.”

T stayed under the radar for the next 69 years, holding steady around magnitude +10.2–10.3. That began to change in February 2015, when it inched up to +10.0 and remained there until early February this year. That’s when things kicked into high gear with the star steadily growing brighter from late winter through early spring to reach its current magnitude of ~9.2.

Alongside the brightening trend, T’s become bluer as well. Astronomers describe its recent unprecedented activity as a star entering a “super active” state. This last happened in 1938, eight years before its last great outburst.

Two For T
Stars like T CrB involve a red giant closely paired with a white dwarf. The giant feeds hydrogen gas into a swirling accretion disk around a massive, compact white dwarf at a rate a million times greater than the solar wind. Material funnels from the disk onto the dwarf’s surface until it ignites in a thermonuclear explosion similar to a nova.
NASA

Galaxies NGC 4290 And NGC 4284 Which Can Be A Real Challenge For The Backyard Observer

Posted March 25, 2025 by rogerivester
Categories: Roger's Articles

Sue French: Observer from New York

M40 is a double star near Megrez (Delta Ursae Majoris). Oddly, M40 was once considered a non-existent Messier object. In his 1784 catalogue, Charles Messier described his 40th object as: “Two stars very close to one another and very small, placed at the root of the great Bear’s tail.” Precessing Messier’s coordinates to equinox 2000 takes us right to such a star pair. Messier noted this double while searching for a “nebulous star” reported by Johannes Hevelius. Messier assumed that Hevelius mistook these two stars for a nebula, but the latter was actually referring to a different pair of stars – also without nebulosity.

To locate M40, start at Megrez and hop 1.1º northeast to mag. 5.5 70 Ursae Majoris. Continue that line for 1/4º to arrive at M40. My 4.1-inch scope at 28x reveals an east-west pair of mag. 10 stars, with the western one slightly brighter. Through my 10-inch scope, I see the primary as yellow-orange and its companion as yellow-white. 

Two galaxies share the field at 118x. NGC 4290 is a small northeast-southwest oval, and NGC 4284 is a tiny faint spot forming a 1½’ triangle with two mag. 13 stars. 

The galaxies are about 140 and 190 million light- years away. Although the distances to its stars are poorly known, M40 is probably an optical (unrelated) pair.  Independently discovered in 1863 by the German astronomer Friedrich August Theodor Winnecke, M40 carries the double-star designation Winnecke 4. Winnecke is also the original discoverer of eight NGC objects, and ten comets that bear his name.

Roger Ivester: Observer from North Carolina 

Due to our recent bad skies, I was unable to make a new observation of M40, and galaxies NGC 4284 and NGC 4290. I was forced to use a sketch and notes from an earlymorning observation on February 25, 2000. 

On that night, I was using a 10-inch reflector from my moderately light-polluted backyard with a 5.8 NELM. It was an especially good night with excellent transparency.

M40, a pair of mag. 10 stars, also known as Winnecke 4, was very easy with a wide separation of about 50 seconds of arc. The pair was oriented mostly east-west and both appeared as whitish-yellow in color.

Two faint galaxies were located very close to M40. All three objects were located within a 1/2º field-of-view.  Just to the west of M40, lay faint galaxy NGC 4290 at mag. 12.0, elongated NNE-WSW. I saw a very subtle brightness in the central region. Very close and to the west of it was a very faint mag. 14 galaxy, NGC 4284, which was extremely difficult, appearing as a faint, mostly round blur. And during a previous observation from the same location with a friend, and in a side-by-side comparison with the 10-inch reflector and an 8-inch Celestron Schmidt-Cassegrain.  We couldn’t see NGC 4284 with the 8-inch SC telescope, but could in the 10-inch Newtonian.  

The following pencil sketch was made using various graphite pencils and a blank 5 x 8 notecard with the colors inverted using a scanner. 

Jaakko Saloranta: Observer from Finland

Here’s all I’ve got: With a 4.5-inch reflector @ 152x (20′), the galaxy appeared as a fairly faint, NE-SW elongated galaxy, without detail, close to double star M40. NGC 4284 was invisible. Altitude of the object was 74°.

Galaxies NGC 3893 And NGC 3896 In Ursa Major Always Be Sure To Document Your Observations…

Posted March 23, 2025 by rogerivester
Categories: Roger's Articles

Mario Motta: Observer from Massachusetts 

This image took some effort. I captured the galaxy in Lum with my 32-inch this past December from Gloucester, but did not have enough night to get it in color.  

I tried in Florida, but it lacks the detail of the 32-inch as it is only 4.5 by 2,4 arc minutes, thus needs the larger telescope for detail.  However, I then used a process in pixinsight to combine images from 2 different optical systems, and it worked. So…lum from the 32-inch scope with about 75 minutes lum ZWO 6200 camera.  

Then RGB from C14 scope in Florida again ZWO 6200, (about 70 min total), processed then combined with dynamic alignment tool in Pixinsight. Note NGC 3896 close by to the immediate east.This worked, I may try for more such galaxies in color only to add to my 32 inch collection of galaxies in Lum only. Spring is so short a season for all the galaxies available.  

Jaakko Saloranta: Observer from Finland

Back in March, the galaxy duo was visible in a good, high (77°) spot in the sky. Using high magnification (304x) with a 4.5-inch reflector, I described the view as follows: Fairly bright, N-S elongated galaxy with a brighter nucleus. Faint mag. 13 star touched the halo in NW. 

NGC 3896 appeared as a tiny, fairly faint and slightly SE-NW elongated galaxy just south of a mag. 13 star. Observing conditions were average: NELM around 6.0 with SQM-L readings of 20.20 near the object. Temperatures still dropped well below zero Celsius on the night of 26 March.

Roger Ivester: Observer from North Carolina 

I wanted to share an article concerning an observation I made on April 20, 1993. It’s a testament that documenting and taking good notes is indeed a good thing! During some recent cloudy weather, while reviewing past logbook entries, I discovered that I had not followed up on an object viewed on 20 April, 1993. The main object was NGC 3893, a mag. 11 galaxy in Ursa Major. While making my sketch of this excellent galaxy, I noticed a smaller, very faint object, SE and very close. I noted this in my logbook as one to look up later. It was almost ten months later, while browsing through the logbook, that I remembered to follow up on this observation.

I checked Burnham’s Celestial Handbook, Tom Lorenzen’s 1000+, and the Tirion Sky Atlas 2000.0, only to find that none of these sources listed a companion galaxy. I then went to the NGC 2000.0 Catalog by Roger Sinnott, and found the companion listed as NGC 3896, a 14th magnitude galaxy. I was elated to find out this was a faint galaxy. It should also be noted that my observation was made from my back deck, with several unshielded streetlights nearby.

If I had not sketched NGC 3893, it’s possible that I would have missed NGC 3896. If I had not logged the mysterious companion, I probably would never have checked any reference material on a future date. 

So, the moral of this story is: Keep a logbook, sketch your observations, and periodically review your notes. You never know what you might find.  I was very excited about going back to NGC 3893 and NGC 3896 after twenty one years, and surprised that they appeared exactly as I remembered them. 

It’s truly amazing how the brain can remember a faint galaxy pair after all this time.Using a 10-inch Newtonian reflector, I could easily see NGC 3893 at 57x, appearing as a faint oval, oriented NNW-SSE. When I increased the magnification to 200x, the halo became enlarged and I saw a faint stellar nucleus. I also spotted a mag. 13 star on the NW tip.

The faint companion galaxy, NGC 3896, at mag. 14.0 was very difficult, especially when observed from my moderately light polluted backyard. Using 200x and averted vision, it appeared mostly round with low surface brightness. I noted little to no detail. With patience and careful viewing, I saw two very faint stars on the NW tip.

Revised: Seeing Uranus Without Optical Aid? Is It Possible From A Suburban Back Yard, With A 5.5 NELM At The Zenith?

Posted March 8, 2025 by rogerivester
Categories: Roger's Articles

I received an email Saturday morning (March 7th 2025) from expert visual observer, Jaakko Saloranta from Finland. He asked me if I’d ever seen Uranus without optical aid. Seems that Jaakko had a “lively” discussion with some reporters concerning the visibility of seeing Uranus naked eyes.

March 18th 2025: My observation to see Uranus was unsuccessful, as transparency was poor and my NELM was less than 4.8 at the zenith, and the planet has a magnitude of ~ 5.75. And unfortunately, Uranus was already getting into the light dome of Boiling Springs, North Carolina.

After more than an hour of careful observing with a small 6 x 30 finder (by design) then looking over the finder, I could not see the planet naked-eye. I’d suggest this technique is an advantage as opposed to attempting to find Uranus in a mostly blank area of the sky. I used a 4.5-inch f/8 Newtonian on a GoTo mount to locate Uranus. A planet…unlike a deep-sky object does not have a permanent sky address.

My observational attempts are now over until November 2025. The trees and plants (March 22nd) are showing new life and pollen is beginning to fill the sky and reduce the sky transpacy considerably. I’d suggest pollen is similar to snow covering reflection.

I made the following wide-field sky photos last night (March 18th) at 9:30 PM using my iPhone. Can you see Uranus?

March 8th 2025 Observation:

Despite a bright moon, I wanted to use a 4.5-inch Newtonian from my suburban backyard, just to observe the planet telescopically. I’ll then try the small 6 x 30 finder, and then my 7 x 21 Pentax mini-binoculars. I was successful in seeing the planet with all three, but never attempted naked eyes for obvious reasons. Roger

Reports as following

Alan French (New York)

Long ago, it was the late 1980s or early 1990s, Sue and I made a point of catching Uranus by eye from the Texas Star Party. If I recall correctly, the folks at TSP suggested it because the planet was in a sparser star field than usual.  It’s not something I could probably do today. 

Observer 2: March 8th 2025 @ 8:30 PM EST

Roger Ivester (North Carolina)

March 8th 2025: 71% illuminated Moon, excellent seeing @ 50º

First let me say, I was using a Goto mount when attempting to see the planet Uranus. A GoTo system would give anyone an advantage. And a faint planet can be difficult to locate…unlike a deep-sky object that has a permanent sky address.

Yes, I know that the objective is to see Uranus without optical aid, but I just had to first see it with a 4.5-inch f/8 Newtonian. It was easy, appearing as a mostly white star using a magnification of 35x. When increasing the magnification to 128x, it still appeared as a star, but now with a greenish tint.

I could easily see with a small 6 x 30 finder scope, but a bit fainter through a pair of 7 x 21 Pentax binoculars. Then when looking over the finder, then alternately looking through the finder, I could not see Uranus without optical aid.

I wanted to document all things on this night, even with a photo of the telescope and mount used. This was a telescope given to me recently by a friend, and I’ve been spending a little time this week tuning it up. I was interested in seeing Uranus with the tiny 6 x 30 finder.

Observer Three: March 9th 2025

Mario Motta (Massachusetts)

Hi Roger,

As it turns out I have such an image, taken five years ago with my 32-inch telescope. The small planet size at such a great distance, does indeed has a slight greenish color, just like you mentioned in your post.

Taken with my 32-inch f/6 telescope, with ZWO asi 071 OSC camera, video the stacked and processed

The second image presents five of the planets moons…and very nicely!

Mario

Supplemental: Successful observation without optical aid by Mario Motta:

I once saw it naked eye from my place in New Hampshire, about 20 years ago with a mag. 6.5 sky.

Observer 4: Jaako Saloranta from Finland:

Hey Roger,

Here’s my sketch of Uranus – this is the original one I made at the site and as I no longer have a working scanner… this is all I could muster with my phone.

I rode my bicycle roughly 10 kilometers west from my house and found a decent, dark spot for myself. Temperature was roughly 27°F so it didn’t take too long for me to get cold after some sweaty cycling! While waiting for full night vision I could see M34, M35 and maybe M36 with the naked eye. Winter Milky Way was faintly visible from Perseus to Monoceros. 

But Uranus itself… seeing it was quite difficult because of the low altitude (~30 degrees). I could see roughly down to magnitude 6.5 from the west/zenith but at the general region of the Pleiades I could barely make out 6 magnitude (I managed to saw 65 Arietis only a few times during the 30 minutes I was observing Uranus) stars. I could see Uranus only… maybe 30% of the time with optimal averted vision. See Uranus back in 2011 was a lot easier from Canary Islands (high altitude, higher object altitude, darker skies and younger observer).

After I was done observing, I noticed that green aurora borealis arc in the northern sky. When I eventually got back home, I could see faint aurora glow even at the zenith.

/Jaakko

Observer 5: Steve O’Meara (Tucson)

Hi Roger,

Sometime in the 1980’s, I was outside David Levy’s Tucson home, casually stargazing by eye with Steve O’Meara, when Steve noticed Uranus in the sky.

Clear skies, Kelly Beatty

A 6-Inch Newtonian Is An Excellent Deep-Sky Telescope And With More Than 2x The Light Gathering Capability Of A 4-inch Refractor

Posted February 22, 2025 by rogerivester
Categories: Roger's Articles

Saturday February 22nd 2025:

My plans for this year (2025) are to use my 6-inch f/6 Newtonian almost exclusively as my primary deep-sky telescope. The 6-inch is relatively light and much easier to set up and bring back inside after a night of observing, as compared to my much heavier 10-inch solid-tube Newtonian.

Note the number of counterweights, as the 6-inch with an 80 mm f/5 refractor and required another weight to properly balance.

Vixen has an odd diameter declination shaft, which will allow only a Vixen weight. I just ordered and received the extra weight only yesterday (Friday February 21st 2025.)

Note the carbon fiber tape around the back or bottom of the optical tube: This is to prevent “bumping” into the back of another mount used with this telescope, which is a CGE-Pro, when setting in place, and removing. The optical tube has to be set in from the upper or top side, and removed by pulling up also, which puts the tube in an awkward position, as it’s above waist height.

The piggyback 80 mm refractor with an amici diagonal (correct image) serves as both a second telescope and my finder. Note: I also have a Rigel Quick Finder for quick pointing, and as another source to locate brighter deep-sky objects.

Using a Celestron CGE-Pro GoTo mount is always possible for finding “immediately” those very faint deep-sky objects without spending an excessive amount of time. This mount will be used to locate and see those objects on the threshold of the 6-inch. When I know a “very faint” object is in the center of the telescope field of view, “it’s much easier” to see.

A Supernatural Event On A Summer Afternoon…Or Was It Something Else?

Posted February 5, 2025 by rogerivester
Categories: Roger's Articles

During the summer of 2023 while my wife, Debbie and I were in Gaffney, South Carolina, we stopped at a drive-thru restaurant. Upon leaving I noticed a person sitting at an outside table under an umbrella, shielding themselves from the sun. It appeared they might possibly have had all of their earthly possessions in a shopping cart. The contents in that cart were piled high and so much so, they were spilling over the sides. 

However, when driving past, a strange feeling came over me, that I just had to stop and talk to this person. I stopped and asked If I could buy them something to eat. They hardly looked up, all the while continuing to write on a sheet of paper. They glanced up with an annoyed look and said:  “I’m not here for you to buy me something to eat” I’m here to pray for you.” I was a bit taken aback, but said thank you.

This person continued writing almost fervently, and I asked: Could I have the prayer to take with me, and read later?  The person said: “No…I’ll read it to you” but saying so with conviction.  

The mysterious person began reading the prayer, but I could not seem to hear or understand anything they were saying.  It was just unintelligible words, and I could not comprehend a single thing being said. After reading the prayer, the mysterious person put their pen and prayer away rather hurriedly.  

There was something else, as strange as it sounds, but I could not seemingly see their face. Maybe I wasn’t suppose to and If asked later, what did they look like, I couldn’t say. 

So, we drove away, but there was traffic in the parking lot of the restaurant and shopping center, and was forced to turn around only a few hundred yards away.  This took, maybe a couple minutes or so, at most. I began thinking about the stranger and our encounter, and just had to go back to see them again. However, upon returning to the table and umbrella…neither the person nor the overflowing shopping cart were there.  We drove around the restaurant, looking in all directions, but the person that just read a prayer to me, was nowhere to be seen.

It would have been impossible to simply leave this fast and with a grocery cart running over with bags of clothes and whatever.  But yes, the person seemingly had just vanished into thin air!  And why would this person…this apparition, after not willing to give me the written prayer, suddenly leave?  And now after almost two years, I continue to think and wonder: Was this truly a supernatural event?  Could it really have been something unworldly, maybe even an angel sent to me for a purpose? It could have been for many purposeful reasons, such as a delay to keep us from from leaving, and getting back on the highway. It could have been for countless other reasons, and one day, I believe this reason, or purpose will be manifested to me.

Angels are mentioned in the bible, almost 300 times. And if you believe in God, you also believe in angels. President George Washington experienced a vision, being described as an angel at Valley Forge, during the American Revolution. This event has been well documented by both Washington and others. And there are countless stories of angel encounters, but most of the time people ignore them, and most often, just don’t believe.

However, I cannot definitively prove anything in my story, and it’s just my own recording of a personal event, that happened almost two years ago, on a summer afternoon. If my wife, Debbie had not been with me, and also witnessed this incredible event, I would never have considered writing this story…

Roger Ivester (Boiling Springs, NC on March 16th @ 6:30 AM EDT, 2025)