Galaxy NGC 3079 – Ursa Major: April 2022 Observer’s Challenge Report #159

Posted April 5, 2022 by rogerivester
Categories: Uncategorized

Medusa Nebula – Abell 21 – Planetary Nebula in Gemini: March 2022 Observer’s Challenge Report #158

Posted February 27, 2022 by rogerivester
Categories: Uncategorized

The following Information taken from “Deep-Sky Wonders” by Sue French:

Sweeping 2 1/2º eastward brings us to the cluster NGC 2395. My little refractor at 87x reveals 20 stars loosely scattered across 15′. At 28x, it merely shows a granular-looking patch with two faint stars, but something remarkable happens when I add an oxygen III filter. Although completely invisible before, Abell 21, the Medusa Nebula, joins the scene 1/2º southeast of the cluster! I can see it with direct vision, but it shows up better with averted vision. This unusual planetary nebula is about 8′ across, dented in its northwest side, and brightest toward the northeast and southwest. With my 10-inch scope at 68x, I prefer viewing Abell 21 with a narrowband nebula filter (rather than the oxygen III filter) which shows this large, impressive detailed planetary to be very uneven in brightness. SF

MONTHLY OBSERVER’S CHALLENGE

Compiled by:

Roger Ivester, North Carolina

&

Sue French, New York

March 2022

Report #158

The Medusa Nebula, (Abell 21, PK 205+14 1, PN G205.1+14.2) 

Planetary Nebula in Gemini

Sharing Observations and Bringing Amateur Astronomers Together

Introduction:

This month’s target:

Abell 21 was discovered during the course of the Yerkes-McDonald survey of  symmetric galactic nebulae. The ensuing catalog was published by Hugh M. Johnson in the May 1955 issue of the Astrophysical Journal, in which it was given the designation YM 29. https://ui.adsabs.harvard.edu/#abs/1955ApJ…121..604J/abstract

The nebula was independently discovered by George O. Abell among globular clusters and planetary nebulae newly found on the National Geographic Society-Palomar Observatory Sky Survey. His paper was published in the August 1955 issue of the Publications of the Astronomical Society of the Pacific, which listed 13 globular clusters and 37 planetary nebulae.

https://ui.adsabs.harvard.edu/#abs/1955PASP…67..258A/abstract

Although the nebula is number 16 in Abell’s list of planetaries, it’s now commonly known as Abell 21. His well-known, updated list of  86 planetary nebulae was published in the Astrophysical Journal  in 1966, and since the nebulae are given in order of right ascension their numbers were changed accordingly.

https://ui.adsabs.harvard.edu/#abs/1966ApJ…144..259A/abstract

In his 1961 “A Description of Fifty Planetary Nebulae”  https://ui.adsabs.harvard.edu/#abs/1961AZh….38…75V/abstract, B. A.Vorontsov-Vel’Yaminov, credits the name Medusa Nebula to a 1961 entry in Astronomicheskij Tsirkulyar No.221 (1960), which unfortunately or mercifully, depending on your point of view, I do not have access to. Sue French

Bertrand Laville: Observer from France (pencil sketch)

Roger Ivester: Observer from North Carolina

Pencil sketch using a 10-inch f/4.5 equatorially mounted reflector

Abell 21 also known as the Medusa Nebula:  

After spending four nights and ten hours, with two different telescopes, and multiple eyepieces and filters:  I was finally able to “visually” see the Medusa Nebula.  For me…the euphoria of seeing an extremely faint deep-sky object after many nights and hours, can “or might be similar” to something physical, such as running a marathon, which I’ve never done, but I have competed in bicycle races.  

To be able to locate and “visually” see the Medusa Nebula, a very dark sky is most desirable, but which is something I don’t have from my suburban backyard. My best NELM seldom exceeds 5.0-5.2 on a superb winter night. But I’ve always tried to make-do, and thus far, been successful in seeing all of the challenge objects for the past almost 14 years, and now exceeds more than 200 deep-sky objects.  

The Medusa Nebula is the most difficult (visual) object featured to-date in the Observer’s Challenge report for the past almost fourteen years.  This might be proof that a dark site with a 6.0-7.0 NELM is not necessary to enjoy the wonders of the night sky. 

The Medusa Nebula:   

Easy for the imager, but extremely difficult for the “purist” back yard amateur astronomer, using an eyepiece, an O-III or UHC filters, a pencil, note and sketch pad.  

Amateur astronomy can be anything the amateur wants it to be.  But for me, I want it be “not too distant” from the nights, taking out a 60mm refractor, in what I called the “weedy-field” beside my childhood home.  I wanted to see some of those fabulous spiral galaxies (and in color) that I’d seen in my 6th grade science book.  Of course I never did, but without any support or guidance, I learned what was possible.  

I’ve never been disappointed in those very faint objects that are barely visible in the eyepiece, and requires hours or nights to finally see, but somehow “for me” those are my favorite.  Where in the solitude of the night, I might whisper to myself:  THAT’S IT !  

For those few that choose to carefully, and with patience, observe and sketch a deep-sky object, also supplementing with copious notes, they will never forget what that object looks like, and with instant recall. 

After 50 years of observing, I’m so glad I never lost my EP, my pencil, or my sketchpad, as I never had any desire to become an imager.  I also have a library with hundreds and hundreds of “one of a kind” pencil sketches, to review, and for future reference.   

If you’ve never attempted to make a pencil sketch, with supporting notes, you should consider.  And we need to keep the ancient art of visual observing and “pencil sketching” alive.  A skill or facet of amateur astronomy that fewer and fewer seem to be interested in these days.

After all, this was the original reason or concept for the founding of the Observer’s Challenge back in 2009.     Roger Ivester

Observing Globular Cluster Omega Centauri From North Carolina, Hawaii, Death Valley, And West Virginia

Posted February 19, 2022 by rogerivester
Categories: Roger's Articles

After years of wondering if I could see globular cluster (NGC 5139) Omega Centauri and galaxy (NGC 5128) Centaurus A from my home at a latitude of (+35º 18′) so I gave it a try on April 26th 2009.  

My poor southern view required that I go to a dark-site on the southern rim of the South Mountains, only thirty minutes away.  I met with longtime friend and expert amateur Steve Davis, who brought a Meade 12-inch Dobsonian, which was invaluable in also seeing galaxy Centaurus A.

The 12-inch also provided an excellent resolve of “Omega Centauri” despite the telescope optical tube being almost parallel to the ground!  

Theoretical limiting horizon calculation from Western North Carolina at +35º North Latitude:

(90º-35º) = -55º theoretical limiting south latitude. 

Omega Centauri south latitude:  -47º 28′  

My limiting southern horizon @ -55º (-) -47º = Only 8º above my theoretical southern horizon, and again…which puts my telescope tube almost parallel to the ground!  

I made the following sketch using a 102mm f/10 refractor, on the same night and location The NELM was ~6.5 at the zenith and with a good view of the southern horizon. However, the excellent seeing overhead did not transfer to the extremely low southern view as expected, at only 8ºs about my limiting horizon. The globular appeared fairly dim, mostly round, well-defined edges with some brighter members sparkling in the interior with averted vision.  I also noted many faint outliers enveloping the cluster.

When observing with the 12-inch f/5 reflector the globular cluster was well resolved.  Despite observing at a fairly dark-site, I was looking over distant lights and layers of atmosphere which diminished the view significantly the galaxy was not visible with my 102mm refractor.

Observing galaxy “Centaurus A” with a 12-inch f/5 reflector: My notes read: Difficult! A very small smudge with a stellar nucleus.  Regardless, of the poor view of Centaurus A, I was happy.

102mm refractor: Rough field-sketch of globular cluster Omega Centauri as following using a chalk pencil on black card stock: Date 4-26-09 @ 1:00 AM EDT off Jack Moore Mountain Road.

Pencil sketch as following using a 12-inch f/5 reflector:

James Dire Image from Barking Sands, Kauai, Hawaii

Stellarview 102mm f/6.3 refractor w/Televue 0.8x focal reducer flattener

Omega Centauri from Naples, Florida using a C-14 telescope by Mario Motta:

In close proximity is galaxy, NGC 5128, known as Centaurus A, also with a C-14 telescope from Naples by Mario Motta:

Fred Rayworth of Las Vegas, saw Omega Centauri from Cathedral Gorge, Utah @ +37º 49′ 20″

“I saw Omega Centauri just over the hood of a truck on the horizon. I had a chance to see it at Death Valley, California when we went to the airport, but never caught it.”

+90º North (-) +37º 50′ = (-) 52º 50 mins or limiting southern horizon

So:  -52º 50′ (-) -47º 28′ = ~ 5º 22 mins above the horizon from Cathedral Gorge.    

Larry McHenry: Observing from West Virginia

Globular cluster NGC 5139 “Omega Centauri.”

Location: Calhoun County Park in central West Virginia. Setup on a ridge of about 1100 ft in elevation. (more about Calhoun at: http://stellar-journ…calhounpark.htm 

At the time of observation, NGC 5139 had an elevation of about 3.5º above the horizon.

First a wide-field “finder” image of NGC 5139 (Omega Centauri) using my Canon 100mm video lens & ASI290MC camera. 

Here’s the main EAA observation of Omega Centauri, again thru the trees, from 4/28/22 at 12:28 AM.

(8-inch SCT @ f/6.3 on an Atlas German equatorial mount , ZWO ASI294MC camera with L-Pro filter, 20 second subs, no dark or flat frames, not guided, live-stacked using Sharpcap for 80 seconds). 

Due to the short exposure time, we were able to see the dark feature called the “Eye of Omega”, which is possibly a dark molecular cloud that is in front of the cluster in our line-of-sight. 
This is generally only seen visually, as most images are longer exposures to pull-out more of the cluster stars. 

We Were Fortunate To Have John Dobson Visit For a Couple or More Weeks During The Late 90’s

Posted January 31, 2022 by rogerivester
Categories: Roger's Articles

Myself (L) Tom English in the center, and Dobson. I can’t remember, but I think someone local knitted Dobson the funky hat, which he wore most all of the time during his visit.

We had a get-together and dinner at one of the local astronomy club members home.

Dobson and Tom English during a solar observing session. Best I remember, Dobson didn’t think it was a good idea to observe the sun with a solar filter.

A letter that Dobson wrote to my wife, after he returned to San Francisco. He wanted to tell her about a movie he had seen.

M42 and M43 – Bright Nebulae in Orion: February 2022 Observer’s Challenge Report #157

Posted January 21, 2022 by rogerivester
Categories: Uncategorized

MONTHLY OBSERVER’S CHALLENGE

Compiled by:

Roger Ivester, North Carolina

&

Sue French, New York

February 2022

Report #157

M42 and M43, the Orion Nebula

Sharing Observations and Bringing Amateur Astronomers Together

Final Observer’s Challenge Report:

NGC 1501 – Planetary Nebula in Camelopardalis: January 2022 Observer’s Challenge Report #156

Posted January 19, 2022 by rogerivester
Categories: Work File Only - Observer's Challenge Reports

Work-File: Used only for organization and editing. When all entries are received, a final .pdf report will be issued by the 10th of February. And the link will be posted on this page.

MONTHLY OBSERVER’S CHALLENGE

Compiled by:

Roger Ivester, North Carolina

&

Sue French, New York

January 2022

Report #156

NGC 1501 Planetary Nebula in Camelopardalis

This month’s target:

William Herschel discovered NGC 1501 with his 18.7″ reflector on 3 November 1787. As handwritten by his sister Caroline, his description, reads: A very curious Planetary nebula near 1′ diameter. Round, pretty-well defined of a uniform light and pretty bright. Not surprisingly, the open cluster NGC 1502, sitting just 1.4° north of the nebula, was the next discovery in Herschel’s sweep.

Lawrence Parsons (the 4th Earl of Ross) and his assistant Ralph Copeland observed NGC 1501 several times with the 72-inch Leviathan… Perhaps the best description comes from Lord Rosse’s observation on 15 January 1868: A bright ring and inside it a dark annulus, very decided. A star in the centre seen very clearly and continuously with various powers; suspect variable [unequal?] brightness in the ring, perhaps a dark spot in it nearly on the preceding [western] side. The following [eastern] side of the ring appears broadest and to approach the central star nearer than the preceding side does. The north and south sides of the ring seem rather brighter than the preceding and following sides. Suspect other bright points in it, but am not at all certain. It is slightly elliptical, its major axis being preceding and following.

Complete and Finalized Report: Click on the following Link:

january-2022-observers-challenge-_ngc-1501

Pencil Sketch of NGC 1501 – Planetary nebula in Camelopardalis  

NGC 2264: The Christmas Tree Star Cluster and Cone Nebula In The Constellation Monoceros

Posted December 16, 2021 by rogerivester
Categories: Roger's Articles

“Dubbed the Christmas Tree Cluster by Leland S. Copeland, this striking cluster well deserves its nickname. I recall observing NGC 2264 long ago when I’d heard of the Christmas Tree but didn’t know to which cluster the name referred. One look through the eyepiece and I knew this must be it!”

“…I can imagine them fashioning a large five-pointed star crowning the tree. Since the tree hangs tip-south in the sky, it can sometimes be seen upright when viewed through a telescope that inverts the view…” 

NGC 16; Galaxy in Pegasus: December 2021 Observer’s Challenge Report #155

Posted November 23, 2021 by rogerivester
Categories: Uncategorized

Pencil sketch by Roger Ivester:

NGC 7662 Planetary Nebula in Andromeda: November 2021 Observer’s Challenge Report #154

Posted November 19, 2021 by rogerivester
Categories: Work File Only - Observer's Challenge Reports

MONTHLY OBSERVER’S CHALLENGE

Compiled by:

Roger Ivester, North Carolina

&

Sue French, New York

November 2021

Report #154

NGC 7662 Planetary Nebula in Andromeda

Sharing Observations and Bringing Amateur Astronomers Together

Final November .pdf report, click on the following link:

This is the observer’s challenge “Work-File” report: Used only for organization and editing. When all entries are received, a .pdf report will be issued by the 10th of December. And the link will be posted on this page.

Commonly called the Blue Snowball, the planetary nebula NGC 7662 dwells in the northern reaches of Andromeda. Its nickname springs from an article by Leland S. Copeland in the February 1960 issue of Sky & Telescope magazine. Copeland describes the nebula as “looking like a light blue snowball.” 

William Herschel discovered this nebula on October 6, 1784, with this 18.7-inch reflector. His journal entry reads: A wonderful bright, round planetary pretty well defined disk, a little eliptical [sic]; perhaps 10 or 12″ diameter. Another entry from October 3, 1790, endearingly states: My planetary nebula. A very beautiful object, with a vS [very small] star following; giving one the idea of a large Planet with a vS satellite. In his impressive new book, William Herschel Discoverer of the Deep Sky, NGC/IC researcher Wolfgang Steinicke credits William Herschel with 10 observations of NGC 7662.



NGC 6857: Emission Nebula – Cygnus: October 2021 Observer’s Challenge Report #153

Posted October 13, 2021 by rogerivester
Categories: Work File Only - Observer's Challenge Reports

MONTHLY OBSERVER’S CHALLENGE

Compiled by:

Roger Ivester, North Carolina

&

Sue French, New York

October 2021

Report #153

Click on the following link, for the complete report:

october-2021-observers-challenge-_ngc-6857-1

This month’s target:

William Herschel discovered NGC 6857 on 6 September 1784. His handwritten journal for that date reads: A patch containing some nebulosity…irregularly long.

Heinrich d’Arrest writes of this object and his observation of it in his 1867 Siderum Nebulosorum Observationes Havnienses. My very loosely paraphrased English for the Latin text: Minute, faint; it is most probably a cluster. A 12th-magnitude star precedes it. – Rechecked shortly after: it was not so small; not all of the nebula is resolved, there is at least some cloudiness. I’m not surprised that this was missed by Rosse.

NGC 6857 is the brightest part of the larger, star-forming emission region Sharpless 2-100, which is a much more difficult visual target than NGC 6857. 

A 2010 paper by Manash Samal and colleagues in the Astrophysical Journal indicates that the main ionizing source at the center of NGC 6857 is the bright, massive star at its heart. This compact nebula is estimated to be approximately 28 thousand light-years away from us, and the star is thought to have a spectral type of about OIII. The most likely age of the nebula is in the vicinity of 1 to 2 million years. (Intro and object information by Sue French)