In A Galaxy, Very, Very Far Away...

Just, beyond a galaxy - far, far away....lie, two other galaxies, in a galaxy group that, the three - have all to themselves. The little group is called the "Leo Triplet" but it is actually likely part of a larger group of galaxies called the "Leo-I" ('Leo One') group.

Moreover, like most things 'cosmological', the connections don't end there: gas-streamer bridges connecting one galaxy or group of galaxies to another group - ultimately, ending in "super-clusters"; i.e., a cluster of clusters of galaxies - the largest, single structures in the universe!

The proximity of the Leo Triplet puts it roughly between our own "Local Group" of galaxies and the Leo-I group; "galaxy-group neighbors", so to speak - or numerically: only, around 30-35mly (million light-years) distant. How far away is that? Well, about 300 times the diameter of the Milky Way galaxy, which is ~120kly (~120,000ly), across.

The "Leo Triplet" consists of galaxies NGC 3628 (left), M65 (upper right), and M66 (lower right). Image provided by the author using Insight Observatory's 16" f/3.7 astrograph reflector, ATEO-1.

  
This tiny distant galaxy group features two spiral galaxies M-65 and M-66 discovered by French amateur astronomer Charles Messier; a comet-hunter by avocation. He tallied a list of small, dim objects in the night sky that appeared to be comets but he soon found we were not as they didn't move from their positions over long periods of time. They were permanent entities. He kept this list only to avoid these objects in future comet searches which he performed in the years around 1773.

The third galaxy, NGC-3628, another spiral saw edge-on; that is inclined 90° from our galactic perspective was discovered by German sister, and brother amateur astronomers William and Caroline Herschel back in the middle 1800s.

M-65, is a 'barless spiral, at 35mly. It is slightly warped, and, there has been some recent star birth activity in one of its gaseous H-II regions.

Of the three M-66 is closest at 31mly with a diameter of about 95kly. It is the brightest of the three but it is missing a large portion of one of its spiral arms. The missing mass from that arm was gravitationally removed by one or both of the other galaxies in the trio.

M-66, has a weak bar feature, extending from its core, and in this way is reminiscent of our own barred-spiral galaxy, the Milky Way. As of 2018 five supernovae have been observed in M-66: SN-2016cok, 2009hd, 1997bs, SN-1989B, and 1973R. SN-1989B was discovered independently by amateur astronomers Mike Petrasko and Dale Alan Bryant - one, cold, still morning in Feb of that same year.

Lastly, NGC-3628, the edge-on galaxy in this trio is also known as the "hamburger" galaxy. (Yes - it does indeed look like a "quarter-pounder" - viewed from the side!) Its disk spans 90tly and sits at 35mly away. The galaxy is composed mostly of older stars and like the other two is easily visible in amateur-class telescopes (4+ inches of aperture diameter). NGC-3628 also sports a 300tly-long, 'tidal tail', connecting the other two galaxies. It is the most distant of the three at 35mly. Its disk is around 100tly across.

Since there has been so much supernovae activity within at least one of the galaxies in this trio, I've decided it would be a good idea to begin an extra-galactic supernova search program using these three 'island universes.

So, here's the plan: take images of the three galaxies all within a single frame at some periodic interval (time series). Using an image of the three together that is known to be "supernova-free" - I can then compare subsequent images over time to the SN-free frame using a sort of 'blink comparator.

A blink-comparator is a device that was used frequently by astronomers to compare images of the same area of sky or objects within the same field of view of a telescope or camera over a specified interval. It involves the rapid sequencing back-and-forth of two images - one against the other. (In the distant, remote, ancient past - (*chuckle*: 1980's), I used two Kodak carousel slide projectors one stacked on the other projecting both slides at the same time onto a screen and then using a sheet of cardboard manually to alternately project the slide images one at a time in rapid succession onto the screen.

Currently, I'll use the two images in an animated, ".GIF", file, and "blink" them, that way. In this fashion, I can set the "blink" rate, and interval, for optimal comparison. In this way, any deviation from the standard field (used as a sort of, 'control group'), such as a blinking spot, line, or another anomaly, will stand out as extraneous data. This was how, Dr. Clyde W. Tombaugh, discovered the dwarf planet Pluto back in 1930. I'll be looking for any supernova activity within the three galaxies.

This is something that anyone using one of Insight Observatory's, remote telescopes can do on their own! It's a good way to involve oneself self in a Citizen Science project - of their own design!

I'll let you know if I find any action! -- you let me know what you find too!!

Dale Alan Bryant
Senior Contributing Science Writer

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Searching for Extragalactic Supernovae

I'll soon be doing an extragalactic supernova search, monitoring a small group of 5 or 6 spiral galaxies, similar in structure, to our Milky Way, barred-spiral galaxy - in the Virgo galaxy cluster.

The Virgo Cluster of galaxies is (around) 30-50 million light-years from the "Local Group" - the Milky Way's home, galactic cluster. The Virgo galactic cluster contains a spiral galaxy, M66, in the constellation Leo. It is some 35+ million light-years distant.

Back on 11 February 1989, at around 02:15am EST, Insight Observatory Managing Member and Project Developer, Michael Petrasko, and I, independently co-discovered a supernova (SN1989b), within one of the outer spiral arms of M66 (Michael, was the actual discoverer; I just "looked"!).

The Local Group and other galaxy cluster groups. Graphic by Dale Alan Bryant.

Supernova events within any given galaxy are estimated to occur only two or three times in a century. I'll see if I can refine that estimate, somewhat, over the course of a few months of nightly or bi-nightly photographic time-exposures of the group, using one of Insight Observatory's remote astrographs (photographic telescope) - ATEO-1, or ATEO-2A. The instruments are situated in the western New Mexico region, respectively - some of the clearest and darkest skies in the world.

Typically, an SN burst is so energetic that its brilliance, temporarily, outshines the combined light of all of the billions of stars within a given galaxy. Any SN event will stand out as a tiny, bright, dot, superimposed against the overall, dim, oval blur of light of the main body of the galaxy. It is during a supernova burst that the heavy elements of our universe are forged (iron, nickel, and other heavy metals). From there, the energy of the blast disperses the elemental metals into the surrounding space including any nearby molecular clouds which ultimately condense and become planetary systems (such was the case in our "Solar" system).

This is the history of the metallic content of Earth's mantle and crust, and, its solid iron core.

Dale Alan Bryant
Senior Contributing Science Writer

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The O-TEAM: A Thousand and One Nights - Part 2

Once upon a time, at a tiny cul-de-sac, in the village of North Falmouth, Cape Cod, Mass -

"This morning - was something to remember"...

So the note goes, written in pencil, on an official Edmund Scientific observing notes template, on the warm, sunny morning of 8 May 1983, by one, Mike Petrasko - one-third, of that notorious 3-member "gang" of optical aficionados, the "O-Team".

But, I think the tone of the note, was an understatement;

as observing sessions go, this one was outstanding, on several accounts! We had a guest for this session, a friend of Mike's, Shawn, who had never really had an opportunity, before this, to observe the sky with a telescope (and - he may not have, since!)

I arrived, on location, at around 2:00am. The others - Mike, Muir, and Shawn, were just waking from a short night's sleep, camped out at the center of an unused, undeveloped, someday-to-be, cul-de-sac neighborhood called, "Camelot Court", in North Falmouth, Mass. We had chosen this location for its proximity, open view of the sky, and, for its relative isolation from outdoor lighting - and other, unwelcomed intrusions.

In the span of 3 hours of telescope time, we had assessed, 5 Messier objects, an unknown open cluster, an unknown globular cluster (to us, at the time), and 8 sporadic meteors.

The wee hours of the night present some of the best opportunities for the amateur observational astronomer: fewer episodes of sporadic lighting, fewer people, less traffic, increased meteor activity, and, most of all, quiet.

M57, The Ring Nebula in Lyra imaged on ATEO-1 processed by Utkarsh Mishra (left), and M27, The Dumbell Nebula in Vulpecula imaged on ATEO-1 processed by Michael Petrasko (right).

Our, "optical ambush", begins with M57 - the "Ring" nebula, in Lyra. Though this emission nebulosity does, indeed, appear ring-like through the eyepiece, that is an illusion of perspective. This structure is, in reality, a spherical shell of excited gas molecules, outlining the shock bow from a centralized supernova event. M56, to me, has always appeared to be, a lone "Cheerio", floating in the darkness! It sits, almost squarely, between the two, lower corner stars of the "lyre" shape, Gamma and Beta Lyrae. It can be observed well with a 4" telescope.

The next object was M27, in Vulpecula - the "Dumbbell" nebula.

This, also, can be seen easily in a 4" inch scope. I know this, because Mike had a 4" Edmund Scientific Astroscan, at the time, and usually found these objects before I did. It is a twin-lobed remnant, also of a supernova. Burnham's Celestial Handbook describes it as, "large and shining", at several times the size of M57. About then, we broke out some nutrition to keep up our ambitions: "Nutty Bars", "M&M's" (plain), and a bag of "Doritos". Now, there's some "energy food"!

Edmund Scientific's Astroscan 4" f/4.2 reflector telescope (left) with the original observing log entry this post was adapted from back on May 8th, 1983 written by Insight Observatory Co-Founder Michael Petrasko when he was 17 years old. Image credits: Astroscan - Glenn Votava, Observers Log - Dale Alan Bryant.

Next on our list was M13 - the Hercules cluster (globular cluster, not referring to the cluster of galaxies within that constellation). Easily seen in good binoculars, this is one of my favorite collections. Of stars, that is. A nearly, perfectly symmetrical, uniformly dense, globe-shaped cluster of stars within the halo of globular clusters that orbits the Milky Way galaxy. Well, that's a technical description – but, see it for yourself, and you'll likely choose other, more prosaic wording, I'm sure of it.

M11 - is an open star cluster in the constellations Scutum. Open star clusters are loose congregations of stars, bound together, gravitationally, as are globular clusters, only, not as tightly. It's commonly called, the "Wild Duck" cluster (for reasons I never quite grasped). I have a favorite open cluster, not on this list: the double cluster, NGC'S 864 and 889, in Perseus. At over 7,000 light-years, the stars in the cluster appear as tiny, brilliant, and colorful jewels.

M13, The Great Hercules Globular Cluster imaged on ATEO-1 processed by Utkarsh Mishra (left), and M51, The Whirlpool Galaxy in Canes Venatici imaged on ATEO-1 processed by Michael Petrasko (right).

Next up, M51 - the "Whirlpool" galaxy. M51 is another "Grand Design" spiral galaxy, in reference to its near-perfection. Actually, it's an interactive pair of galaxies - the larger one, slowly consuming the smaller of the two. Located in Canes Venatici, its brightness and relative isolation in the darkness make it an easy target for small scopes.

As for the unknown open and globular clusters, I could only guess at what they would have been; likely, something in Ophiuchus - an area, rich, in such wonders.

And that leaves eight meteors; possibly, or not, connected to the Eta Aquarid meteor shower. Meteors are a fascinating subject, all on their own. The months of April and May have, historically, produced some very large fireballs and bolides, in historic times. Ask Mike or me, about that, sometime!

Dale Alan Bryant
Senior Contributing Science Writer

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