Tag Archives: Trapezium

NASA Night Sky Notes: The Orion Nebula – Window Into A Stellar Nursery

Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. Your tax dollars help promote science! The following article was provided for reprinting by the Night Sky Network in December, 2019.

By David Prosper

Winter begins in December for observers in the Northern Hemisphere, bringing cold nights and the return of one of the most famous constellations to our early evening skies: Orion the Hunter!

Orion is a striking pattern of stars and is one of the few constellations whose pattern is repeated almost unchanged in the star stories of cultures around the world. Below the three bright stars of Orion’s Belt lies his sword, where you can find the famous Orion Nebula, also known as M42. The nebula is visible to our unaided eyes in even moderately light-polluted skies as a fuzzy “star” in the middle of Orion’s Sword. M42 is about 20 light years across, which helps with its visibility since it’s roughly 1,344 light years away! Baby stars, including the famous “Trapezium” cluster, are found inside the nebula’s whirling gas clouds. These gas clouds also hide “protostars” from view: objects in the process of becoming stars, but that have not yet achieved fusion at their core.

The Orion Nebula is a small window into a vastly larger area of star formation centered around the constellation of Orion itself. NASA’s Great Observatories, space telescopes like Hubble, Spitzer, Compton, and Chandra, studied this area in wavelengths we can’t see with our earthbound eyes, revealing the entire constellation alight with star birth, not just the comparatively tiny area of the nebula. Why then can we only see the nebula? M42 contains hot young stars whose stellar winds blew away their cocoons of gas after their “birth,” the moment when they begin to fuse hydrogen into helium. Those gas clouds, which block visible light, were cleared away just enough to give us a peek inside at these young stars. The rest of the complex remains hidden to human eyes, but not to advanced space-based telescopes.

We put telescopes in orbit to get above the interference of our atmosphere, which absorbs many wavelengths of light. Infrared space telescopes, such as Spitzer and the upcoming James Webb Space Telescope, detect longer wavelengths of light that allow them to see through the dust clouds in Orion, revealing hidden stars and cloud structures. It’s similar to the infrared goggles firefighters wear to see through smoke from burning buildings and wildfires.

Learn more about how astronomers combine observations made at different wavelengths with the Night Sky Network activity, ‘The Universe in a Different Light,” downloadable from bit.ly/different-light-nsn. You can find more stunning science and images from NASA’s Great Observatories at nasa.gov.

This image from NASA’s Spitzer missions shows Orion in a different light – quite literally! Note the small outline of the Orion Nebula region in the visible light image on the left, versus the massive amount of activity shown in the infrared image of the same region on the right. Image Credit: NASA/JPL-Caltech/IRAS /H. McCallon. From bit.ly/SpitzerOrion

The Night Sky Network program supports astronomy clubs across the USA dedicated to astronomy outreach. Visit nightsky.jpl.nasa.gov to find local clubs, events, and more!

CNYO Observing Log: Baltimore Woods, 5 April 2013

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Bob Piekiel’s monthly session at Baltimore Woods featured crystal clear skies, increasingly cold conditions (a recurring theme this year for all of the previous sessions), and one large scope.

This Baltimore Woods session was the last scheduled event before our Winter constellations all-but disappear from our nighttime skies. To this pressing deadline was added the last reasonable observation of Comet panSTARRS (C/2011 L4) from the same location, as the return of the foliage through May will all-but obscure the parts of the North/NorthWest horizon that are not already obscured by naked branches. The event itself was scheduled from 7:30 to 9:30 p.m., ending an hour before any first observation of Saturn for the evening. The ever-dropping temperature that evening found us ending the session promptly to the sound of running (with heat on full-blast) cars and depleted propane.

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Bob Piekiel and the author post-assembly.

With a confirmed heavy lifter attending (me), Bob opted to bring out a 16” Meade SCT on a homemade tripod that is (minus the scope) transported in the open – the whole considerable contraption hitches to the back of the car. After a bit of heavy lifting and careful coordination to get the scope up to the mount, the completed assembly was ready for the first signs of bright stars (in this case, Sirius and Capella) to perform the alignment. The time waiting for bright star arrivals was passed with the help of a pair of Zhumell 25×100’s that saw (1) clear views of Jupiter and all four of its largest moons and (2) Sirius in Canis Major to the West.

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Bob Piekiel putting the finishing touches on a 16″ Meade SCT.

The height of the tripod combined with the extra 8” of wheels on the mount’s base meant that a step ladder was required for nearly all viewing throughout the night. With the 16” SCT aligned, the first official view (pre-dark sky) was of Jupiter, which was bright and clear in Bob’s 40 mm Meade eyepiece. The second object was Trapezium in the Orion Nebula (M42), which was also crisp and clear despite our observing it only minutes after sunset.

The third object observed combined low brightness with near-horizon position just past dusk. Bob managed to find Comet panSTARRS almost due North of the Andromeda Galaxy just as it was about to hit the bare tree line. The view was excellent for several minutes as everyone had a few looks at this increasingly difficult-to-observe object (comet’s center was reasonably well defined, but this was a 16” scope with a 40 mm eyepiece). And, it should be noted, the object database in Bob’s GOTO computer is not only older than the discovery of Comet pan-STARRS, but also quite a bit older (decade? maybe two?) than the Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) that originally identified the comet. So, extra kudos to Bob for the timely find!

The cold set in quickly after these first three objects, meaning the last four objects for the evening were approached with haste. In a return to the objects of his last session, Bob treated attendees to excellent dark views of M65 and M66 in Leo, M108 (a faint edge-on galaxy near the Owl Nebula in Ursa Major that was as bright in the 16” as it was with Bob’s 11” scope + image enhancer), and the Owl Nebula (M97). Bob and I saw this final object as a confirmation that it hadn’t flown the coop during our last session, where the image enhancer failed to produce any particular view of this object (see the last session notes for details).

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New supernova in M65. Photo by Felipe Pena.

NOTE: I wish I had known earlier that a new supernova was discovered in M65! As a general point of reference, those looking for the most complete and up-to-date information about supernovas are directed to David Bishop’s excellent Bright Supernova database and log at www.rochesterastronomy.org/supernova.html. Details and many, many images of the new supernova in M65 can be found at: www.rochesterastronomy.org/sn2013/sn2013am.html

The totality of views through the Zhumell 25×100’s were limited to Jupiter (as a sampling for the attendees before the 16″ was properly GOTO’ed), Sirius (just to the left of Orion and the brightest star in our Night Sky), the Double Cluster in Perseus (bright and densely packed), and the Pleiades (M45), the object for which I assume 25×100’s were originally designed to observe (near-perfect fit of the whole cluster in the field of view).

A few street lights and distant clouds to the East reflecting Syracuse back down provided all the illumination that the stars didn’t as we began to pack up the gear at 9:30 p.m.

And did the 3rd Quarter Moon affect the viewing? For those observing at “reasonable” hours, it is the case that the 3rd Quarter Moon doesn’t rise until midnight, meaning the week before a Full Moon, the week of a Full Moon, the few days before a 1st Quarter are excellent for getting outside to observe deep sky objects at “reasonable” hours (reasonable being relative, of course).

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Not a lunar landing scene. Mid-way through the 9:30 pack-up.

Next session is scheduled for May 4 (Saturday) – 5 (Sunday), 8-10 p.m. and will feature Jupiter, Saturn, and hopefully a few shooting stars from the Eta Aquariids meteor shower. For details and registration, see the details on this CNYO page.

CNYO Observing Log: 2013 March 8 At The Syracuse Inner Harbor

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This past Friday (2013 March 8), CNYO hosted its first official public observing session at the Onondaga Lake Inner Harbor, centrally located between Downtown Syracuse and Destiny USA. While this may seem like a rather poorly-advised location for amateur astronomy, the Inner Harbor served several simultaneous purposes for the organization and the attending public. I shall consider these points below intermixed with a brief discussion of the event itself.

Setup began with Larry Slosberg and myself around 6:00 p.m., arriving early enough to reserve the large mound just behind the Inner Harbor amphitheater (map below) and generally take in the location. While a somewhat out-of-the-way location (in the desert between the mall and downtown), the Creekwalk provided traffic in the form of a few joggers, dog walkers, and cyclists (and, as it happened, part of our audience for the evening). The Inner Harbor itself is a very large space full of parking, calm water, airplanes into and out-of Hancock International Airport (the take-offs, approaches, and landings themselves were fun to watch) and reasonably distant horizons. All of Syracuse is visible from the mound, serving as a familiar backdrop for bright stars as they came above the horizon (and it’s just a really neat spot to take the city in – I’d recommend it to everyone when the temperature increases). The only point of minor concern was the murder of crows parked near the city school bus depot, which lead to us all keeping our scopes tilted to the ground when not in use (to spare out primary mirrors from collecting anything falling from above). The location is surrounded by sodium lights and some rather bright walking path lights. Remarkably, Destiny USA was not the major source of light pollution for the area (a bit of a tree line actually kept the mall’s glare to a minimum). As a result of the Inner Harbor and Creekwalk lights, all decent observing began about 30 degrees off the horizon (where the glare and reflection of city air particulates gives way to darker, steadier skies).


View Larger Map

Within minutes of Larry getting his Meade set up, the first public visitors appeared in the form of three teens walking past the Inner Harbor amphitheater. While I was busy setting up my 12.5” Dobsonian (herein referred to by her name, “Ruby”), Larry had Jupiter in his scope (easy to see immediately after sunset and the first celestial object to appear for several minutes before Sirius, Betelgeuse and Rigel marked their respective locations) and was describing the sight as everyone took turns with first views of the evening. Larry and I both tried to see Comet Pan-STARRS in the West/SouthWest sky, but it is clearly too early in its appearance (and too low on the horizon) for CNY viewing (perhaps the skies will clear over the next few days). By 6:30 p.m., Larry (Meade), Ryan Goodson (with two New Moon Telescope Dobsonian beauties in tow), Dan Williams (running one of the Ryan’s), Simon Asbury (with two testing pairs of Zhumell 25×100’s) and I (Ruby) had equipment out and were observing, as Barlow Bob describes it, “with attitude.” John Giroux appeared soon after with two scopes, marking the peak of operating optics for the evening.

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Setup at sundown.

So, The Big Question!

What can one see from near-Downtown Syracuse when surrounded by sodium lights and a glowing skyline? In my 12” Dobsonian, my public observing list for the evening consisted of:

* Jupiter – clearly visible banding, obvious Great Red Spot, nicely steady skies for pulling out detail.

* Pleiades – fit perfectly in its entirety in my Pentax XL40 eyepiece. The coloring in my favorite binary system (Tyc1800-1961-1 (blue) and Tyc1800-1974-1 (orange)) was clear as a bell.

* Trapezium in M42, the Orion Nebula – all 6 stars were no problem.

* The rest of M42 – the filamentous nebulosity is still obvious at any magnification.

* M41 (the “Little Beehive”) in Canis Major – A multi-colored open cluster one full Telrad diameter from Sirius, the brightest star in the Night Sky. Orange and slightly blue stars were easy to see.

* M31, The Andromeda Galaxy – just a circular fuzzy ball with barely any additional structure present. But it was obviously a galaxy in the scope (and in the near direction of Destiny USA to boot).

* In Ryan’s 16” NMT Dobsonian, I was able to just barely make out M65 and M66, two of the three galaxies in the Leo Triplet (NGC 3628 was just outside of visible).

All together, that isn’t a bad list of observed objects even in dark sky locations, and several other open clusters would have been easily visible from the Inner Harbor had I focused on them (and perhaps others did).

This brings me to a lesson that I hope others planning sidewalk astronomy and similar events keep in mind (and clearly comes with my own bias). The goal of a public viewing session should not be to introduce completely new observers to subtle, dim objects that even professional amateurs require time and training to see. The goal of the session should be to expose new eyes to clear, bright objects that don’t require averted vision or averted imagination. It is commonplace in all manner of scientific endeavor for a professional to forget that they spent 10 years getting to the point where something is obvious. You can describe what someone is supposed to see all you want, but a dim face-on spiral galaxy with any appreciable NGC designation is not going to wow someone like Jupiter or the Moon. I’ve made it a point in several past observing sessions to try to get several scope owners to pick tiers of objects, with someone focused on the bright clusters and planets, then someone else focused on objects that tax the new observer who really wants to see what amateur astronomers consider to be tempting targets (and this tier-based approach has worked and failed to varying degrees).

Observing from the lit surroundings of a city does wonders for removing the dim fuzzy-wuzzies from the list of objects scope runners might consider as interesting objects. Very quickly, the observing candidates for a trained amateur astronomer reduces to the list of objects most anyone can observe and appreciate with little description beyond the interesting physics and history of the objects themselves. New observers are not taxed with seeing subtle detail. Clusters, many binaries, and planets become the pick hits that keep the crowds cycling between scopes (and are also good for new amateur astronomers, as these objects are usually the easiest to find). The Inner Harbor, despite its flaws as a location for dedicated amateur observing, is a choice location for introducing new people to an ancient craft (that, then, hopefully draws them out to darker skies). Frankly, I’m looking forward to a first Moon-centric observing session for this very same reason.

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Some of the attendees pose for a first group shot. Photo by Simon Asbury. See the CNYO facebook page for more photos. From left: Mike Phelps, Larry Slosberg, John Giroux, Dan Williams, Ryan Goodson, Damian Allis, and Jack Allen.

The session concluded with a father and daughter spending several minutes with Ryan’s scope as we all talked observing, science, and general light conversation. In all, around 20 people showed, all but five of whom were somehow connected with the facebook page. Ryan, John, and I finally packed the last of our gear (and did the last search for dropped eyepiece caps) just after 10:00 p.m., a good hour after the city became quite frosty (we definitely would not have lasted to Saturn’s arrival after 11:00 p.m.).

All in all, the first official event was excellent! All had a good time despite the cold, I had my scope out earlier in the year than ever before, much observing was had through many optics, all enjoyed a broad range of conversation around the scopes, we all learned a bit about what light pollution REALLY means to city observers, and the CNYO attendees all agreed that this is something we definitely need to do on a regular basis. Therefore, stay tuned to the website and facebook page for observing announcements, hopefully with another (warmer!) nighttime session to follow after our daytime appearance at The MOST on April 2nd for their Climate Day event.

CNYO Observing Log: Baltimore Woods, 9 February 2013

Ryan Goodson, Larry Slosberg, and I joined Bob Piekiel for his monthly New Moon observing session at Baltimore Woods on his weather-alternate session (having lost Friday’s session to Snow Storm Nemo). What started as a remarkably cold session, which then progressed to a bitterly cold session, and then finally to an intolerably cold session (forcing us to close shop up around 8:30 p.m.), still provided some excellent views of the Winter Sky, including the Solar System‘s largest planet Jupiter right between the Hyades and Pleiades.

For those who haven’t ventured for a session, the view from the Baltimore Woods parking lot includes a clear zenith (what luck!), a tree to the North that extends almost up to Polaris (so one must walk around it to get the view of constellations below our North Star), low-lying trees to the West, then the warm orange glow (the only thing warm on the 9th) of Baldwinsville and Syracuse to the East-Southeast. As we’re mid-winter, the evening observing was obstructed occasionally by blindingly bright snowmobiles (but one had plenty of lead time to take cover).

The evening started early with a fly-by of the yellow-orange ball that is (from the ground, anyway) the International Space Station (ISS), right on schedule with the predictions from heavens-above.com:

Date Brightness Start Highest point End Pass type
[Mag] Time Alt. Az. Time Alt. Az. Time Alt. Az.
09 Feb -3.3 18:55:57 10° SW 18:59:16 68° SE 18:59:56 51° E Visible

Reaching a total session count of eight, the evening included several observations of Jupiter, noting specifically how quickly Io rushed from Jupiter as even 10 minute intervals progressed (the slow cooling of mirrors resulted in many returns of increasingly crisp views). A comparison of eye piece magnifications and field-of-views was performed with the Pleiades in Bob’s 11″ Schmidt–Cassegrain and Ryan’s 16″ NMT Dob. In both cases, one my my favorite doubles, Tyc1800-1961-1 (blue) and Tyc1800-1974-1 (orange), jumped right out from the center of the tea cup. The lesson learned from such an exercise is that magnification is not the key to observational astronomy – it is seeing all that you want to see in the field of view that is key to enjoying the Night Sky.

A second highlight of the evening included M35, an open cluster in Gemini that, at 2,800 light years away, still covers an area the size of the Full Moon. Clearly visible as a slight “smudge” in the upper-left corner of the eyepiece (so the lower-right corner of M35) at low magnification is the compact open cluster NGC 2158.

After Jupiter, the night belonged to the massive Orion Nebula (M42), a hydrogen cloud doubling as a stellar nursery. At a magnitude of +4.0, the fuzzy patch in Orion’s Belt is visible to the Naked Eye, increasing in density with small binoculars, and leading to magnificent views of filamentous nebulosity at low magnification in both telescopes. The splitting of the main binaries in Trapezium was trivial in Ryan’s 16″ NMT Dob even without a completely cooled mirror.

I noted to Ryan that, given the usual CNY winter conditions, “It’s a rarity to see Pegasus in the West.” The quintet of Sirius, Orion’s Belt, the Hyades, Jupiter, and the Pleiades was worth the visit with or without equipment. After 90 minutes of observing in cold, continually patchy skies, the temperature dropped precipitously, instigating a rapid retreat and scope packing by all attendees. The lessons learned – your gloves are never thick enough & always have a headlamp in the car for the end of the evening!