Author: Tammy Plotner

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Greetings, fellow Stargazers! Were you up early this morning? If so, you were greeted by an awesome scene, much like this one captured by Danilo Pivato. There’s nothing more eyecatching the a close appearance of Venus and the Moon! With dark skies this weekend, it will be a good opportunity to broaden your astronomical horizons by chasing lesser known objects in both binoculars and telescopes. Of course there are challenges, too! Whenever you’re ready, I’ll see you in the back yard….

Friday, October 16 – Celestial scenery alert! Be up and outside this morning before dawn. The incredible duo of Venus and Saturn will be joined by the Moon! In 1982, the 30th return of Halley’s Comet was observed with the 5-meter (20000) Hale Telescope at the Mount Palomar Observatory. The comet was beyond the orbit of Saturn!

Tonight let’s head toward the region of Cas A and see what we can find. Although Cas A is itself not visible in amateur equipment, it is known to be associated with a 10,000-light-year-distant supernova remnant related to an unnoticed event occurring more than 300 years ago. The remnant itself has now expanded to a region filling some 10 light-years of space and has been imaged using orbiting X-ray observatories.

The closest deep-sky study to Cas A is the dense and compact open cluster NGC 7510 (RA 23 11 00 Dec +60 34 00). This diminutive, magnitude 7.9 study can just be glimpsed as a hazy patch in large binoculars and small scopes, with a few of its brightest 10th magnitude members resolvable at higher magnifications. Doubling the aperture brings out a dozen or so of NGC 7510’s 12th magnitude stars against the teeming glow of numerous fainter members. Double the aperture again, and 60 stars to magnitude 14 are possible. Many amateurs have discovered that the combination of a small rich field refractor, a 600 apochromatic refractor, and a 1200 Newtonian makes for the ultimate in observing equipment. But don’t forget those binoculars!

Saturday, October 17 – Today we mark the birth of Dr. Mae C. Jemison, the first black woman to go into space! Tonight let’s revisit M39 and use it as our touchstone to seek out other deep-sky gems. Starting with M39, head less than two finger-widths east-southeast (RA 21 53 32 Dec +47 16 06) to a 7.2 magnitude open cluster, one associated with the 12th magnitude ‘‘Cocoon Nebula.’’

Collectively known as IC 5146, this cluster with nebulosity consists largely of 12th magnitude stars and is just about mid-sized. Barely detectable in a small scope, this 4,000-light-year-distant cluster needs aperture to come out and play. Large scopes may make seeing the nebula possible, although an appropriate filter may be necessary from most observing sites. To assist in finding the Cocoon, look for the stream of the dark obscuration nebula B168 touching its eastern frontier.

Returning again to M39, head two finger-widths southwest in the direction of Deneb to seek 6.8 magnitude IC 1369 (RA 21 12 06 Dec +47 44 00). Mid-sized instruments will show a dozen or so 12th and 13th magnitude members within a misty haze of those waiting to be resolved. Also known as alternative catalog study Pechue (AN 3259), IC 1369 has been studied for luminosity features.

Sunday, October 18, 2009 – Tonight it’s a New Moon! Time to break out the muscle and challenge big telescope users to hone their skills. It’s galaxy-hunting time, and our destination for tonight is the Hickson Compact Group 87 (RA 20 48 11 Dec -19 50 24).

Several billion years ago, on the ecliptic plane about 4 degrees west/southwest of Theta Capricorni, and around 400 million light-years from our Solar System, a galactic association decided to form its own ‘‘Local Group.’’ Orbiting around a common center every 100 million years, their mutual gravity is pulling each of them apart, creating starbursts and feeding their active galactic nuclei. Small wonder they’re shredding each other. They’re only 170,000 light-years apart! One day HCG 87 may even form a single elliptical galaxy bright enough for the average telescope to see, but as they are now, this group isn’t going to be seen with anything less than 20 inch aperture.

So, shall we try something a little more within the realm of reality? Then go ahead and drop about 8 degrees south of Theta, and try picking up on the NGC7016/17/18 group (RA 21 07 20 Dec -25 29 15). Are they faint? Of course! It wouldn’t be a challenge if they were easy, would it? With an average magnitude of 14, this tight trio known as Leavenworth 1 is around 600 million light-years away. They’re very small and not very easy to locate, but for those who like something a bit different, give it a try!

Until next week? Dreams really do come true when you keep on reaching for the stars!

This week’s awesome images are (in order of appearance): The Moon and Venus: Courtesy of Danilo Pivato of Northern Galactic, NGC 7510, IC 5146, IC 1369, Hickson Compact Group 87 and NGC 7016/17/18 (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!

Greetings, fellow SkyWatchers! It’s a much darker weekend – and just in time for the Draconid Meteor Shower! If you haven’t been watching the early morning trio of Venus, Mercury and Saturn, there’s still time… Just as there is time to chase a couple of Caldwell Objects and a very challenging galaxy study for more practiced observers. But we’re not forgetting small scopes and binoculars either as we take a look at “What was Charles Messier thinking when he recorded M73?” It’s time to turn your eyes to the skies and I’ll see you in the dark…

Friday, October 9, 2009 – Have you been watching our early morning planetary conjunction? Mercury was nearly touching Saturn 24 hours ago! If you’re up early over the next few days, enjoy celestial mechanics in action as Venus, Mercury and Saturn slowly shift their positions in the sky.

Tonight is the peak of the northern Draconid meteor shower, whose radiant is near the westering constellation of Hercules. This particular shower can be quite impressive when comet Giacobini–Zinner passes near Earth. When this happens, the fall rate jumps to 200 per hour and has even been known to reach 1,000. Comet Giacobini–Zinner reached perihelion on July 2, 2005, passing within 8 million kilometers of Earth but has now greatly distanced itself from our region of the Solar System. Chances are the Draconids will produce only about 3–5 meteors per hour, but this number can vary.

Tonight’s skies remain dark into the early hours, so let’s take this opportunity to have a look at two objects from one of the more obscure catalogs. Set your sights on Alpha Pegasi, and drop due south less than 5 degrees to pick up NGC 7479 (RA 23 04 56 Dec +12 19 23).

Discovered by William Herschel in 1784, this 11-magnitude barred spiral galaxy experienced a supernova as recently as 1990. Although the 16th magnitude event near its nucleus is no longer visible, modest telescopes will easily pick out the bright core and elongation of the central bar. Larger aperture will find this one a real treat, as the spiral arms curl over and under the central structure, resembling a ballet dancer en pointe.

Congratulations! If you’ve found it, you’ve just observed Caldwell 44.

NGC 7814 is easy enough to find. Start at Gamma Pegasi and use the finderscope to center on a star around 3 degrees northwest (RA 00 03 14 Dec þ16 08 43). In the scope, look southeast to see NGC 7814 as a scratch of light in the low power field. Magnify and enjoy! This galaxy has a deeply concentrated nucleus and a very prominent dissecting dark dust lane. This one is also known by another name, Caldwell 43.

Saturday, October 10, 2009 – On this date in 1846, William Lassell was busy at his scope as he made a new discovery, Neptune’s moon Triton. Although our everyday equipment can’t ‘‘see’’ Triton, we can still have a look at Neptune! You’ll find it on the ecliptic around 21:45 in right ascension. On this date 140 years later (1986), a tiny asteroid, Asteroid 3753, was found orbiting Earth. Named Cruithne, the little body will orbit our Earth for at least another 5,000 years from a minimum distance of 15 million kilometers. While time and the stars appear to stand still, and astronomical twilight begins earlier each night, let’s take one last look at the exiting constellation of Sagittarius. Our return study for this evening is a telescopic challenge for skilled observers only. Set your sights about 2 degrees northeast of easy double 54 Sagittarii and around 7 degrees west of Beta Capricorni (RA 19 44 58 Dec –14 48 11), and let’s have a look at NGC 6822.

Often referred to as ‘‘Barnard’s Galaxy’’ for its discoverer (E.E. Barnard, 1884), this unusual customer is actually a member of our local galaxy group. For the 400–600 telescope, this 11th magnitude, 1.7-million-light-year-distant object will not be easy to see, but it can be achieved with good conditions. Lower power is essential in even larger scopes, and those into the 1200–1600mm range will see NGC 6822 burst into stunning resolution. Barnard’s Galaxy almost appears like an open cluster overlaid with nebulosity, but the experienced eye will clearly see that the ‘‘shine’’ behind the stars is galactic in nature. It’s a very clumpy and unusual galaxy, one that you will very much enjoy. Be sure to look for the small, pale blue, 10th magnitude planetary nebula NGC 6818 in the same field to the north-northwest. This pair rocks!

Sunday, October 11, 2009 – Today we begin with the 1758 birth on this day of Heinrich Olbers, a German astronomer who calculated the orbit of the 1779 comet, discovered the minor planets (asteroids) Pallas (1802) and Vesta (1807), and discovered five comets during his career. Tonight we’ll have a look at a collection of stars as we ponder the age-old mystery of M73. Located about three finger-widths north-northwest of Theta Capricorni (RA 20 59 00 Dec –12 38 00), this 9th magnitude open cluster consisting of four stars was discovered by Charles Messier on October 4, 1780. Messier described it as a ‘‘cluster of three or four small stars, which resembles a nebula at first glance. . ..’’ Hotly debated as to whether or not the grouping is a genuine cluster or simply an asterism, it was also included in J. Herschel’s catalog (GC 4617) and given the NGC 6994 designation by Dreyer. In 1931, Collinder cataloged M73 as Cr 426, with an estimated distance of 12,000 light-years. Still, the debate about its authenticity as a physically related group continues.

At least two stars show the same proper motion, leading scientists to believe that M73 may be the remnant of a much older and now dispersed cluster—or simply two related stars. Of the 140 stars
investigated in the region, 24 may be real members, including those in Messier’s original observation. Thanks to the work of Hertzsprung and Russell, these candidates fall within the color-magnitude diagram of a 2–3-billion-year-old cluster with Messier’s suspect four being evolved giants. Although more recent data indicate that M73 may simply be an asterism—sharing no common proper motion— you can still enjoy this unusual Messier in even a small telescope!

Until next week? Dreams really do come true when you keep on reaching for the stars!

This week’s awesome images are (in order of appearance): NGC 7479 and NGC 7814 (credit—Palomar Observatory, courtesy of Caltech), NGC 6822 (credit—Local Group Galaxies Survey Team/NOAO/AURA/NSF), Heinrich Olbers (historical image) and M73 (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!