Weekend SkyWatcher’s Forecast – January 22-24, 2010

Greetings, fellow SkyWatchers! I don’t know about everyone else, but most observations here have been of the big M0. Clouds, clouds and more clouds! Perhaps we’re really in a nebula? However, for those fortunate few that do have clear skies, let’s take a look at what’s happening on the lunar surface each night. And, since we’ve got to deal with a little “Moonlight Sonata”, we’ll also inspect some bright stars and alternative catalog studies to add to your knowledge and pleasure of the night sky! Whenever you are ready, dust off your optics and I’ll meet see you in the backyard….

January 22, 2010: Start the astronomical day by observing the 1592 birth on this date of Pierre Gassendi, French scientist, mathematician, philosopher… and the first to use a Galilean telescope to observe a Mercury transit by the projection method. Gassendi was a prodigious observer, known for his humor, and was friends with Cassini, Galileo, Hevelius, and Kepler. His writings included work on falling bodies – a rare coincidence, since the only known piece of ‘‘space junk’’ to ever re-enter our atmosphere and strike a human occurred on the 405th anniversary of his birth!

Let’s begin our weekend by taking a look with binoculars at the first quarter Moon and see what we can discover… First repeat our first litany: #1—Mare Crisium, #2—Mare Fecunditatis, and #3—Mare Nectaris. Head north to the huge area of #4, Mare Tranquillitatis, which appears with its irregular borders. Beneath the smooth appearing regolith, the ‘‘Tranquil Sea’’ basin is cracked and overlapped by accompanying basins – lava spilling and flowing into other areas as large as the Kimberley region of Australia, or three times larger than England! Now, #5 Mare Serenitatis, the ‘‘Sea of Serenity.’’ Home to a violent past, its outer edges appear darker than the interior—mute testimony to continued seismic and volcanic activity allowing the basin to fill with lava more than once. Take a telescopic look at the rilles adorning this lunar desert, whose surface is the size of Italy. Then go north for #6, Mare Frigoris, the ‘‘Sea of Cold.’’ Congratulations on another learning exercise and if you’re thinking about how cold you are, think about how cold you’d be if you were observing Earth from Mare Frigoris!

Now open your eyes and let’s head for the star on Orion’s western shoulder, Gamma. Named Bellatrix, the 243 light-year distant ‘‘Amazon’’ is not actually part of the Orion association. Gamma is a foreground star and is the hottest of its type visually observable. Historically this star was used as a luminosity standard to compare with other stars to check for variability. But it was later discovered that Bellatrix itself is an eruptive variable, changing in luminosity by a few percent over time. It ranges in magnitude from 1.59 to 1.64. Sure, it’s a minor change – but still a change! There are a couple of types of eruptive variable stars, some with a broad range of increase in luminosity and a fixed time line. These types of eruptive variables include flare stars – very faint stars on the main sequence; novae and dwarf novae – which are caused by the sharing of material between evolved stars in binary systems; and supernovae – the violent and uber brilliant end for several classes of star.


Use binoculars to spot a fainter star about a half degree northeast and say hello to alternative catalog study Dolidze 21 (RA 05 26 50 Dec +06 58 30). This loose association of stars contains a few solar types, and many stars fainter than small optics can resolve – an unusual observation for your notes. Here we have what is considered a “poor” open cluster. Not because it isn’t nice – but because it isn’t populous. It is home to around 20 or so low wattage stars of mixed magnitude with no real asterism to make it special.

January 23, 2010: On the Moon the clockwork movement of the terminator has slowly marched across the surface, revealing more lunar landscape and its 12 maria for exploration. While it ticks along the ecliptic, Luna is passing by other orbiting bodies. Want a challenge? Then we’ll pass on the Moon and aim binoculars towards the constellation of Leo and take on an asteroid! Although Vesta isn’t as exciting, now is a good time to practice observing these rocky Solar System bodies. Spinning completely on its axis about every 5.5 hours and spanning 525 kilometers, this Arizona-sized minor planet is a treat for amateurs because its surface is highly reflective. At times Vesta can reach near unaided-eye visibility, but moonlight steals away fainter objects from easy view. Chances are very good that even in a starry field Vesta will be one of the brightest points visible. See if you can discover Vesta tonight!

Looking for an unusual star to spark your imagination? Then set your sights on the westernmost star of Orion’s ‘‘belt’’ – Mintaka. Like clockwork, astronomical objects can also keep incredibly accurate time. Located around 1,500 light-years away, Delta Orionis is a multiple star system: its companion star is almost equal in brightness and orbiting at a clockwork rate of 5.7325 days from only 8 million kilometers away. In astronomical terms, these two white-hot suns are nearly touching! Mintaka is a prime example of a spectroscopic binary star – a pair so close they are only detectable by changes in the stars’ spectra. Its stationary spectral lines proved the existence of interstellar matter! Take a closer look, and Delta Orionis will reveal a visible 6.7 magnitude companion to its north – a challenge well suited to small optics.

January 24, 2010: Tonight, let’s take time to work toward learning more major lunar features by sailing across 12 seas. The key to learning is to repeat these again and again: #1: Mare Crisium, #2: Mare Fecunditatis, #3: Mare Nectaris, #4: Mare Tranquillitatis, #5: Mare Serenitatis, and #6: Mare Frigoris. Excellent work! Now let’s go have a closer look at #7: Mare Imbrium. Identical in size to Saudi Arabia and about one-fourth the size of the United States, the ‘‘Sea of Rains’’ basin was formed 38 million years ago during a dramatic impact causing a Moon-wide series of faults. The massive strike shattered the lithosphere to a depth of 100 kilometers, embedding the impactor as a mascon. Seismic waves traveled through the interior—re-shaping the far side and creating magnetic anomalies—while the basin floor rebounded and flung ejecta 800 kilometers away. Over 500 million years, at least three areas of distinct lava flow poured into the impact basin (the oldest and largest about 1,200 kilometers long), far out-producing any earthly volcano. The youngest and smallest is about 400 kilometers in length, matching our terrestrial Columbia River Flood Basalt, an area stretching from Idaho to the Pacific Ocean! Now, here are some more to learn: #8: Mare Vaporum, #9: Mare Insularum, #10: Mare Cognitum, #11: Mare Nubium, and #12: Mare Humorum. Remember: repeat, repeat, repeat!

Now turn your eyes towards Orion and its Alpha star – Betelgeuse. Early in the evening, Orion the ‘‘Hunter’’ is beginning its journey across the night sky. Alpha stands out as an orangish star in the northeastern corner. It is a giant among stars! Betelgeuse has a long literary history and was one of the most massive stars known. In the mid-1800s, John Herschel observed that Betelgeuse varied in brightness, its light intensity changing by as much as a magnitude in under 6 years. The red giant is continually contracting and expanding to a formidable size – one that would fill the orbit of Jupiter around our own small star. But, it’s not alone…. Alpha also has four companion suns! Estimated to be 6 million years old, the light you see tonight from Betelgeuse left the
star around the time Nostradamus was making his predictions. Should it go supernova tomorrow, it would be almost another half century before this spectacular sight would be seen in our night sky!

Until next week? Ask for the Moon… But keep on reaching for the stars!

This week’s awesome images are an historical photo of Gassendi, lunar images we done by Greg Konkel. Stellar and cluster images are from Palomar Observatory, courtesy of Caltech and the Betelgeuse diagram is courtesy of NASA. We thank you so much!

The Coma Berenicid Meteor Shower Peaks


Awake during the wee hours of the morning? Try heading outdoors for awhile to watch for the “guess-timated” peak of the Coma Berenicid meteor shower on the morning of January 19. It might not be the most prolific meteor shower on record and this might not be the perfect peak, but this year’s presence is making headlines!

Not normally known for kicking up a fuss, the Coma Berenicid meteor shower is active from December 8 to January 23. At best, it might throw a handful of bright meteors per hour, but this year’s activity has already made a stir to eyewitnesses in the UK. According to Associated Content Press, here’s what observer’s have reported:

Graham Riley said, “We were out in Brigsteer, Cumbria, UK to watch fireworks at midnight New Years Eve [2010]. Brigsteer has no street lighting myself and my wife witnessed a huge bright yellow square with four triangular yellow flashes emitting from the main body… it traveled slowly with no sound from NE to SW and burnt out over the Sea— fantastic sight!” Posted on 01/01/2010 at 2:01:10 PM.

Martin Howie said, “My brother-in-law went out to walk the dogs just after the New Year Bells, and came running back in to call me out to see if I could rationally explain what he’d seen over Rosyth, in Fife, Scotland. Suffice to say, I was at a loss for words, seeing 20-25 orange balls streaking across the sky. The whole family came outside, and a few neighbours came to see what the commotion was. My wife saw one meteor break up into 3 parts and fizzle out. I don’t think any of us will be forgetting this New Year anytime soon. Curious as to the lack of TV coverage or Internet postings thus far also.” Posted on 01/01/2010 at 3:01:08 PM

David Pulman, a pilot who has given earlier eyewitness accounts of this spectacular celestial event, said, “My wife has been in a bit of a panic ever since as she fears there is some sort of official news black out! They were very easily visible— no need for telescope or binoculars. They must have been pretty big too in order that we could see them so clearly— and obviously fire balls— to the point of being able to see them (mostly) burn up in the atmosphere.”

Samantha Istead said, “…I feel so lucky because on Christmas night, I saw two [meteors] on their own at 10.39pm in the UK/Sussex. They were massive, lasting about 6-7mins, but scary at the same time.,. and tonight 1st Jan at 12:07am, I saw about 8/9. They were not difficult to spot. I dragged my neighbour out. He was totally freaked by it, Then halfway through one dropped down and we saw smoke fizzle from it, So amazing. It went on for about 10/15mins.”

Lynn, Keith and Emma Aston in Rothertham, South Yorkshire, England said, “Wow what a night! [We] went upstairs to watch the fireworks at midnight New Year’s Eve only to see meteors flying across the sky and burning out into the atmosphere. Must have seen at least 50. Was amazing but scary at the same time. 4 of them were huge and you could see the flames. Never in my life have I experienced what I saw last night and early morning.”

Can you count on a similar experience just by watching tomorrow morning? Not hardly. Meteor showers are fickle things and a rogue stream relies more on being in the right place at the right time. However, you can even the odds out a bit by watching the general area around the constellation of Coma Berenices. The ecliptic plane is visible the world over, and activity will seem to come from a region just east of Leo. The time to begin is several hours after local midnight and best observations will probably occur when the radiant is highest just before dawn.

Traditionally, the Coma Berenicid activity is weak, with an average fall rate of about 7 per hour, it still warrants study. Noted first around 50 years ago, the stream was connected to another minor shower in the same orbit, the December Leo Minorids . Meteoroid streams are traditionally by-products of comets, but in this case the comet had not been confirmed! Observed in 1912 by Australian amateur astronomer B. Lowe, it was officially designated as 1913 I and was only seen four times before being lost to the sunrise. Using Lowe’s observations, independent researchers computed the comet’s orbit, but it was forgotten until Fred Whipple made the association between his photographic studies and the enigmatic comet. By observing the annual shower, Whipple placed the orbital period of Comet Lowe at 75 years, with the two major streams occurring about 27 and 157 years apart. Due to the uneven dispersion of material, it may be another decade before we see some real activity and the time just might be now! Because when opportunity knocks?

Ya’ gotta’ be there to open the door…

Observing Alert: Possible Nova in Ophichus

Image courtesy of K. Itagaki
Image courtesy of K. Itagaki

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Are you ready for some excitement that won’t take an observatory telescope to spot? Then get out your binoculars, because according to CBET 2128 there’s a new object showing its stuff off in the constellation Ophiuchus…

Released by A. Henden in AAVSO Special Notice #187: “CBET 2128 indicates that Hideo Nishimura has discovered a new outbursting object in Ophiuchus. This object has magnitude 8.4 on Jan 15.857UT, and is located at RA 17:39:40.94 DEC -21:39:47.9 J2000. No spectra have been reported, but K. Kadota has inspected the 1997 DSS red plate and finds no object at this position, with a limiting magnitude of 20. This object has now been added to VSX. You may submit observations as N Oph 2010, VSX J173940.9-213947, or with AUID 000-BJS-899. Note that there is a 10.3 magnitude irregular variable a few arcmin west of this position, so do not use it as a comparison star.”

Information on submitting observations to the AAVSO may be found at: http://www.aavso.org/observing/submit/. However, even if you don’t choose to submit an observation, it’s rather rare that an object of this type can easily be observed with even the most modest of equipment. Magnitude 8.4 is easily within reach of small binoculars, and given that most of the world isn’t having the best of luck with weather, you may be one of only a few who get to see it! Use this map to get you in the general area….

Once you have your position in the sky, use this more localized map to help you identify the nova. This field spans approximately 12 degrees – or about the same size as an average binocular field. I’ve filtered the stars to match the magnitude, so look for any star that’s as bright as – or brighter – than what you see within or very near to the red square area. You’ve discovered the nova! (Hint: Look for obvious star patterns that are easy to see, like the group of stars that seems to resemble Orion’s belt and sword just below the target area.) It might take you several tries and several minutes to locate it, but what a reward when you do!

Enjoy your observations….

Weekend SkyWatcher’s Forecast: January 15-17, 2010

Greetings, fellow SkyWatchers! It’s a dark weekend and time to get out and rock the night… If you’re up to the challenge, one of the finest and most exciting objects we’ll study here isn’t a Messier… it’s a comet. And not just any comet – but one that fits right into this time frame in history! Not up to hunting a moving object? Then we’ll take a look at two objects that could resemble comets and not only present a challenge, but add to the fun! Whenever you’re ready, dust your optics off and I’ll see you in the backyard….

January 15, 2010 – In 2006, Stardust was nearing Earth with its payload of cometary dust particles from Comet Wild 2. The tiny interstellar dust particles were collected by the spacecraft Stardust, which on January 15, 2006, completed its 7-year Odyssey in space by returning its samples to Earth. Two years before, on January 2, 2004, Stardust flew through the hail of rocks and dust that make up comet Wild 2’s coma, collecting invaluable samples of cometary particles that will help scientists decipher the history of our solar system. But during its long voyage Stardust also picked up a different type of sample — minuscule particles of interstellar dust that arrived at our solar system from distant stars, light years away. Stardust collected these particles between February and May 2000, and again between August and December 2002, while passing through a stream of dust that flows into our solar system from interstellar space. The stream was discovered quite recently — in 1993 by the spacecraft Galileo, which passed through that region of space on its way to Jupiter. When Stardust flew through the stream, it extended its tennis-racket shaped aerogel collector, picking up and storing the interstellar particles. No such pristine particles from distant stars have ever been collected before! Then, on January 15, 2006, Stardust swung by the Earth once more and released a sample return capsule, which parachuted safely down onto the Utah desert. Nestled within the capsule’s science canister were two sets of samples: cometary particles on one side of the aerogel collector, and interstellar dust on the other. Within days of arrival, mission scientists began extracting the dust grains from Wild 2 and preparing them for shipment to scientists around the world. Don’t forget to participate in StarDust@Home!

If you’d like to collect a little “stardust” of your own, then this weekend is a great opportunity to actually view Comet 81P Wild 2! Holding a near respectable magnitude 10 and cruising through Virgo (rough RA 13 10.7 and DEC -04 48). 81P Wild 2 has a distant and circular orbit which has it about 1.642 AU away from our Sun at the moment and it will continue to brighten slowly over the next couple of months and is expected to be its brightest (magnitude 9) towards the end of March and in early April. While Comet 81P Wild 2 is just a bit too faint to be found with average binoculars, even a small telescope will reveal its diffuse form. It won’t be bright, and it will appear more like a small, round nebulous patch rather than what folks traditionally think of as a comet… But history is out there waiting on you to come and collect on history!

January 16, 2010 – In 1978 on this date, NASA named 35 candidates for space shuttle missions, including Sally Ride as the first female U.S. astronaut and Guion Bluford, Jr., as the first black. In 1973, the Lunokhod 2 mission was beginning its robotic lunar expedition, and in 1969 Soyuz 4 and 5 became the first vehicles to dock in space and exchange cosmonauts. The year 1730 saw the birth of Jean Bochart – publisher of LaPlace’s planet/ecliptic theory. Although eventually beheaded for his politics, Bochart put together Europe’s largest collection of astronomical instruments and was renowned for his calculations of cometary orbits, made jointly with long-time friend and co-observer Charles Messier.

Tonight, venture into Lepus for a faint, round, fuzzy object that might easily be mistaken for a comet in a small telescope or binoculars – Messier Object 79 (RA 05 24 10 Dec +24 31 27). The true beauty of this object is revealed in large telescopes. Behold a globular cluster, one of many densely packed balls of stars that mainly congregate near our galactic center. Discovered by Pierre Mechain and cataloged by Messier in 1780, M79 is on the opposite side of our galaxy, and about 4,200 light-years away. Spanning 118 light-years, this starry sphere may not be an original member of our galaxy at all but an import. Although we can’t see it happening, the Canis Major Dwarf galaxy is slowly being incorporated into our own system, and M79 might very well be a product of this union!

Thanks to Mechain and Messier’s careful notes, William Herschel later recovered M79 and resolved its stars. Although the practice of maintaining an astronomy diary isn’t for everyone, keeping simple records is very rewarding. Make note of the object’s appearance, equipment used, and sky conditions. Observing diaries just like those of Messier and Mechain have led countless astronomers along the road of discovery to all the deep-sky objects we know today!

January 17, 2010 – Celebrate the 1723 birthday of Johann Tobias Mayer, the German astronomer who created the first lunar tables for determining longitudes at sea. His calculations were accurate to within a half degree! Mayer was also the first to develop the “reflecting circle” – a complete circular instrument graduated to 720°. The reflection circle was a welcome addition, because at the time the technology did not had enough accuracy for surveying measurement. To reduce the error, they relied on making the average of three sequential readings over the circle, separated 120º from each other. A very cool instrument that preceded the sextant!

Are you ready for one last cometary object? Then get out there and capture NGC 2261 (RA 6:39.2 Dec +08:44). You’ll find it about 2 degrees northeast of star 13 in Monoceros. Perhaps you know it better as “Hubble’s Variable Nebula”?


Named for Edwin Hubble, this 10th magnitude object is very blue in appearance through larger apertures, and a true enigma. The fueling star, the variable R Monocerotis, does not display a normal stellar spectrum and may be a proto-planetary system. R is usually lost in the high surface brightness of the “comet-like” structure of the nebula, yet the nebula itself varies with no predictable timetable – perhaps due to dark masses shadowing the star. We do not even know how far away it is, because there is no detectable parallax!

Until next week? Keep your feet on the ground and your eyes on the skies! There’s even more about to happen…

This week’s awesome images are (in order of appearance): Artist’s conception of the Stardust spacecraft Credit: NASA / JPL , Sally Ride – Credit: NASA, M79 Credit: NOAO/AURA/NSF, Johann Tobias Mayer (historical image) and the Hubble Variable Nebula by John Chumack. We thank you so much!!

Weekend SkyWatcher’s Forecast – January 8-10, 2010

Greetings, fellow SkyWatchers! While the skies don’t change a whole lot from year to year, how you approach astronomy and what you can do with your “astronomy time” certainly does! We begin the weekend with a variable star and a great galaxy. Ready for more? Then why not tackle an historic learning project with Mars? No scope or binoculars? No problem. There’s still lots of cool things you can do when you know where to look! Whenever you’re ready, I’ll see you in the backyard….

Friday, January 8, 2010 – Tonight we begin by celebrating two births – first Johannes Fabricius (1587). In 1616 he returned from the Netherlands with a telescope to observe with his father David, the discoverer of Mira. The father – son team studied sunspots, and Johannes was the first to submit work on the Sun’s rotation. Precisely 300 years later (and on the anniversary of Galileo’s death), Stephen Hawking was born – who went on to become one of the world’s leaders in cosmological theory. Hawking’s belief that the lay person should have access to his work led him to write a series of popular science books in addition to his academic work. The first of these, “A Brief History of Time”, was published on 1 April 1988 by Hawking, his family and friends, and some leading physicists.

Tonight let’s honor both men as we start with Mira for the unaided eye, binoculars or a telescope. Located in the heart of Cetus the Whale, Mira is one of those variables that even when well placed above the horizon, you can’t always count on it being seen. At its brightest, Mira achieves magnitude 2.0 – bright enough to be seen 10 degrees above the horizon. However Mira “the Wonderful” can also get as faint as magnitude 9 during its 331 day long “heartbeat” cycle of expansion and contraction. Mira is regarded as a premiere study for amateur astronomers interested in beginning variable star observations. For more information about this fascinating and scientifically useful branch of amateur astronomy contact the AAVSO (American Association of Variable Star Observers).

Now for the black hole! All you’ll need to do is starhop about three fingerwidths northeast of Mira to Delta Ceti. About one degree to the southeast you will discover M77. At magnitude 10, this bright, compact spiral galaxy can even be spotted with larger binoculars as a faint glow and is unmistakable as a galaxy in smaller scopes. Its small bright nucleus shows well in mid-sized scopes, while larger ones will resolve out three distinctive spiral arms. But this “Seyfert” Galaxy isn’t alone… If you are using a larger scope, be sure to look for 11th magnitude edge-on companion NGC 1055 about half a degree to the north-northeast, and fainter NGC 1087 and NGC 1090 about a degree to the east-southeast. All are part of a small group of galaxies associated with the 60 million light-year distant M77.

Saturday, January 9, 2010 – Tonight we’re all about Mars. We have precisely 3 weeks to go until opposition – meaning Mars rises as the Sun sets and will be visible all night. This means the Red Planet is very well placed for observing at a convenient time and it’s high time we learned to do some things the “old fashioned way”! Every couple of years Mars comes close enough to Earth for amateur astronomers to do something interesting… measure its distance from Earth using the original method of parallax. The first experiment first carried out by David Gill in 1877 on Ascension Island and now we can do the same from our own backyard. But let’s start with a little history, shall we?

Gill was originally a watchmaker and his love of precision instruments led him into astronomy. Even in those times, employment was scarce… So Gill and his wife set out for Ascension Island to improve the Observatory and measure the solar parallax by observing Mars. But, as all astronomers know, you don’t make a date with the sky – it makes a date with you… and things weren’t about to go easy. From Mrs. Gill’s journal:

“Tonight Mars will be nearer to us – his ruddy glare brighter than ever again for a hundred years, and what if we should not see him? The sun had shone all day in a cloudless sky, but before sunset some ugly clouds rolled up from windward… Six o’clock, and still the heavens look undecided; half-past six, and a heavy cloud is forming in the south. Slowly the cloud rises – very slowly; but by-and-by a streak of light rests on the top of the dark rocks – it widens and brightens, and at last we see Mars shining steadily in the pure blue horizon beneath… How slowly the minutes passed! How very long each little interruption appeared! The wind was blowing lazily, and light clouds glided at intervals across the sky, obscuring, for a few moments, the Planet as they crossed his path. But at last I heard the welcome note “All right,” and then I went to bed, leaving David to add the pleasant postscript of “Evening success” to his letters. When the letters were finished, he gave them in charge to Hill, with orders that they should be sent off at daybreak, and then he lay down to rest.

I now took the watch for the morning. The first hours of my waiting promised well, but before 1 A.M. a tiny cloud, no bigger than a man’s hand, arose in the south, and I called my husband to know what he thought of it. On this, the night of Opposition, the planet would be in the most favourable position for beginning morning observations about 2.30. Now it was but 12.50, and the question came to be—shall some value of position be lost, so as to give a greater chance of securing observations before the rising cloud reach the zenith, or shall we wait, in the hope that this cloud has “no followers”? David began work at once in a break-neck position, with the telescope pointed but a few degrees west of the zenith. How my heart beat, for I saw the cloud rise and swell, and yet no silver lining below. I dared not go inside the Observatory, lest my uncontrollable fidgets might worry the observer, but sat without on a heap of clinker, and kept an eye on the enemy. Five, ten, fifteen minutes! Then David called out, “Half set finished—splendid definition—go to bed!” Just in time, I thought, and crept off to my tent, thankful for little, and not expecting more, for one arm of the black cloud was already grasping Mars.

My husband would, of course, remain in the Observatory for the rest of the night to watch for clear intervals, while I was expected to go to sleep. But how could I? I took up a book and tried to read by the light of my lantern for a few minutes; then I thought to myself, “Just a peep to see whether the cloud promises to clear off.” I looked forth, and lo! no cloud! I rubbed my eyes, thinking I must be dreaming, and pulled out my watch, to make sure I had not been asleep, so sudden was the change. No! truly the obnoxious cloud had mysteriously vanished, and the whole moonless heavens were of that inky blueness so dear to astronomers. While my eyes drank in this beautiful scene, my ears were filled with sweet sounds issuing from the Observatory, “A, seventy and one, point two seven one; B, seventy-seven, one, point three six eight,” Let not any one smile that I call these sweet sounds. Sweet they were indeed to me, for they told of success after bitter disappointment; of cherished hopes realised; of care and anxiety passing away. They told too of honest work honestly done – of work that would live and tell its tale, when we and the instruments were no more; and, as I thought of this, there came upon me with all their force the glowing words of Herschel: “When once a place has been thoroughly ascertained, and carefully recorded, the brazen circle with which that useful work was done may moulder, the marble pillar totter on its base, and the astronomer himself survive only in the gratitude of his posterity; but the record remains, and transfuses all its own exactness into every determination which takes it for a groundwork.”

Gill’s work with Mars was such a success that it redetermined the distance to the sun to such precision that his value was used for almanacs until 1968. He went on to photograph the southern sky and helped initiate the international Carte du Ciel project to chart the entire sky. Now, thanks to the efforts of Brian Sheen of Roseland Observatory and John Clark Astronomy, you can easily participate in the same kind of historic project or get the correct information to “do it yourself” with your classroom or astronomy club.

The project involves photographing Mars and nearby stars – images taken at the same time from a number of different locations around the globe. John Clark is prepared to undertake the mathematical analysis or will provide the method for those wishing to do this themselves. All they are asking is for those groups and individuals who normally take images of stars and planets to contact the Observatory and they will provide you will all the detailed information to get in on the Mars action!

Sunday, January 10, 2010 – On this date in 1946, Lt. Col. John DeWitt, a handful of full-time researchers, and the U.S. Army’s Signal Corps were about to become the first group to successfully employ radar to bounce radio waves off the Moon. It might sound like a minor achievement, but let’s look into what it really meant.

Believed impossible at the time, scientists were hard at work trying to find a way to pierce Earth’s ionosphere with radio waves. Project Diana used a modified SCR-271 bedspring radar antenna aimed at the rising Moon. Radar signals were broadcast, and the echo was picked up in exactly 2.5 seconds. Discovering that communication was possible through the ionosphere opened the way to space exploration. Although a decade would pass before the first satellites were launched into space, Project Diana paved the way for these achievements, so send your own ‘‘wave’’ to the late rising Moon tonight!

Let’s also note the 1936 birth of Robert W. Wilson, the co-discoverer (along with Arno Penzias) of the cosmic microwave background. Although the discovery was a bit of a fluke, Wilson’s penchant for radio was no secret. As he once said, ‘‘I built my own hi-fi set and enjoyed helping friends with their amateur radio transmitters, but lost interest as soon as they worked.’’ But don’t you loose interest in the night sky! Even if you don’t use a telescope or binoculars, you can still look towards Cassiopeia, which contains the strongest known radio source in our own galaxy – Cassiopeia A.

Although traces of the 300-year-old supernova can no longer be seen in visible light, radiation noise still emanates from 10,000 light-years away – an explosion still expanding at 16 million kilometers per hour! So, where is the source of this radio beauty? Just a little bit north of the constellation’s center star.

Until next week? Have fun learning!

This week’s awesome image (in order of appearance) are: Stephen Hawking (public domain photo), Mira courtesy of SEDS (contributed by Jack Schmidling), M77 courtesy of NOAO/AURA/NSF, David Gill (historic image), Mars Hubble Photo, Ascension Island Map (Library on Congress – David Weaver), Mars Retrograde Animation courtesy of Arizona State University, Mars Horizon Map courtesy of Your Sky, Project Diana (public domain image), Cassiopeia A courtesy of Spitzer. We thank you so much!

Weekend SkyWatcher’s Forecast – October 16-18, 2009

Crescent Moon and Venus - Danilo Pivato

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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.

ngc7510

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.’’

ic5146

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.

ic1369Returning 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).

hickson87

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.

ngc7016So, 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!

Weekend SkyWatcher’s Forecast – October 9-11, 2009

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).

ngc7479

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.

ngc7814NGC 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.

ngc6822

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!

olbersSunday, 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.

m73

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!

Weekend SkyWatcher’s Forecast – October 2-4, 2009

Greetings, fellow SkyWatchers! Are you ready to catch the planetary action? Then get thee out into the night, because right now is the perfect time of year to catch all of our solar system bodies in the same day! Be sure to be out on Saturday night, too… Because it’s “Harvest Moon”! Need a little bit more of a challenge? Then fly off to Cygnus as we take a look at two of its most beautiful (and challenging) double stars! Whenever you’re ready, I’ll see you in the dark…

solarsystemFriday, October 2, 2009 – It’s that time of year! Time to be able to see all the planets in 24 hours! If you’re able to get up before sunrise, it’s a good time to watch celestial mechanics in action as Mercury, Venus, and Saturn are beginning to draw together just before dawn. Be on the lookout for Mars nearly overhead. Now is a good time to see details.

If you haven’t spotted Uranus yet, let the Moon be your guide tonight for finding it about 5 degrees south. Even with bright skies, you should be able to distinguish its faint greenish disk from surrounding stars. What of Neptune? The blue world is a bit further from the Moon tonight on the ecliptic, and you’ll find it around 21:45 in right ascension. The last is the mighty Jove. For binoculars and telescopes, Jupiter is definitely the king of the observable planets for detail. Not only can you spot its different zones and equatorial belts, but refractor users can also regularly distinguish the faded Great Red Spot and other fine features, such as white ovals. For all larger apertures, be on the lookout for the moons! It’s very exciting to watch a shadow transit or to catch a Galilean as it reappears from behind the limb. In just a matter of a few hours, Jupiter’s details can change greatly!

For those who still cheer for Pluto’s status as a planet? The tiny god of the underworld still holds its place in our Solar System. . .and the sky! You can find it during the early evening around 18:02 in right ascension. Good luck on your planet quest!!

Saturday, October 3, 2009 – When the Universal Date changes tonight, the Moon will become full, and this will be the one closest to the autumnal equinox. Because the Moon’s orbit is more nearly parallel to the eastern horizon, it will rise near dusk for the next several nights in a row. On the average, the Moon rises about 50 minutes later each night, but at this time of year it’s around 20 minutes later for mid-northern latitudes and even later further north. Because of this added light, the name ‘‘Harvest Moon’’ was coined; it allowed farmers more time to work in the fields.

smoon

Often times we perceive the Harvest Moon as being more orange than at any other time of the year. The coloration is caused by the scattering of the light by particles in our atmosphere. When the Moon is low, like now, we get more of that scattering effect, and it truly does appear more orange. The very act of harvesting itself produces more dust, and often times that coloration will last the whole night through. And we all know the size is only an ‘‘illusion’’. . .

So, instead of cursing the Moon for hiding the deep-sky gems tonight, enjoy it for what it is, a wonderful natural phenomenon that doesn’t even require a telescope!

sputnik1Sunday, October 4, 2009 – This date in 1957, the USSR’s Sputnik 1 made space history, as it became the first man-made object to orbit Earth. Earth’s first artificial satellite was tiny, roughly the size of a basketball, and weighed no more than the average man. Every 98 minutes it swung around Earth in its elliptical orbit. . .and changed everything. It was the beginning of the ‘‘Space Age.’’ Take the time with your children or grandchildren to check Heaven’s Above for visible passes of the International Space Station (ISS), and think about how much our world has changed in just over half a century!

Tonight we’ll begin with an easy double star and make our way toward a more difficult one. Beautiful, bright, and colorful, Beta Cygni is an excellent example of an easily split double star.

betacygni

As the second brightest star in the constellation of Cygnus, Albireo lies roughly in the center of the ‘‘Summer Triangle,’’ making it a relatively simple target for even urban telescopes. Albireo’s primary (or brightest) star is around magnitude 4 and has a striking orangish color. Its secondary (or B) star is slightly fainter at a bit less than magnitude 5, and often appears to most as blue, almost violet. The pair’s wide separation of 3400 makes Beta Cygni an easy split for all telescopes at modest power, and even for larger binoculars. At approximately 410 light-years away, this colorful pair has a separation of about 4,400 Astronomical Unit (AU). As Burnham noted:

‘‘It is worth contemplating, in any case, the fact that at least 55 Solar Systems could be lined up, edge-to-edge, across the space that separates the components of this famous double!’’

deltacygniNow let’s have a look at Delta (RA 19 44 58 Dec +45 07 50). Located around 270 light-years away, Delta is a more difficult binary star. Its duplicity was discovered by F. Struve in 1830, and it is a very tough test for smaller optics. Located no more than 220AU away from the magnitude 3 parent star, the companion takes anywhere from 300 to 540 years to orbit its star and is often rated as dim as 8th magnitude. If skies aren’t steady enough to split it tonight, try again! Both Beta and Delta are on many challenge lists.

Until next week? Ask for the Moon… But keep on reaching for the stars!

This week’s awesome images are (in order of appearance): Solar System Montage (credit—NASA), Saguaro Moon (credit and copyright—Stefan Seip (NASA/APOD), Sputnik Archival Image, Beta Cygni: Albireo (credit—University of Nebraska-Lincoln) and Delta Cygni (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!

Weekend SkyWatcher’s Forecast – September 18-20, 2009

Greetings, fellow SkyWatchers! It’s an awesome weekend forecast for many of us attending Fall Star Parties, and all over the world we’re looking forward to moonless nights and the fellowship with our brother and sister amateur astronomers. If you’ve never been to a star party, try the Goggle pages for information… you just might find one going on near you! In the meantime, let’s have us a “Snowball” fight, chase some galaxies and ponder double stars! I’ll see you in the night…

Friday, September 18, 2009 – One of the most interesting features of the autumn sky is how slowly the stars and constellations seem to proceed across the heavens. This is only an illusion, since skydark arrives earlier each night (after summer solstice in the Northern Hemisphere), making the progress of the constellations across the sky seems to ‘‘freeze.’’ Tonight, Capella can be seen rising to the northeast just as Antares settles southwest. Four planets—Jupiter, Pluto, Neptune, and Uranus—are still above the horizon, with Jupiter now very low to the west-southwest. Descending to the northwest is Ursa Major, the ‘‘Big Dipper.’’ Across the sky is Piscis Austrinus, and lonely but bright Fomalhaut is beginning its rise. Seven stars of the first magnitude now grace the heavens. Against this backdrop, one of the darkest skies of the month is now upon us. It’s the New Moon…

Let’s have a look at another fine planetary nebula—NGC 7662. At 9 magnitude, this one is more commonly known as the ‘‘Blue Snowball’’ and can be found about three finger-widths east of Omicron Andromedae, or a little less than a handspan northwest of Alpha Pegasi (RA 23 25 54 Dec +42 32 06).

snowball

Similar in size to M57, even low power with a small scope easily reveals the planetary nature of this very fine study. Power up and you’ll discover that the annulus of this roughly circular planetary is definitely brighter inside than out. Large telescopes will highlight NGC 7662’s blue coloration and reveal a bright inner globe surrounded by a faint outer ring.

Saturday, September 19, 2009 – On this date in 1848, William Boyd was observing Saturn and discovered the planet’s eighth moon, Hyperion. If you’re out before sunset, some lucky stargazers are going to discover that the slender crescent Moon is about to occult Mercury! Check the Resources in this book and IOTA for locations and dates. Then check them both out in binoculars!

Would you like to try for another pair? Then wait until the skies are fully dark and head north for a galaxy and cluster pairing—NGC 6946 (RA 20 34 51 Dec +60 09 18) and NGC 6939 (RA 20 31 30
Dec +60 39 42).

6946

Located in western Cepheus, you’ll find them about a finger-width southwest of Eta.

6939Discovered by William Herschel on September 9, 1798, 10 million-light-year-distant face-on spiral NGC 6946 spreads itself pretty thin in modest instruments. Lacking a bright core, this oval mist orients southwest to northeast. Larger telescopes will reveal traces of rotating spiral arms, especially in the southwest. This galaxy would appear extraordinary if we weren’t looking through Milky Way obscuration to view it! Through smaller scopes, northwestern open cluster NGC 6939 appears like a tight little formation of 11th and 12th magnitude stars similar in pattern to a very small M11. It resolves well in larger scopes.

humboldtSunday, September 20, 2009 – Today we recognize the passing of cosmonaut Gherman S. Titov in 2000; Titov was not only the second human in space but also the youngest! Perhaps when he was orbiting Earth in Vostok 2 he had a chance to see the Moon. Why don’t we join him? Tonight, your lunar mission is to journey to the edge of the east limb and slightly south of central to identify crater Humboldt. Seen on the curve, this roughly 200-kilometer-wide crater holds a wealth of geographical details. Its flat, cracked floor has central peaks and a small mountain range, as well as a radial Rille structure. If libration and steadiness of skies are in your favor, power up and look for dark pyroclastic areas and a concentric inner crater.

betalyraeNow, let’s have a look at Beta and Gamma Lyrae, the lower two stars in the ‘‘Harp.’’ Beta is actually a quick-changing variable, which drops to less than half the brightness of Gamma in about 12 days. For a few days, the pair will seem of almost equal brightness, and then you will notice the star closest to Vega fade away. Beta is one of the most unusual spectroscopic stars in the sky, and it is possible that its eclipsing binary companion may be the prototype of a ‘‘collapsar’’ (yep, a black hole!), rather than a true luminous body.

Enjoy your weekend!!

This week’s awesome images (in order of appearance) are: NGC 7662 (credit—Adam Block/NOAO/AURA/NSF), NGC 6946 and NGC 6939 (credit—Palomar Observatory, courtesy of Caltech), Crater Humboldt (credit—Ricardo Borba) and Beta Lyrae (credit—Palomar Observatory, courtesy of Caltech). We thank you so much!!

Weekend SkyWatcher’s Forecast: September 4-6, 2009

Greetings, fellow SkyWatchers! Ah, yes… Full Moon. Are you ready to howl? If you didn’t get a chance to watch the galiean moons do their dance last weekend, then be sure to catch the awesome video you’ll find inside! In the meantime, keep your ears alert for the rise of tonight’s “Full Corn Moon” and check out the Omicron gems. As the skies get darker, the Herschel challenges warm up – so dust off your optics and I’ll see you in the backyard…

Friday, September 4, 2009 – It’s a Full Moon tonight. Many cultures refer to this one in particular as the ‘‘Corn Moon,’’ because at this time of year most corn crops are ready for harvest. Tonight let’s harvest some bright lunar features as we trace the ray system of Tycho in the lunar south. Look for the bright points of Kepler and Aristarchus in the northwest quadrant. In the east, dazzling crater Proclus will light up the western shore of Mare Crisium. Just north of central, look for the two bright rings of Manlius and Menelaus.

nasafullmoon

Although the Moon will dominate tonight’s sky, we can still take a very unusual and beautiful journey to a bright and very colorful pair of stars known as Omicron 1 Cygni. Easily located about halfway between Alpha (Deneb) and Delta on the western side (RA 20 13 28 Dec +46 46 40), this is a pure delight in binoculars or any size telescope.

omicron1cygThe striking gold color of 3.7-magnitude Omi 1 A is easily highlighted against the blue of its same-field companion, 5th magnitude Omi 1 B. Although this wide pairing is only an optical one, the K-type giant (A) is indeed a double star—an eclipsing variable about 150 times larger than or own Sun—and is surrounded by a gaseous corona more than double the size of the star itself. If you are using a scope, you can easily spot its blue tinted, 7th magnitude companion star about one-third the distance between the two giants. Although our true pair is some 2 billion kilometers apart, they are oriented nearly edge-on from our point of view, allowing the smaller star to be totally eclipsed during each revolution. This total eclipse lasts for 63 days and happens about every 10.4 years, but don’t stay up too late. . . We still have years to wait!

Saturday, September 5, 2009 – Tonight before the Moon commands the sky, let’s start with the brightest star in Vulpecula—Alpha. Although it is not a true binary star, it is quite attractive in the telescope, and an easy split for binoculars. Alpha itself is a 4.4-magnitude red giant, which makes a nice color contrast with the unrelated yellow field star that is 2 magnitudes dimmer.

Now head around a half degree northwest of Alpha (RA 20 19 29 Dec –70 51 36) for open cluster NGC 6800. Also known as Herschel VIII.21, this cluster is suitable for even smaller scopes but requires aperture to resolve completely. Discovered by Sir William in this month (10th) in 1784, you’ll like this ring-like arrangement of stars!

ngc6800

ngc6793Now drop 2.7 degrees southwest of Alpha (RA 19 23 12 Dec +22 08 00) for yet another open cluster, NGC 6793. Discovered by Herschel in 1789 and logged as catalog object VIII.81, you’ll find a few more bright stars here. The challenge in this cluster is not so much being able to see it in a smaller telescope—but being able to discern a cluster from a star field! Try using the photo to help you distinguish it from the rest…

Sunday, September 6, 2009 – Today we celebrate many births. In 1891, it’s Yrjo Vaisala who produced telescope optics and discovered asteroids. In 1830, John Henry Dallmeyer, who was a master at making telescopes and eyepieces, was born. Last, in 1811, was James Melville Gilliss who founded the United States Naval Observatory.

Tonight we’ll return again to Vulpecula, but with a different goal in mind. What we’re after requires dark skies yet can be seen in either binoculars or a small telescope. Once you’ve found Alpha, begin about two finger-widths southeast, and right on the galactic equator you’ll find NGC 6823 (RA 19 43 10 Dec +23 17 54.). The first thing you will note is a fairly large, somewhat concentrated magnitude 7 open cluster.

Resolved in larger telescopes, the viewer may note these stars are the hot, blue-white variety. For good reason. NGC 6823 only formed about 2 billion years ago. Although it is some 6,000 light-years away and occupies around 50 light-years of space, it’s sharing the field with something more—a very large emission/reflection nebula, NGC 6820 (RA 19 42 27 Dec +23 05 14).

ngc6820

In the outer reaches of star cluster NGC 6823, new stars are being formed in masses of gas and dust as hot radiation is shed from the brightest of the stellar members of this pair. Fueled by emission, NGC 6820 isn’t always an easy visual object; it is faint and covers almost four times as much area as NGC 6823. But trace the edges very carefully, since the borders are much more illuminated than the central cluster region. Take the time to really observe this one! The processes going on here are very much like those in the ‘‘Trapezium’’ area of the Orion nebula. Be sure to mark your siting in your observing notes. NGC 6823 is Herschel VII.18 and NGC 6820 is also known as Marth 401!

Did you catch last week’s awesome Jupiter events? If not – then enjoy this great footage taken by the one and only Joe Brimacombe. (Not only is Dr. Joe cool… but he’s also one of the best observers I know!)

Perhaps you need another little nudge to get you out and observing, huh? Then here’s a list of Jupiter activities over the weekend:

Friday

  • 00:58 UT, Io begins transit of Jupiter.
  • 01:28 UT, Io’s shadow begins to cross Jupiter.
  • 03:16 UT, Io ends transit of Jupiter.
  • 03:48 UT, Io’s shadow leaves Jupiter’s disk.
  • 22:10 UT, Io enters occultation behind Jupiter.

Saturday

  • 01:00 UT, Io exits eclipse by Jupiter’s shadow.
  • 02:36 UT, Europa exits eclipse by Jupiter’s shadow.
  • 19:24 UT, Io begins transit of Jupiter.
  • 19:58 UT, Io’s shadow begins to cross Jupiter.
  • 21:42 UT, Io ends transit of Jupiter.

Sunday

  • 16:36 UT, Io enters occultation behind Jupiter.
  • 17:06 UT, Europa begins transit of Jupiter.
  • 18:14 UT, Europa’s shadow begins to cross Jupiter.
  • 18:20 UT, Ganymede enters occultation behind Jupiter.
  • 19:28 UT, Io exits eclipse by Jupiter’s shadow.

Now get out there and observe!!

This week’s awesome images are (in order of appearance): Full Moon (credit—NASA), Omicron 1 Cygni, NGC 6800, NGC 6793, NGCs 6823 (central) and 6820 (credit—Palomar Observatory, courtesy of Caltech) and Jupiter footage courtesy of Joe Brimacombe. We thank you so much!