Tag Archives: Leo

Bob Piekiel Hosts Observing Sessions At Baltimore Woods (And More!) – 2018 Observing Schedule

This event list will be added to as the year progresses. Check back often!

I’m pleased to have obtained the official schedule for Bob Piekiel’s growing observing and lecture programs for the 2018 season. For those who have not had the pleasure of hearing one of his lectures, attending one of his observing sessions, or reading one of his many books on scope optics (or loading the CD containing the massive Celestron: The Early Years), Bob Piekiel is not only an excellent guide but likely the most knowledgeable equipment and operation guru in Central New York.

Notes On Baltimore Woods Sessions:

The Baltimore Woods events calendar is updated monthly. As such, I’ve no direct links to the sessions below. Therefore, as the event date nears, see the official Calendar Page for more information and any updates on the event.


* Registration for these events are required. Low registration may cause programs to be canceled.
* $5 for members, $15/family; $8 for nonmembers, $25/family.
* To Register By Email: info@baltimorewoods.org
* To Register By Phone: (315) 673-1350

Baltimore Woods:

* January 19 (Fri.)/20 (Sat. weather alternate), 7:00-9:00 p.m.

Winter skies at their finest, The area surrounding the constellation Orion has more bright stars and deep-sky clusters than any other section of the sky. Still good views of Uranus.

* February 16 (Fri.)/17 (Sat. weather alternate), 5:30-8:30 p.m.

This is a good chance to see the elusive planet Mercury, right after sunset, plus the area surrounding Orion, one of the brightest in the sky. We have to start early to catch Mercury. We might still get a good view of Uranus.

* February 24 (Sat.)/25 (Sun. weather alternate), 1:00-3:00 p.m.

Solar viewing program – see our nearest star with specially-equipped solar telescopes, showing sunspots, flares, and eruptions.

* March 16 (Fri.)/17 (Sat. weather alternate), 6:00-9:00 p.m.

Goodbye to winter skies, but still great views of Orion. Maybe a few Lyrid meteors as well.

* April 13 (Fri.)/14 (Sat. weather alternate), 7:30-9:30 p.m.

Hello to Spring skies. Watch as the seasons change both on the ground and the starry night. Orion will be setting, and being replaced by Leo the lion.

Green Lakes:

Awaiting 2018 scheduling.

Clark Reservation:

Awaiting 2018 scheduling.

Regulus Occultation Update – We’ve Got Erigone On Our Minds

Greetings fellow astrophiles!

Despite the torrential snowfall at present, we remain ever optimistic (and it’s too far out to trust any weather predictions anyway) about the possibility of clear skies on the early-early morning of March 20th, when the Main Belt asteroid Erigone will occult the star Regulus in Leo the Lion.

Richard Nugent’s silent youtube movie about the Regulus occultation.

We’ve already posted two lengthy articles on the topic, including the official press release:

* IOTA Official Press Release: Best And Brightest Asteroid Occultation Ever To Be Visible Across New York State

And an article describing the occultation measurement and data-collection process itself for determining Erigone’s shape:

* Central New York: Take Note (And Help Out)! – The Occultation Of Regulus By Asteroid Erigone On March 20th

I am happy to report that the press release has now appeared on the Kopernik Astronomical Society website (thanks to the efforts of their postmaster general Patrick Manley – the Vestal observatory may be on the far, far western edge of the occultation measurement, but hopefully a good spread of members down there can cover the measurements of the asteroid’s far western side):

* Best And Brightest Asteroid Occultation Ever To Be Visible Across New York State

And a recent universetoday article on the occultation even gives CNYO a linked shout-out (which we gladly accept):

* How to Watch an Asteroid Occult a Bright Star on March 20th

Expect a small flurry of posts next week as we prepare for 14 seconds of pure adrenaline between 2:00 and 2:10 a.m. E.D.T. on March 20th (and, to clarify – because it came up – this means you’ll be staying wide awake on the 19th, pass midnight, then kill two more hours before going outside. Plenty of time to practice while you wait, and hopefully your thumb won’t freeze over waiting to push your stopwatch app).

In the meantime, if you plan on measuring the occultation time, do consider giving the official Regulus Occultation FAQ a thorough once-over: Volunteer observers invited to time the March 20, 2014 Occultation of Regulus

And, to keep track of official International Occultation Timing Association (IOTA) announcements and anything else that might come across the page, consider joining the Regulus2014 Facebook page at: www.facebook.com/Regulus2014

IOTA Official Press Release: Best And Brightest Asteroid Occultation Ever To Be Visible Across New York State

Greetings fellow astrophiles!

Below is the official press release by the International Occultation Timing Association (IOTA) on the upcoming occultation of Regulus by asteroid Erigone on March 20th. CNYO will have more to announce about our efforts to monitor this occultation in the next week or two. Meantime, this is your one-month warning!

Public invited to help measure size and shape of distant asteroid

Media contact: Ted Blank, tedblank@gmail.com
Alternate contact: Steve Preston, stevepr@acm.org

Just after 2:05 a.m. EDT on March 20, 2014, anyone with clear skies along a 70-mile-wide belt running diagonally from Long Island and New York City up through New York State into Canada may be able to see the bright star Regulus simply disappear from the sky for up to 14 seconds as an invisible asteroid glides silently in front of it.

A chance alignment of orbits is predicted to cause Regulus to “wink out” as the mammoth asteroid Erigone passes directly between Earth and the star, temporarily blocking its light from reaching us (the asteroid itself remains in its normal orbit which never comes anywhere near Earth). Regulus (the star which will wink out) is in the constellation Leo the Lion and, as one of the brightest stars in the sky, is easy to find.

An event where an object in space blocks the light from a distant star is called an “occultation,” from the Latin word meaning “to conceal or hide.” The International Occultation Timing Association (IOTA), a group of volunteers, collects observations on about 200 asteroid occultations per year. However, this is the first time that such a dramatic and obvious occultation will be visible in such a heavily populated area without the need for any kind of optical aid like a telescope or binoculars.

What makes this asteroid event more notable is that the public is invited to assist scientists in recording the event to measure the size and shape of the asteroid. Just by using a video camcorder, a digital SLR camera with video capability, or just a smartphone or a stopwatch, anyone can contribute to the scientific study of the asteroid in question. “In addition to the opportunity to share in a moment of celestial drama, we hope to enlist thousands of ‘citizen-scientists’ to time this event, allowing us to document it more thoroughly than any other asteroid occultation in history” said Steve Preston, President of IOTA. “The more observers scattered across the path of the shadow who time the disappearance and reappearance of the star, the more accurately we can measure the asteroid’s size and shape.”

IOTA has created a “Frequently Asked Questions” page at www.occultations.org/Regulus2014. Here, detailed information may be found on the recommended techniques that the public may use to record and time the event, as well as how to submit their observations for analysis after the event.

Although the asteroid will remain a safe 100 million miles from Earth, as it passes in front of the star its 70-mile-wide shadow will sweep from southeast to northwest across Nassau and Suffolk counties, all five boroughs of New York City and the Hudson River Valley, with the center of the predicted shadow path following a line roughly connecting New York City, White Plains, Newburgh, Oneonta, Rome and Pulaski before crossing into Canada. See Illustration 1 for the current prediction of where the shadow will pass.


Ill. 1. Estimated path of the shadow of the asteroid Erigone during the occultation of Regulus on March 20, 2014. The green line represents the predicted center line of the ~50 mile wide asteroid shadow. The blue lines represent the width of the asteroid, where edges of the shadow would fall if the actual center of the shadow followed the green line. The red lines represent the uncertainty in the path, meaning that the actual shadow will most likely pass somewhere between the red lines. There is a smaller chance that one edge could be slightly outside one or the other of the red lines.

At the time of the occultation, Regulus will be about 40 degrees high in the southwest, or about half-way up from the horizon to a point straight overhead. Illustration 2 below is a “sky-map” showing the star’s location in the sky along with some convenient reference points to help get oriented.


Ill. 2. Finder chart for March 20, 2014, looking southwest. The red dot at the top represents the point directly overhead. Regulus will be approximately half-way up in the sky, at the bottom of the reversed “question mark” that makes up the “mane” of Leo the Lion. Saturn, the Moon, Mars and Jupiter are shown on this map in the positions they will occupy on this date, as are the twin stars of Gemini (Castor and Pollux) just above Jupiter.

To choose an observing location, members of the public can refer to Illustration 1 and select any place between the outer lines. Since the path the shadow will follow may change slightly, observers should check the online zoomable map at tinyurl.com/regulus2014map in the days before the event for any last-minute adjustments to the path prediction. Additionally, people situated as far as 10 path-widths on either side of the center line are encouraged to make an observation in case Erigone has a moon which might momentarily block the star’s light. Video recordings will be needed to confirm the fleeting disappearance that a tiny moon of Erigone might cause.

After the event, the public may report their timing observations at tinyurl.com/regulus2014report, including reports of a “miss,” or no occultation. “Both actual timings and ‘miss’ observations are extremely valuable,” said Preston. “Timings of the disappearance measure the asteroid’s diameter in the dimension along its orbital path, but ‘miss’ observations improve our understanding of how wide it is across its path. Furthermore, both types of reports improve our understanding of the asteroid’s orbit.”

Typically only a few observers see these types of events, allowing the diameter of the asteroid to be measured at just a few places. However, with a large number of observers, the opportunity exists to categorize the asteroid’s entire silhouette, as seen for asteroid (234) Barbara in Illustration 3 below.


Ill. 3. Outline of asteroid (234) Barbara obtained by multiple observers timing an occultation in 2009. The observers were spread out across an area over 40 miles wide. The horizontal white gaps in the solid lines represent the period of time when the asteroid blocked the light from the star for that observer. The gaps between the lines themselves represent the distance between observers on the ground. Each observer saw the star pass behind a slightly different portion of the asteroid, allowing the asteroid’s diameter to be measured at multiple locations. Note the large crater at the south end of the asteroid. This level of resolution is far greater than anything possible with ground-based telescopes, but more observers would have allowed even finer details to be measured.

Members of the public with additional questions should refer to the FAQ page at www.occultations.org/Regulus2014, email regulus2014@occultations.org or see the article in the March, 2014 issue of Sky and Telescope Magazine.

About IOTA

The International Occultation Timing Association, with its worldwide sister organizations in Europe, the United Kingdom, Australia/New Zealand, Japan, S. Asia/India, Mexico, Latin America and South Africa, provides free occultation predictions and planning and analysis software, sponsors online Internet discussion groups and publishes the Journal of Occultation Astronomy. The main IOTA webpage is www.occultations.org. The Yahoo discussion group can be found at http://groups.yahoo.com/neo/groups/IOTAoccultations/info and is open to all with an interest in this topic.

A PDF copy of an article from the March, 2014 issue of Sky and Telescope Magazine on the occultation is linked HERE. Permission to include this article has been granted by Sky and Telescope.