Tag Archives: Far Side

Transit Of Mercury Session @ Baltimore Woods – Monday, May 9th, 8 a.m. To 10 a.m.

Greetings, fellow astrophiles –

There will be no next-day reschedule of this event! Our hemisphere is being treated to the third Transit of Mercury this century, and Bob Piekiel is hosting an official observing session at Baltimore Woods to mark the event and to give keen viewers a sight of our (now) smallest planet.

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This NASA graphic depicts the time and location of Mercury as it crosses the face of the sun during the May 9, 2016 Transit of Mercury event. – From NASA

For those new to the phenomenon, a transit occurs when one small body passed in front of another larger body relative to the observer’s position. If you’ve ever been in the left lane of a three-lane highway, had a big truck in the right lane, and had a motorcycle pass in the middle lane at some blistering speed, you’ve witnessed a (kind of) transit. From our Earth-centric perspective (and sticking to one definition of a transit), transits occur when the inferior planets (which just means their between us and the Sun) Mercury or Venus pass between us and the Sun. Once we’re living on Mars, transits will occur when the inferior planets Mercury, Venus, or Earth pass between us (there) and the Sun. And you get the idea.

2016may5_orbital_angles_q4O5UNow a little math – Mercury revolves around the Sun once every 87.9 days – what we call its sidereal period. Because the Earth revolves as well, the time it takes for Mercury to hit the same basic spot between us and the Sun is 115.9 days (its synodic period). If all of the planets of the Solar System were in a perfect flat plane, that would mean we’d get a Mercury Transit every 116-ish days and the phenomenon would be a little less impressive. Because all of the planets are at slight tilts with respect to Earth’s orbit, we don’t always get clean passes – the Sun is huge overall, but still a small target at an Astronomical Unit, so the slight angles of Mercury and Venus matter when it comes to the proper lining-up needed for transits to occur.

Click the map to make directions to Baltimore Woods.

The next Mercury Transit (from an Earth viewing location, that is) won’t occur until 11 Nov 2019, then there’s a loooong wait until 13 Nov 2032. If you can get a free block in the morning, I highly encourage you to make the trip out to Baltimore Woods. The two Venus Transits I witnessed definitely “clicked” something in me about how the Solar System works (and the size of Venus against the Sun was a very impressive sight!).

The text from Bob’s official announcement is below:

Rare Transit of Mercury Across the Sun. The planet Mercury will move directly between the Earth and the Sun. Viewers with telescopes and approved solar filters will be able to observe the dark disk of the planet Mercury moving across the face of the Sun. This is an extremely rare event that occurs only once every few years. There will be one other transit of Mercury in 2019 and then the next one will not take place until 2039. (Venus will also be visible right near the sun as well).

If you can’t make it out but still want to see it, the good news is that your tax dollars are being put to good use – NASA will be live streaming the transit. For details, see www.nasa.gov/press-release/nasa-to-provide-coverage-of-may-9-mercury-transit-of-the-sun

CNYO Brochure – A Guide For Lunar Observing

Greetings fellow astrophiles!

In preparation for upcoming 2013 lecture and observing sessions, we have put together instructional brochures to help introduce the Night Sky to attendees. The fifth of these, entitled “A Guide For Lunar Observing,” combines facts and figures about our nearest natural satellite with a map of the largest features on its “near side,” all easily visible in low-power binoculars. This brochure will be available at our combined lecture/observing sessions, but feel free to bring your own paper copy (or the PDF on a tablet – but have red acetate ready!).

Download: A Guide For Lunar Observing (v5)

NOTE: These brochures are made better by your input. If you find a problem, have a question, or have a suggestion (bearing in mind these are being kept to one two-sided piece of paper), please contact CNYO at info@cnyo.org.

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A Guide For Lunar Observing

Some Interesting Facts About The Moon

620 millions years ago, the day was 21.9 hours long and one year was 400 days!

Phases Of The Moon

With respect to a fixed spot over the Earth’s surface, the Moon completes one orbit in a
sidereal month – 27 days, 7 hours, and 43 minutes.

The Blue Moon (Not Really Blue)

Since the synodic cycle of the Moon (FM to FM) is 29.5 days, a FM at the very beginning of a month will result in a FM at the end of same month.

The Man In The Moon & Other Features

The surface of the Moon shows evidence of the violent nature of the early Solar System.

The Moon – Not Just A Pretty Face!

On the side of Earth nearest the Moon, lunar gravity is strongest, pulling the water up slightly (“sublunar” high tide).

Can I See The American Flag?

There is lots of equipment left on the Moon from manned and unmanned missions, but Earth-based and many space-based telescopes do not have the resolving power to see any of it.

The Dark Side Of The Moon

The Moon’s orbital period and rotation period are the same – as it makes one trip around the Earth, it completes one spin on its axis – this is called “Tidal Lock,” and is why we only ever see one side from Earth.