Monthly Archives: May 2016

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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

NASA Space Place – Hubble Shatters The Cosmic Record For Most Distant Galaxy

Poster’s Note: One of the many under-appreciated aspects of NASA is the extent to which it publishes quality science content for children and Ph.D.’s alike. NASA Space Place has been providing general audience articles for quite some time that are freely available for download and republishing. Your tax dollars help promote science! The following article was provided for reprinting in April, 2016.

By Dr. Ethan Siegel

2013february2_spaceplaceThe farther away you look in the distant universe, the harder it is to see what’s out there. This isn’t simply because more distant objects appear fainter, although that’s true. It isn’t because the universe is expanding, and so the light has farther to go before it reaches you, although that’s true, too. The reality is that if you built the largest optical telescope you could imagine — even one that was the size of an entire planet — you still wouldn’t see the new cosmic record-holder that Hubble just discovered: galaxy GN-z11, whose light traveled for 13.4 billion years, or 97% the age of the universe, before finally reaching our eyes.

There were two special coincidences that had to line up for Hubble to find this: one was a remarkable technical achievement, while the other was pure luck. By extending Hubble’s vision away from the ultraviolet and optical and into the infrared, past 800 nanometers all the way out to 1.6 microns, Hubble became sensitive to light that was severely stretched and redshifted by the expansion of the universe. The most energetic light that hot, young, newly forming stars produce is the Lyman-α line, which is produced at an ultraviolet wavelength of just 121.567 nanometers. But at high redshifts, that line passed not just into the visible but all the way through to the infrared, and for the newly discovered galaxy, GN-z11, its whopping redshift of 11.1 pushed that line all the way out to 1471 nanometers, more than double the limit of visible light!

Hubble itself did the follow-up spectroscopic observations to confirm the existence of this galaxy, but it also got lucky: the only reason this light was visible is because the region of space between this galaxy and our eyes is mostly ionized, which isn’t true of most locations in the universe at this early time! A redshift of 11.1 corresponds to just 400 million years after the Big Bang, and the hot radiation from young stars doesn’t ionize the majority of the universe until 550 million years have passed. In most directions, this galaxy would be invisible, as the neutral gas would block this light, the same way the light from the center of our galaxy is blocked by the dust lanes in the galactic plane. To see farther back, to the universe’s first true galaxies, it will take the James Webb Space Telescope. Webb’s infrared eyes are much less sensitive to the light-extinction caused by neutral gas than instruments like Hubble. Webb may reach back to a redshift of 15 or even 20 or more, and discover the true answer to one of the universe’s greatest mysteries: when the first galaxies came into existence!

This article was provided by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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Caption: (top); NASA, ESA, P. Oesch (Yale University), G. Brammer (STScI), P. van Dokkum (Yale University), and G. Illingworth (University of California, Santa Cruz) (bottom), of the galaxy GN-z11, the most distant and highest-redshifted galaxy ever discovered and spectroscopically confirmed thus far.

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With articles, activities, crafts, games, and lesson plans, NASA Space Place encourages everyone to get excited about science and technology. Visit spaceplace.nasa.gov (facebook|twitter) to explore space and Earth science!