Jan 2018

Local Eclipsers Snowed Out!

Most of Ontario and much of eastern Canada saw no lunar eclipse Jan 31 due to poor weather. However, NASA TV did broadcast the eclipse from 4 sites, and only one, the Institute for Astronomy in Hawaii was clouded out. Griffith Observatory near Los Angeles and Armstrong Flight Research Center at Edwards AFB as well as the Mt Lemmon Observatory north of Tucson AZ had clear conditions. NASA was able to supply high quality images from start to finish as the Moon set in the west around 7 am MST. Even in the most western locations in North America (except Alaska), the Moon set just after or a bit before the last bit of umbra had departed the face of the Moon.

The full Moon was visible through thin, quickly moving clouds for a time after moonrise in Owen Sound and climbed above the escarpment to the east of my location.

IMG_162465_plusFM_comp_580K

Composite image of Jan 30 full Moon only 12 hours before eclipse. Last time we saw it from Owen Sound was around midnight.
Canon 60Da with 100 mm lens (eff=160mm) ISO 3200 f/4.5 1/15 s (background) plus FM at 1/800 s at 6:18 pm EST (John H. Image)


But even then the clouds hid the moon for 20% of the time and by 9 pm, there was significant cloud cover. When I rose at 5:45 am to check the skies, there was a barely perceptible disk of moonlight and by 6 am, it was snowing in Owen Sound and the Moon was invisible. NASA TV to the rescue!

Images below from NASA TV were broadcast live and viewers got to see it from different locations (Griffith Observatory and Armstrong Flight Research Center near Los Angeles, Mt. Lemmon Observatory (N. of Tucson AZ) and the Institute for Astronomy in Hawaii. The latter location was clouded out. Here is a sampling of images.


Mt.Lemmon-mid-ecl_enh

The fully eclipse Moon was right next to the Beehive Cluster in the centre of Cancer at right. The original image was a screen capture of the NASA feed and was slightly enhanced in PS to bring out more stars in the cluster. Mt. Lemmon Observatory near Tucson AZ.

Screen Shot 2018-01-31 at 7.51.14 AM

This image was taken just before the inset of totality from Griffith Observatory north of Los Angeles.

Screen Shot 2018-01-31 at 8.11.08 AM
Another Griffith Observatory image around mid-totality.

Screen Shot 2018-01-31 at 9.08.16 AM

Totality is just over and the edge of the Earth’s umbra is starting to appear at lower left.

Screen Shot 2018-01-31 at 9.23.30 AM

Partial phase is underway after umbral eclipse ends in this image from Armstrong Flight Research Center at Edward’s AFB

Screen Shot 2018-01-31 at 9.45.25 AM

Partial is still underway as daylight approaches and the Moon sets below the western horizon at Edward’s AFB.





Griffith Observatory has put together a time-lapse video here: Griffith Time-Lapse

Screen Shot 2018-02-01 at 5.59.23 PM


Jan 31 LUNAR ECLIPSE

At the risk of adding to the “super Moon” hype, allow me to point out that both full Moons in January are “super”. The Jan 1 full Moon is more super than the full Moon at month-end by a mere 2 429 km, but the full Moon on Jan 31 is also a so-called “blue” Moon. Adding to the hype, the Moon is supposed to turn “blood red” during a lunar eclipse that morning. So on Jan 31, we are due for a Super, Blue, Blood Red Moon! Sheesh.

The “blood red” label appears to be a relatively recent development, a result of two prophets of doom that thought four lunar eclipses in a row (ending with the Sep 27, 2015 eclipse) meant something special. It did not. The apocalypse did not happen in 2015, just like the other 20 times doomsday was predicted since Jan 1, 2000. By the way, there are three dates (so far) on which the world will end in 2018. I would watch out for the doomsday of May 20, a date supposedly guaranteed in the Bible (or your money back).

The Earth’s shadow in space has two parts, a dark circular core called the umbra, which is about 3 times the diameter of the Moon, and an invisible outer shadow called the penumbra which is even larger. It is only the umbra that we see progressing across the Moon during an eclipse, making it appear to go through its monthly cycle of phases in a just a few hours. See our website
www.bluewaterastronomy.com for a neat graphic depicting this.

Moon colour during lunar eclipses is caused by our atmosphere filtering out blue light the same way it does whenever the Moon or Sun are near the horizon. For any of the lunar eclipses I have seen, “blood red” would not be a colour description I would have used. I have seen “reddish-brown”, “orange”, “yellowish-orange”, and even “gray” the one time that volcanic ash in our atmosphere filtered out all the colour from the light getting to the Moon. That time, the eclipsed Moon was invisible to the naked eye and only just detectable in binoculars, appearing like a black hole among the stars. Furthermore, the central part of Earth’s shadow is darker so the Moon’s colour changes as the eclipse progresses. Colour-wise, no two lunar eclipses are ever exactly the same and hardly ever do we see “cherry” or “blood red” colours, -except after some Photoshop “enhancement” also known as “astro-fake-it-ography”.

The total lunar eclipse just before sunrise on Jan 31, 2018 will be visible all over the western hemisphere more or less. For us here in Bruce and Grey county, it will be less than more. Folks in the Prairie provinces get more, and those farther west in Calgary or Kelowna, for example, will see the entire event.

The hour-long passage of the full Moon through Earth’s shadow is the most interesting part of a lunar eclipse, but unfortunately this time, all of eastern Canada misses it. Locally, the Moon sets below our western horizon 10 minutes before totality begins and we will see only a bright “crescent” Moon with a bit of redness to the darkened portion like the image provided here of the Sep 27, 2015 lunar eclipse. Seeing conditions will have to be perfect to see anything like this and the Moon will be dimmed because sunrise is at the same time as moonset.

IMG_122192_crop

Sep 27 Total Lunar eclipse by John H. at prime focus (TeleVue NP101) eff.foc.len. = 864mm
Exposure 1/20 s at ISO 2000

For Bruce-Grey, the first umbral contact occurs at 6:48 am EST with the full Moon only 8 degrees above the western horizon (about the width of your out-stretched hand). A darkening at upper left should be noticeable by 6:45 am or so and it will progress across the Moon until the Moon sets at 7:44 am EST below our western horizon. For those in the Pacific Time Zone, totality starts at 4:52 am PST (7:52 EST), and lasts for 76 minutes until 6:08 PST. The eclipse ends when the last bit of the full Moon reappears by 7:11 am PST. You need to be west of the Manitoba-Saskatchewan border to see all of totality before the Moon sets.

The Bluewater Astronomical Society will make the best of the event locally with telescopes at a location with a good view to the western horizon. We will be scouting locations along the Lake Huron shore where snowbanks are manageable. Assuming weather co-operates, check our website
www.bluewaterastronomy.com as the time approaches for last-minute confirmation of viewing site. Fingers crossed for clear skies!