This full Moon will be a perigee full Moon, with the Moon appearing a bit larger and brighter. Today lunar perigee occurs about 17 hours of full, producing a full moon that is about 12% larger and 30% brighter than if full occurs while the Moon is at apogee.
Laser Gallery
Snow on Mauna Kea?
The forecast looks promising. Not for observing, we lost most of the night last night to fog and clouds, the rest of the week looks worse. It does look like we may get some snow this week. Checking the cameras there are already a few flakes coming down, just a degree or so too warm to stick.
Winter is here… Snow for Christmas?
Update! Sticking now…
Mercury at Maximum Elongation
Today Mercury will be at maximum eastern elongation, as high in the evening sky as it will appear for this current apparition. After today the planet will slide back into the sunset, passing through inferior conjunction on December 12th to reappear in the morning sky around the end of the year.
There are no transits of Mercury in 2017, the next will be Nov 11, 2019.
Behind the Mirror
New Moon
Alaska Gallery
Ochoco Divide
Nudi Gallery
Astronomers Discover A Star That Would Not Die
W. M. Keck Observatory press release…
An international team of astronomers led by Las Cumbres Observatory (LCO) has made a bizarre discovery; a star that refuses to stop shining.
Supernovae, the explosions of stars, have been observed in the thousands and in all cases they marked the death of a star.
“The spectra we obtained at Keck Observatory showed that this supernova looked like nothing we had ever seen before. This, after discovering nearly 5,000 supernovae in the last two decades,” said Peter Nugent, Senior Scientist and Division Deputy for Science Engagement in the Computational Research Division at Lawrence Berkeley National Laboratory who co-authored the study. “While the spectra bear a resemblance to normal hydrogen-rich core-collapse supernova explosions, they grew brighter and dimmer at least five times more slowly, stretching an event which normally lasts 100 days to over two years.”
Researchers used the Low Resolution Imaging Spectrometer (LRIS) on the Keck I telescope to obtain spectrum of the star’s host galaxy, and the Deep Imaging and Multi-Object Spectrograph (DEIMOS) on Keck II to obtain high-resolution spectra of the unusual star itself.
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