Sunday, August 2, 2015
Sunday, July 12, 2015
I've discussed the issue of whether Pluto is a planet elsewhere and I don't have much to add except that Alan Stern (the principle investigator of the New Horizons mission) argues that Pluto should be considered a planet. There are differences of opinion on the matter.
If you consider Pluto a planet, Pluto is the only planet which has never been visited by a planet (either landing or flyby). That is until New Horizons.
If you don't, Pluto is still an interesting place. We know very little about Pluto and New Horizons should give us a lot of new data. If fact it already has, and unless there is a major failure it will continue to do so. It will take time to analyze the data, but it is very likely we will have a new understanding of Pluto in the near future.
For more information...
Alan Stern talked about New Horizon and Pluto on NPR's Science Friday (July 10th), see http://www.sciencefriday.com/
Dr Stern gave a talk at the University of Michigan in February 2009. This talk discussed Pluto and the solar system; for a description of this talk see http://www.lowbrows.org/reflections/2009/dwarshow.5.html .
See also see this page from NASA: http://www.nasa.gov/feature/latest-images-of-pluto-from-new-horizons
Wednesday, July 8, 2015
Pulsars are rotating neutron stars, the leftover remnants of stars that once shone and were more massive than our sun. Pulsars "pulse" because they emit highly directional "beams" of electromagnetic energy from their poles, and we detect this every time they rotate and the beam crosses our path. This can happen thousands of times per second, making them excellent timekeepers!
Stars come in different sizes, and the one of interest in 2018 is about 15 times as massive as our sun. It is in the constellation Cygnus and is about 5,000 light years away from us. This star has a binary companion, a pulsar, that will actually move through its outer atmosphere in 2018. The orbit is fairly long at 25 years.
Check out the NASA press release for more information.
Friday, April 10, 2015
By Aimee Balfe (Department of Astronomy) and Carol Rabuck (Department of Physics)
University of Michigan scientists and students will build components of a giant camera that will map 30 million galaxies' worth of the universe in three dimensions.
To read the rest of the article, go to: http://record.umich.edu/articles/u-m-help-build-next-generation-dark-energy-probe
Wednesday, March 4, 2015
Exoplanets are planets in orbit around stars other than our own sun. Over the past decade, hundreds of exoplanets have been discovered. The hope: exoplanets similar to the earth will eventually be discovered, planets that might be capable of supporting life. In fact we've discovered a wide variety of exoplanets, but we haven't found life beyond our solar system.
Individuals like you can be part of the process of naming one of these exoplanets. For now everyone must go through an official IAU astronomical organization. At the time of this post, there are two such organizations in the Ann Arbor area, the Ann Arbor Hands Museum and the University Lowbrow Astronomers. If you want to participate now you should look at the rules for this process (see the following web site)...
If you want to work through the Lowbrows, please leave a suggested name along with a short reason why you think it is an good name for a planet as a comment on this post. We will go through the comments, we are allowed to submit one name, so we will pick what we consider to be the best name and submit it.
You can also go to https://directory.iau.org/directory to find other organizations to work with.
Over the next few months suggested names will be send to the IAU by the Lowbrows and other organizations. Sometime this summer, all interested parties will be allowed to vote on the different names that the IAU has received.
Wednesday, January 28, 2015
I like articles such as this one that take mundane phenomena and link them to the stars. Though worth a read, punchline / TL;DR of this is that nuclear fusion stops generating excess energy at iron and this leads to an abundance of iron seeding the universe following supernovae, finding its way to rocky planets such as ours. Thus, iron oxide is plentiful, cheap, and just happens to make red paint.
Monday, January 19, 2015
This is easy to observe with a small telescope, provided it is clear and dark at your location while the transit is taking place. For observers in the eastern United States (in the Eastern time zone) here is the timing....
Friday January 23 22:09 Callisto's shadow appears
Friday January 23 23:36 Io's shadow appears
Saturday January 24 00:03 Io begins transit
Saturday January 24 01:27 Europa's shadow appears
Saturday January 24 01:31 Callisto begins transit
Saturday January 24 01:54 Io's shadow disappears
Saturday January 24 02:07 Io ends transit
Saturday January 24 02:17 Europa begins transit
Saturday January 24 02:59 Callisto's shadow disappears
Saturday January 24 04:23 Europa's shadow disappears
Saturday January 24 04:54 Europa ends transit
(These timings are approximate, it is best to start observe a few minutes before the times indicated to be safe). Observers at other locations can adjust the time zone to determine the timings. If the sun is above the horizon at the specified time, you wont be able to see the transit.
See this article from Astronomy Now: "Jupiter’s moon dance and shadow play to delight observers:" http://astronomynow.com/2014/12/03/jupiters-moon-dance-and-shadow-play-to-delight-observers/
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