

Photo: David Cendejas, Mount Wilson Superintendent

To recover from the Bobcat Fire and the loss of revenue from the pandemic, Mount Wilson Observatory needs your help! If you can, please make a donation, join with a supporting membership, spread the word by helping out with our GoFundMe campaign, or send us a check the old fashion way at: Mount Wilson Institute, P.O. Box 94146, Pasadena, CA 91109. Our largely volunteer organization receives no regular support from any institutions or government, so any help we get from the public during this tough year is greatly appreciated!!! Thanks to those who have given to us recently in our many hours of need!
For the first half of the 20th Century, Mount Wilson was the most famous observatory in the world. The biggest telescopes were here, and their new designs were changing the way astronomy was done. Among the many discoveries made on the mountain, a few revolutionized our understanding of our place in the Universe. Here, during WWI, Harlow Shapley measured the size of the Milky Way Galaxy for the first time and located our position in it, far from the center. Then, in 1924, Edwin Hubble proved that the mysterious spiral nebulae, which astronomers had speculated about for decades, were in fact distant galaxies similar to our own. Then Hubble teamed up with Milton Humason and confirmed that this immense Universe was expanding. Space itself was getting bigger. This finding, when run backwards in time, led a few decades later to the Big Bang Theory. Mount Wilson is where modern observational cosmology began. It holds a unique place in humanity’s search for our most distant origins. Today, our original solar and nighttime telescopes, the world’s largest for two generations of astronomers, have been joined by the new CHARA array, which has the highest resolution of any optical or infrared system ever built, achieving unprecedented views of the stars.

A publicity photo of astronomer Edwin Hubble guiding Mount Wilson’s 100-inch Telescope in 1924, shortly after he proved the existence of distant galaxies. Photo: Carnegie Observatories/ Huntington Library.


Mars, imaged with Mount Wilson’s 60-inch Telescope on October 18, five days after opposition and its closest approach to Earth until 2035. Astrophotographer Blake Estes and our executive director and telescope operator Tom Meneghini waited patiently for Mount Wilson’s famous seeing to capture the red planet in amazing detail.

Click here to read the Summer issue of our newsletter and get a quick update on our status during the pandemic.
The feature article is the second part of the story of how Mount Wilson astronomers measured, for the first time, the size of a star (other than the Sun). This monumental achievement was made in the fall of 1920, nearly one hundred years ago. To read the first part, see last December’s issue of Reflections here. The followup article in this issue details how Walter Adams, the second director of the Observatory, figured out how to measure distances to thousands of stars, a prerequisite to determining their sizes. When Mount Wilson Observatory was founded, only about 60 stellar distances were known. Adams developed a whole new way to determine distances to stars called spectroscopic parallax. It became an essential rung on the “cosmic distance ladder,” by which astronomers measure the Universe. While Hubble’s work is relatively well known, these two articles offer a good introduction into some of the more obscure ways that astronomers on the mountain used astrophysics to revolutionize their field.
Our Executive Director, Tom Meneghini, updates us on the 100-inch Telescope shutter repair and our current state of affairs. There is also a short article on the Snow Solar Telescope renovation and a big thank you to our 2020 supporters.





Comet Neowise captured by Mount Wilson’s Blake Estes on the Evening of July 17th. Note the beautiful, blue ion tail.

Mount Wilson Observatory’s Blake Estes imaged Comet Neowise as it rose above the San Gabriel Mountains into the morning twilight around 4:45 AM, on Monday, July 13. His images, with the 100-inch Telescope dome in the foreground, were taken from the 150-foot Solar Tower Telescope.

Another shot of the Comet Neowise by Estes. To the right is the bright star Aldebaran in the constellation Taurus.

Another shot with the lights of Los Angeles. The comet made its closest approach to Earth on July 23, and is fading rapidly as it speeds away from the Sun towards the far reaches of our Solar System, not to return for 6,000+ years.

Join the Observatory as a member! By doing so, you get a number of benefits and you help us renew this historic mountaintop, so that it may inspire well into the future. We aim to build a larger community to keep us moving forward with educational STEM programs, undergraduate research, public outreach, ongoing scientific research, and restoration of our 116-year-old observatory.
Please consider becoming a member in 2020, to help us through this year. If you can. Sign up for the individual membership, family membership, or a higher level, all named after one of our famous astronomers. Sign up is easy. Click here to go to our membership page.

Called Sunstar, it is an array of six prisms which take incoming sunlight and refract it, bending the light and spreading it into a spectrum–all the colors of the rainbow. It is mounted near the top of the Observatory’s 150-foot Solar Telescope Tower. With motion controls, it can be remotely directed to project the spectrum to a specific point in the Los Angeles basin. An observer below will see an intense point of light in a single wavelength, shining like a brilliant jewel from the ridgeline of Mount Wilson, 5800 feet above in the San Gabriel Mountains. The prisms can be moved to change the color of light an observer sees, or the observer can walk in one direction or another to change the color. In this case, the observer is actually walking across a giant spectrum some 250 yards long. While still very bright, at the great distances involved, it is perfectly safe to look at a single wavelength of sunlight. For more information and a schedule, go to our Sunstar page.






George Ellery Hale, 1910. Photo: Carnegie/ Huntington Library
The Observatory’s founder, George Ellery Hale, built four telescopes, each one in succession becoming the largest in the world. Here they are shown to the same scale. His first was the 40-inch refractor at Yerkes (in Wisconsin) on the left, but then he began building the more revolutionary–and more compact–reflector telescopes, using a large mirror instead of a lens. His next two are on Mount Wilson, the 60-inch and the 100-inch. (While not quite as grand as his last, these two had the light-gathering power for astronomers to discover our place in the expanding Universe.) His fourth, the 200-inch Hale Telescope at Palomar, is represented on the right by one of Russell Porter’s famous cutaway drawings. This image has been reversed and extended on the left side for a better comparison of the relative sizes of the full domes. Hale’s telescopes were the biggest from 1897, when Yerkes opened, to 1993, when the Keck telescope in Hawaii was completed–a span of 96 years. To see these drawings enlarged, click here. Drawing credits: University of Chicago/Yerkes Observatory, Carnegie Observatories, Palomar Observatory/Caltech.
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