Wed. 11/20 - We're Not Sure About Tonight's Weather Yet. We'll Try To Decide By 3:30 Pm If We'll Open

Follow this link to learn more about the BSU Center for the Advancement of Stem Education!

So far, the forecast this Wednesday doesn't look good, but we'll wait til that day to make the announcement. Stay tuned for August public night announcements, too!

Wed. 11/13: We expect gorgeous, clear skies tonight! We'll be open, 6 -7 for public night and from 7 - 9 for attendees of Open Lab Night.

Please be aware the elevator which goes to the 5th floor (observatory) is out of order. We will only be accessible by stairs tonight, though you can still take the other elevator to the 4th floor.

The Hidden Galaxy, IC 342 // Ondřej Pešák

Wed. Nov. 8 - Observatory closed due to cloud cover. We'll try again next week.

Wow, it really does look like a hummingbird!

2023 September 25

Arp 142: The Hummingbird Galaxy Image Credit: NASA, ESA, Hubble, HLA; Processing & Copyright: Basudeb Chakrabarti

Explanation: What’s happening to this spiral galaxy? Just a few hundred million years ago, NGC 2936, the upper of the two large galaxies shown at the bottom, was likely a normal spiral galaxy – spinning, creating stars – and minding its own business. But then it got too close to the massive elliptical galaxy NGC 2937, just below, and took a turn. Sometimes dubbed the Hummingbird Galaxy for its iconic shape, NGC 2936 is not only being deflected but also being distorted by the close gravitational interaction. Behind filaments of dark interstellar dust, bright blue stars form the nose of the hummingbird, while the center of the spiral appears as an eye. Alternatively, the galaxy pair, together known as Arp 142, look to some like Porpoise or a penguin protecting an egg. The featured re-processed image showing Arp 142 in great detail was taken recently by the Hubble Space Telescope. Arp 142 lies about 300 million light years away toward the constellation of the Water Snake (Hydra). In a billion years or so the two galaxies will likely merge into one larger galaxy.

∞ Source: apod.nasa.gov/apod/ap230925.html

2023 October 18

Dust and the Western Veil Nebula Image Credit & Copyright: Jiang Wu

Explanation: It’s so big it is easy to miss. The entire Veil Nebula spans six times the diameter of the full moon, but is so dim you need binoculars to see it. The nebula was created about 15,000 years ago when a star in the constellation of the Swan (Cygnus) exploded. The spectacular explosion would have appeared brighter than even Venus for a week - but there is no known record of it. Pictured is the western edge of the still-expanding gas cloud. Notable gas filaments include the Witch’s Broom Nebula on the upper left near the bright foreground star 52 Cygni, and Fleming’s Triangular Wisp (formerly known as Pickering’s Triangle) running diagonally up the image middle. What is rarely imaged – but seen in the featured long exposure across many color bands – is the reflecting brown dust that runs vertically up the image left, dust likely created in the cool atmospheres of massive stars.

∞ Source: apod.nasa.gov/apod/ap231018.html

Cosmic fireworks ahead! This dramatically colorful image shows MACS J0717, one of the most complex and distorted galaxy clusters known. It was formed by the collision of four smaller galaxy clusters. A visible-light image from the Hubble Space Telescope shows hundreds of galaxies, both within the cluster and throughout the background, and myriad foreground stars. A pink overlay represents radio data from the Karl G. Jansky Very Large Array, which traces enormous shock waves and turbulence. The diffuse emission in blue, from the Chandra X-ray Observatory, highlights gas with temperatures of millions of degrees. Credit: NASA, ESA, CXC, NRAO/AUI/NSF, STScI, and R. van Weeren (Harvard-Smithsonian Center for Astrophysics); NASA, ESA, J. Lotz (STScI), and the Hubble Frontier Fields team. ALT TEXT: Hundreds of small galaxies of various shapes on the black background of space. They are concentrated near the center of the image. Dramatic pink ribbons form a curving L shape near the center. Below them, a linear pink feature with a blue blob in the middle extends from upper left to lower right. Diffuse blue light fills much of the field of view and is brightest just to the right of the pink ribbons.

If galaxies could talk, we’d want to ask for this galaxy’s skincare routine!

Meet I Zwicky 18, a galaxy lying 60 million light-years away in the constellation Ursa Major.

The bluish-white knots in the center are regions where stars are forming at a rapid rate. These large hubs of stellar creation and the lack of heavy elements in the surrounding gas caused astronomers to think that this dwarf irregular galaxy was very young, since it resembles galaxies in the early universe.

However, the Hubble Space Telescope revealed that I Zwicky 18 is more mature than it first appears. Hubble found faint, older stars within the galaxy, indicating that I Zwicky 18 has been forming stars for more than a billion years.

Credit: NASA, ESA, A. Aloisi (Space Telescope Science Institute and European Space Agency).

ALT TEXT: A bright white and blue oval-shaped area takes up most of the view and is largely centered. Cloud-like wisps of blue material surround the bright-white center, forming a fluffy wreath-like shape. The fluffy material begins as light blue near the center and gradually darkens moving outward. Stars, seen as many bright white and yellow small points of light, are densely grouped in the white and light blue region, forming two roughly circular clumps, one in the upper left and one in the lower right. The corners of the image are dark and mostly empty, with a few larger, fuzzy yellow points of light scattered infrequently throughout.

Did you know that there are 5 known dwarf planets in our solar system? Everyone knows Pluto, but there is also Ceres, Haumea, Makemake and Eris.

Info from: https://www.iau.org/public/themes/pluto/#n6