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The recent James Webb Space Telescope(JWST) guide camera’s test image looks really similar to Hubble’s deep fields, which are my favorite. I decided to take a long exposure to the same target to see what my telescope can see and compare it to JWST’s image. I found one really faint galaxy 26–32 million light-years away, and a cute planetary nebula called Abell 39, pause and see if you can find it in my image.

- Scope: Celestron RASA 8.
- Mount: Ioptron cem40.
- Camera: ZWO ASI183mm pro.
- Guide scope: ZWO mini120mm.
- Guide Camera: ZWO ASI224mc.
- Filter: Astronomik MaxFR 12nm Ha filter.

NASA article: https://www.nasa.gov/image-feature/countdown-to-the-webb-telescopes-first-images.

More of my astrophotography work on Instagram.
https://www.instagram.com/ethan_gone/

Epic music: Omega by Scott Buckley.
Scott Buckley is an amazing musician, check out his work:
www.scottbuckley.com.au/library.
https://www.youtube.com/channel/UCUuUqWLLsUjheuYkP9AWxTA

Astronomers from the University of Warwick reveal a new phenomenon dubbed the “rocking shadow” effect that describes how disks in forming planetary systems are oriented, and how they move around their host star. The effect also gives clues as to how they might evolve with time. Dr. Rebecca Nealon presented the new work this week at the 2022 National Astronomy Meeting at the University of Warwick.

Stars are born when a large cloud of gas and dust collapses in on itself. The leftover material that doesn’t make it into the star ends up circling around it, not unlike how water swirls around the drain before falling in. This swirling mass of gas and dust is called a , and it’s where planets like the Earth are born.

Protoplanetary disks are often thought to be shaped like dinner plates—thin, round and flat. However, recent telescope images from the Atacama Large Millimeter/Submillimeter Array (ALMA) show that this is not always the case. Some of the disks seen by ALMA have shadows on them, where the part of the disk closest to the star blocks some of the stellar light and casts a shadow onto the outer part of the disk. From this shadow pattern, it can be inferred that the inner part of the disk is oriented completely differently to the outer part, in what is called a broken disk.

Breaking the previous record by 60 percent.

The team behind the first Chinese X-ray astronomy satellite, Insight-HXMT, has discovered the strongest magnetic field directly measured in the universe hitherto.

It is a known fact that neutron stars generate the strongest magnetic fields in the universe. These magnetic fields, close to a neutron star’s surface, can only be measured accurately and directly by looking for cyclon resonance scattering features (CRSF). The Insight-HXMT team discovered a cyclotron absorption line with an energy of 146 keV in the neutron star X-ray binary Swift J0243.6+6124, which translates to a surface magnetic field of more than 1.6 billion Tesla.