The Universe's Brightest Lights Have Some Dark Origins

Ask Ethan: How Does Very-Long-Baseline Interferometry Allow Us To Image A Black Hole?

“[The Event Horizon Telescope] uses VLBI. So what is interferometry and how was it employed by [the Event Horizon Telescope]? Seems like it was a key ingredient in producing the image of M87 but I have no idea how or why. Care to elucidate?”

If it were easy to network radio telescopes together across the world, we’d have produced an image of a black hole’s event horizon long ago. Well, it’s not easy at all, but it is at least possible! The technique that enabled it is known as VLBI: very-long-baseline interferometry. But there are some critical steps that aren’t very obvious that need to happen in order for this method to succeed. Remarkably, we learned how to do it and have successfully employed it, and the Event Horizon Telescope marks the first time we’ve ever been able to get an image with a telescope that’s effectively the size of planet Earth!

Come get the incredible science behind how the technique of VLBI enabled the Event Horizon Telescope to construct the first-ever image of a black hole’s event horizon!

"Your dreams are yours to pursue, they are beautiful, and you can't let anyone slow you down." ~ Sky Taylor to Vesha Celeste Pathway to the Stars: Part 1, Vesha Celeste #scifiauthor #spaceopera #authorsofinstagram #scifi #sciencefictionnovels #biotechnology #neuroscience #nanotechnology #longevity #theoreticalphysics #astronomy #virtualuniverse https://www.instagram.com/p/Bunk5e_ARbJ/?utm_source=ig_tumblr_share&igshid=fezlj30jxc0z

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Black-Hole Powered Jets Forge Fuel for Star Formation

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have discovered a surprising connection between a supermassive black hole and the galaxy where it resides. 

Powerful radio jets from the black hole – which normally suppress star formation – are stimulating the production of cold gas in the galaxy’s extended halo of hot gas. This newly identified supply of cold, dense gas could eventually fuel future star birth as well as feed the black hole itself.

The researchers used ALMA to study a galaxy at the heart of the Phoenix Cluster, an uncommonly crowded collection of galaxies about 5.7 billion light-years from Earth.

The central galaxy in this cluster harbors a supermassive black hole that is in the process of devouring star-forming gas, which fuels a pair of powerful jets that erupt from the black hole in opposite directions into intergalactic space. Astronomers refer to this type of black-hole powered system as an active galactic nucleus (AGN).

Read more ~ AlmaObservatory.org

Video: Video explaining the complex relationship between a supermassive black hole and its host galaxy.     Credit: NRAO/AUI/NSF; ALMA (ESO/NAOJ/NRAO); Animations: NASA/GSFC/CI Lab, ESO; Science Images: NASA/ESA Hubble; Chandra X-Ray Observatory/NASA/MIT, M. McDonald; Music, Comfortable Mystery 4 - Film Noire by Kevin MacLeod

Images: Left: Composite image showing how powerful radio jets from the supermassive black hole at the center of a galaxy in the Phoenix Cluster inflated huge “bubbles” in the hot, ionized gas surrounding the galaxy (the cavities inside the blue region imaged by NASA’s Chandra X-ray observatory). Hugging the outside of these bubbles, ALMA discovered an unexpected trove of cold gas, the fuel for star formation (red). The background image is from the Hubble Space Telescope.     Credit: ALMA (ESO/NAOJ/NRAO) H.Russell, et al.; NASA/ESA Hubble; NASA/CXC/MIT/M.McDonald et al.; B. Saxton (NRAO/AUI/NSF) Right: ALMA image of cold molecular gas at the heart of the Phoenix Cluster. The filaments extending from the center hug enormous radio bubbles created by jets from a supermassive black hole. This discovery sheds light on the complex relationship between a supermassive black hole and its host galaxy.     Credit: ALMA (ESO/NAOJ/NRAO), H. Russell et al.; B. Saxton (NRAO/AUI/NSF) Bottom: Artist impression of galaxy at the center of the Phoenix Cluster. Powerful radio jets from the supermassive black hole at the center of the galaxy are creating giant radio bubbles (blue) in the ionized gas surrounding the galaxy. ALMA has detected cold molecular gas (red) hugging the outside of the bubbles. This material could eventually fall into the galaxy where it could fuel future star birth and feed the supermassive black hole.     Credit: B. Saxton (NRAO/AUI/NSF)

An un-released remix of "Into the Light." 2004 7 additional remixes of C+E's Billboard Club Hit, including mixes by Dave Aude, Black Light Odyssey (Floria & DeGraff,) and Andres Oscuro are available on the: "Into the Light" - (Remixes) single at iTunes, Amazon and the C+E Shop.

No matter what people tell you, words and ideas can change the world.

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Now, together, Part 1, Vesha Celeste, and Part 2, Eliza Williams, have been paired together, and are available for those interested in the types of science, the directions of science, and the speculation that leads to well-being and quality of life, feel free to follow, message, and share ideas, and be a part of a positive future where, if we so choose, we can navigate the stars. This is just the beginning of this series and prequel, “Pathway to the Stars,” to a giant series, “Further than Before!” Please enjoy. https://www.amazon.com/author/matthewopdyke #sciencefiction #scifi #sciencefictionfantasy #scififantasy #politicalscifi #politicalsciencefiction #strongfemalelead #utopian #technologyidealism #neuroscience #nanotech #nanotechnology #physics #theoreticalphysics #problemresolution #apoliticalscifi #biology #CRISPR #stemcellresearch #geneticmodification https://www.instagram.com/p/BpUMW6ZgB1I/?utm_source=ig_tumblr_share&igshid=1nhhhf9ev7vpq

Meet Fermi: Our Eyes on the Gamma-Ray Sky

Black holes, cosmic rays, neutron stars and even new kinds of physics — for 10 years, data from our Fermi Gamma-ray Space Telescope have helped unravel some of the biggest mysteries of the cosmos. And Fermi is far from finished!

On June 11, 2008, at Cape Canaveral in Florida, the countdown started for Fermi, which was called the Gamma-ray Large Area Space Telescope (GLAST) at the time. 

The telescope was renamed after launch to honor Enrico Fermi, an Italian-American pioneer in high-energy physics who also helped develop the first nuclear reactor. 

Fermi has had many other things named after him, like Fermi’s Paradox, the Fermi National Accelerator Laboratory, the Enrico Fermi Nuclear Generating Station, the Enrico Fermi Institute, and the synthetic element fermium.

Photo courtesy of Argonne National Laboratory

The Fermi telescope measures some of the highest energy bursts of light in the universe; watching the sky to help scientists answer all sorts of questions about some of the most powerful objects in the universe. 

Its main instrument is the Large Area Telescope (LAT), which can view 20% of the sky at a time and makes a new image of the whole gamma-ray sky every three hours. Fermi’s other instrument is the Gamma-ray Burst Monitor. It sees even more of the sky at lower energies and is designed to detect brief flashes of gamma-rays from the cosmos and Earth.

This sky map below is from 2013 and shows all of the high energy gamma rays observed by the LAT during Fermi’s first five years in space.  The bright glowing band along the map’s center is our own Milky Way galaxy!

So what are gamma rays? 

Well, they’re a form of light. But light with so much energy and with such short wavelengths that we can’t see them with the naked eye. Gamma rays require a ton of energy to produce — from things like subatomic particles (such as protons) smashing into each other. 

Here on Earth, you can get them in nuclear reactors and lightning strikes. Here’s a glimpse of the Seattle skyline if you could pop on a pair of gamma-ray goggles. That purple streak? That’s still the Milky Way, which is consistently the brightest source of gamma rays in our sky.

In space, you find that kind of energy in places like black holes and neutron stars. The raindrop-looking animation below shows a big flare of gamma rays that Fermi spotted coming from something called a blazar, which is a kind of quasar, which is different from a pulsar… actually, let’s back this up a little bit.

One of the sources of gamma rays that Fermi spots are pulsars. Pulsars are a kind of neutron star, which is a kind of star that used to be a lot bigger, but collapsed into something that’s smaller and a lot denser. Pulsars send out beams of gamma rays. But the thing about pulsars is that they rotate. 

So Fermi only sees a beam of gamma rays from a pulsar when it’s pointed towards Earth. Kind of like how you only periodically see the beam from a lighthouse. These flashes of light are very regular. You could almost set your watch by them!

Quasars are supermassive black holes surrounded by disks of gas. As the gas falls into the black hole, it releases massive amount of energy, including — you guessed it — gamma rays. Blazars are quasars that send out beams of gamma rays and other forms of light — right in our direction. 

When Fermi sees them, it’s basically looking straight down this tunnel of light, almost all the way back to the black hole. This means we can learn about the kinds of conditions in that environment when the rays were emitted. Fermi has found about 5,500 individual sources of gamma rays, and the bulk of them have been blazars, which is pretty nifty.

But gamma rays also have many other sources. We’ve seen them coming from supernovas where stars die and from star factories where stars are born. They’re created in lightning storms here on Earth, and our own Sun can toss them out in solar flares. 

Gamma rays were in the news last year because of something Fermi spotted at almost the same time as the National Science Foundation (NSF)’s Laser Interferometer Gravitational-Wave Observatory (LIGO) and European Gravitational Observatory’s Virgo on August 17, 2017. Fermi, LIGO, Virgo, and numerous other observatories spotted the merger of two neutron stars. It was the first time that gravitational waves and light were confirmed to come from the same source.

Fermi has been looking at the sky for almost 10 years now, and it’s helped scientists advance our understanding of the universe in many ways. And the longer it looks, the more we’ll learn. Discover more about how we’ll be celebrating Fermi’s achievements all year.

Make sure to follow us on Tumblr for your regular dose of space: http://nasa.tumblr.com.

Pathway to the Stars: Part 9, Allure & Spacecraft "We cannot engage in human progression as solo artists, alone, and expect long-term and optimal results. While we can inspire momentum for a time, while working diligently, ultimately the laws of chaos will prevail unless we work together to preserve our world, our solar system, and our Universe." ~ Eliza Williams Vesha has completed her Virtual Universe training, and now she becomes immersed in missions and callings as never before! Enjoy as she tackles issues where society seems muddled in the chains of self-bondage, rather than moving forward with a bright and beautiful future for all. Joanne revisits a problem that can affect Eliza Williams' hopes for the future. Among Eliza's many goals within the Solar System to that end, related to space travel, is the construction of spacecraft being built just above Pluto! Enjoy this Space Opera as Eliza continues her quest to nurture humanity into a space-faring, world-preserving, and Universe-exploring civilization! She believes that the most significant step toward moving forward is kindness, and that kindness is the greatest strength we have! ISBN: 978-1951321093 LCCN: 2019918425eBook: https://smile.amazon.com/dp/B081XLG9JV Paperback: https://smile.amazon.com/dp/195132109X For more info: https://www.mjopublications.com https://smile.amazon.com/author/matthewopdyke Tags: #sciencefiction #scifi #spaceopera #fantasy #stem #astronomy #sentience #spacecraft #spaceelevator #wellbeing #author #matthewjopdyke #ebook #paperback #amazon