NASA is Having a Tough Time Testing the SLS

NASA’s Space Launch System (SLS) has been having some problems getting tested since it rolled out onto launch pad 39B last month. These tests, called wet dress rehearsals, are used to find any problems with loading the propellant and verify that all of the rocket’s systems are able to handle it being exposed to cryogenics.

After this most recent attempt on April 14th, it is clear that the SLS isn’t ready for flight yet. The problems that the teams have been encountering have led them to make some procedural changes and slight adjustments in operations and software triggers. There are also the leak problems that have shown up that have to be addressed.

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SETI Researchers can now Scan all Data at the Very Large Array for any Evidence of Alien Transmissions

The Karl G. Jansky Very Large Array, located in central New Mexico. Credit: NRAO

On February 14th, 2020, the SETI Insitute and the National Radio Astronomy Observatory (NRAO) announced a new partnership, which they appropriately named the Commensal Open-Source Multimode Interferometer Cluster Search for Extraterrestrial Intelligence (COSMIC SETI). This partnership will allow the Karl G. Jansky Very Large Array (VLA) to participate in the Search for Extraterrestrial Intelligence (SETI) for the first time in its history.

In recent weeks, the project took a big step forward with the installation of fiber optic amplifiers and splitters on all VLA antennas, which give COSMIC access to the data streams from the entire VLA. Once this digital backend is online, COSMIC will have access to all data provided by the VLAs 27 radio antennas, which will be able to conduct observations 24/7. In the process, COSMIC SETI will examine around 40 million stars in the Milky Way for possible signs of intelligent life.

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Space for All: Bringing Astronomy to Remote Mountain Villages in Morocco

Credit: AABACA/SSVI/IAU/Asif Astronomy Club, Al-Medhi E.

The night sky is a great leveler, something that people from all walks of life have been able to look upon and draw inspiration from. Unfortunately, the ability to observe the planets and stars and study the mysteries of the Universe is still not open to everyone. When it comes to astronomy, there is still a problem of access, which mirrors disparities in development, education, and health outcomes worldwide.

This disparity is persistent not only in developed and developing nations but between urban and rural communities as well. In southern Morocco, this disparity is felt by public schools in the remote villages of the Atlas Mountains. But thanks to the Asif Astronomy Club and its founder – Ph.D. student El-Mehdi Essaidi – children in these schools are getting the chance to use a professional astronomical telescope to observe the stars and planets for the first time.

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An Ancestor of Supermassive Black Holes, Found at Cosmic Dawn

An international team of astronomers using archival data from the NASA/ESA Hubble Space Telescope and other space- and ground-based observatories have discovered a unique object in the distant, early Universe that is a crucial link between young star-forming galaxies and the earliest supermassive black holes. Current theories predict that supermassive black holes begin their lives in the dust-shrouded cores of vigorously star-forming “starburst” galaxies.
An international team of astronomers using archival data from the NASA/ESA Hubble Space Telescope and other space- and ground-based observatories have discovered a unique object in the distant, early Universe that is a crucial link between young star-forming galaxies and the earliest supermassive black holes. Current theories predict that supermassive black holes begin their lives in the dust-shrouded cores of vigorously star-forming “starburst” galaxies.

At the center of the more-massive galaxies in the Universe lie the intensely powerful and energetic phenomena known as supermassive black holes (SMBHs). This includes the SMBH at the center of the Milky Way, the mysterious radio source known as Sagittarius A*. The presence of these black holes causes the nuclei of these galaxies to become particularly energetic – aka., an Active Galactic Nucleus (AGN), or a Quasar – and causes them to outshine all of the other stars in the galactic disk combined.

For decades, astronomers have sought to learn more about SMBHs and their role in the evolution of the cosmos. A particularly burning question is how early SMBHs formed in the Universe, which would place constraints on how they have influenced galaxies over time. In a surprising discovery, an international team observed the ancestor of an SMBH for the first time. This black hole (known as GNz7q) existed during a period known as “Cosmic Dawn,” far earlier than expected.

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Life Might Have Gotten Started Just 300 Million Years After the Earth Formed

On an outcrop of exposed volcanic and sedimentary rock on the eastern shores of Hudson Bay in northern Quebec, researchers have discovered what may be the earliest fossilized lifeforms ever discovered. These microbial ancestors lived between 3.75 and 4.28 billion years ago, only 300 million years after the Earth itself formed – a blink of an eye in geologic timescales. If life developed this rapidly on Earth, it suggests that abiogenesis – the process by which non-living matter becomes a living organism – is potentially ‘easy’ to achieve, and life in the Universe may be more common than we thought.

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Astronomy Jargon 101: Trans-Neptunian Objects

This composite image of the primordial contact binary Kuiper Belt object 2014 MU69 (officially named Arrokoth) was compiled from data obtained by NASA's New Horizons spacecraft as it flew by the object on Jan. 1, 2019. The image combines enhanced color data (close to what the human eye would see) with detailed high-resolution panchromatic pictures. Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute//Roman Tkachenko
This composite image of the primordial contact binary Kuiper Belt object 2014 MU69 (officially named Arrokoth) was compiled from data obtained by NASA's New Horizons spacecraft as it flew by the object on Jan. 1, 2019. The image combines enhanced color data (close to what the human eye would see) with detailed high-resolution panchromatic pictures. Credits: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute//Roman Tkachenko

In this series we are exploring the weird and wonderful world of astronomy jargon! You’ll be far from home in today’s topic: trans-Neptunian objects!

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Star Formation Simulated in the lab, Using Lasers, of Course

Illustration of the evolution of a massive cloud which indicates the importance of SNR propagation in forming new stars. CREDIT: Albertazzi et al.

The vacuum of space isn’t really a vacuum. A vacuum is defined by Merriam-Webster as “a space absolutely devoid of matter.” However, even empty space has some matter in it. This matter, in the form of dust and gas, tends to collect into what are called molecular clouds. Without anything interfering with them they continue to float as a cloud.

When something happens to interrupt the balance of the molecular cloud, some of that dust and gas starts clumping together. As more and more of this dust and gas clump together gravity takes over and starts forming stars. One way that the balance of a molecular cloud can be interfered with is by a supernova remnant, the remains of an exploded star. Plasma jets, radiation, and other clouds can also interact with these clouds.

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