Space News & Blog Articles

It’s time to take a thorough, more serious look at using geoengineering to protect the planet’s icesheets, according to a group of scientists who have released a new report examining the issue. Glacial geoengineering is an emerging field of study that holds some hope for Earth’s diminishing glaciers and ice sheets.

While black holes are known as the most destructive objects in the universe, their evolution is largely shrouded in mystery. This is because while astronomers are familiar with supermassive black holes that exist at the center of galaxies like our own and black holes whose masses are less than 100 times the size of our Sun, the notion of intermediate-mass black holes (IMBHs) have largely eluded discovery. However, this might change with the recent discovery of a black hole candidate that could exist within the globular cluster, Omega Centauri, and holds the potential to be the “missing link” in scientists better understanding black hole evolution.

Ae inflatable habitats the future of human space exploration? This is what the space-tech company, Sierra Space, hopes to achieve as they recently conducted a successful Ultimate Burst Pressure test on June 18 with its Large Integrated Flexible Environment (LIFE®) technology at NASA’s Marshall Space Flight Center. The goal of these tests is to inflate the test article until it explodes while ascertaining if the maximum pressure falls within NASA’s strict safety guidelines regarding a recommended operating pressure of 60.8 psi (maximum operating pressure of 15.2 psi times four as a safety factor). Upon explosion, Sierra Space engineers immediately found the recent test achieved 74 psi, thus exceeding NASA’s safety standards by 22 percent.

Academic research on solar system objects has increased dramatically over the last twenty years. However, information on most of the estimated 1.2 million objects discovered in our solar system has been spread throughout various databases and research papers. Putting all that data into a single data store and making it easy to access would allow researchers to focus on their research rather than on where to collect data. That is the idea behind the Solar System Open Database Network (SsODNet), a project by data scientists at the Observatoire de Paris.

Universe Today has had the incredible opportunity of exploring various scientific fields, including impact craters, planetary surfaces, exoplanets, astrobiology, solar physics, comets, planetary atmospheres, planetary geophysics, cosmochemistry, meteorites, radio astronomy, extremophiles, organic chemistry, black holes, cryovolcanism, planetary protection, dark matter, supernovae, neutron stars, and exomoons, and how these separate but unique all form the basis for helping us better understand our place in the universe.

How will future robotic explorers navigate the difficult subterranean environments of caves and lava tubes on the Moon and Mars? This is what a recent study published in Science Robotics hopes to address as a team of researchers from Stanford University investigated the use of a novel robotic explorer called ReachBot, which could potentially use its unique mechanical design to explore deep caves and lava tubes on the Moon and Mars in the future.

One of the hazards astronauts must contend with is muscle loss. The more time they spend in a microgravity environment, the more muscle loss they suffer. Astronauts use exercise to counter the effects of muscle atrophy, but it’s not a perfect solution. Researchers want to develop drugs to help, and understanding the muscle-loss process in space is a critical first step.

What does it take to have life at another world? Astrobiologists say you need water, warmth, and something for life to eat. If it’s there, it’ll leave signs of itself in the form of organic molecules called amino acids. Now, NASA scientists think that those “signatures” of life—or potential life—could exist just under the icy surfaces of Europa and Enceladus.

Sometimes, brainstorming does work. In 2019, America’s National Science Foundation (NSF) held the CubeSat Ideas Lab, a shindig that brought together some of the world’s best CubeSat designers. One outcome of that shindig is the Virtual Super-Resolution Optics with Reconfigurable Swarms, or VISORS, mission. Expected to launch in October, this mission will be a proof of concept for many swarming technologies in CubeSats. Hopefully, It will also capture a pretty impressive picture of the Sun’s corona.

What would the economy of a future Mars society look like, and how could it be self-sustaining while being completely sovereign from Earth and its own economy? This is what a recent study submitted to Space Policy hopes to address as a sole researcher discusses a model that could be used for establishing economic freedom on Mars, enabling both monetary and political stability across all Red Planets settlements. This study holds the potential to help scientists, economists, and world leaders better understand plausible governmental systems used by human settlers on other worlds while maintaining sovereignty from Earth and its own governmental law and order.

Mars exploration vehicles typically have wheels, allowing them to traverse some challenging terrain on the Red Planet. However, eventually, their systems start to wear down, and one of their wheels gets stuck. The “Free Spirit” campaign in 2009 was the most widely known case. Unfortunately, that campaign wasn’t successful, and now, 15 years later, Spirit remains stuck in its final resting place. Things might have been different if NASA had adopted a new robot paradigm developed by Guangming Chen and his colleagues at the Nanjing University of Aeronautics & Astronautics Lab of Locomotion Bioinspiration and Intelligent Robots. They devised a robot based on a desert lizard, with adaptable feet and a flexible “spine” that, according to their calculations, would be well suited to traversing over Martian regolith.

Dark matter is a mysterious and captivating subject. It’s a strange concept and we don’t really have a handle on what it actually is. One of the strongest pieces of evidence that dark matter is a particle comes from cosmic collisions. These collisions chiefly occur when clusters of galaxies interact such as the famous Bullet Cluster. Gravitational lensing reveals how the dark matter component couples from gas and dust in the cluster but now, astronomers have found another galaxy cluster collision but it is different, showing the collision from a new angle. 

Johannes Kepler is probably most well known for developing the laws of planetary motion. He was also a keen solar observer and in 1607 made some wonderful observations of our nearest star using a camera obscura. His drawings were wonderfully precise and enabled astronomers to pinpoint where the Sun was in its 11-year cycle. Having taken into account Kepler’s location and the location of sunspots, a team of researchers have identified the Sun was nearing the end of solar cycle-13.

Mercury, the closest planet to our Sun, is also one of the least understood in the Solar System. On the one hand, it is similar in composition to Earth and the other rocky planets, consisting of silicate minerals and metals differentiated between a silicate crust and mantle and an iron-nickel core. But unlike the other rocky planets, Mercury’s core makes up a much larger part of its mass fraction. Mercury also has a mysteriously persistent magnetic field that scientists still cannot explain. In this respect, Mercury is also one of the most interesting planets in the Solar System.

The JWST has directly imaged its first exoplanet, a temperate super Jupiter only about 12 light-years away from Earth. It could be the oldest and coldest planet ever detected.

Venus’s atmosphere has drawn a lot of attention lately. In particular, the consistent discovery of phosphine in its clouds points to potential biological sources. That, in turn, has resulted in numerous suggested missions, including floating a balloon into the atmosphere or having a spacecraft scoop down and suck up atmospheric samples. But a team of engineers led by Jeffrey Balcerski, now an adjunct at Kent State University but then part of the Ohio Aerospace Institute, came up with a different idea years ago – use floating sensor platforms shaped like leaves to collect a wide variety of data throughout Venus’ atmosphere.

It’s not always possible to observe the night sky from the surface of the Earth. The blocking effects of the atmosphere mean we sometimes need to put telescopes out into space. The Chandra X-Ray Observatory is one such telescopes and it has just completed its 25th year of observations. To celebrate, NASA have just released 25 never-before-seen images of various celestial objects in x-rays. The collection includes images showing the region around black holes, giant clouds of hot gas and extreme magnetic fields. Sadly though, NASA is planning on shutting down the mission to save budget so best to enjoy the images while you can. 

SpaceX is flying again after the Federal Aviation Administration ruled that the company can resume Falcon 9 rocket launches while the investigation into a failed July 11 mission continues.

When we think of Jupiter-type planets, we usually picture massive cloud-covered worlds orbiting far from their stars. That distance keeps their volatile gases from vaporizing from stellar heat, similar to what we’re familiar with in our Solar System. So, why are so many exoplanets known as “hot Jupiters” orbiting very close to their stars? That’s the question astronomers ask as they study more of these extreme worlds.

Venus is known for being really quite inhospitable with high surface temperatures and Mars is known for its rusty red horizons. Even the moons of some of the outer planets have fascinating environments with Europa and Enceladus boasting underground oceans. Recent observations from the James Webb Space Telescope show that Ariel, a moon of Uranus, is also a strong candidate for a sub surface ocean. How has this conclusion been reached? Well JWST has detected carbon dioxide ice on the surface on the trailing edge of features trailing away from the orbital direction. The possible cause, an underground ocean!

When the James Webb Space Telescope was launched it came with a fanfare expecting amazing things, much like the Hubble Space Telescope. One of JWST’s most anticipated target was TRAPPIST-1. This inconspicuous star is host to seven Earth-sized planets, with at least three in the habitable zone. The two inner planets are airless worlds but so far there has been no word of the third planet, the first in the habitable zone. The question is why and what makes it so tricky to observe?