Space and astronomy news
Do we have a planetary bias when it comes to understanding where life can perpetuate? It’s only natural that we do. After all, we’re on one.
However, planets may not be necessary for life, and a pair of scientists from Scotland and the USA are inviting us to reconsider the notion.
Continue reading “Does Life Really Need Planets? Maybe Not”
Nature often defies our simple explanations. Take comets and asteroids, for example. Comets are icy and have tails; asteroids are rocky and don’t have tails. But it might not be quite so simple, according to new research.
Continue reading “Citizen Scientists Find Fifteen “Active Asteroids””
Red dwarf exoplanet habitability is a hot topic in space science. These small dim stars host lots of exoplanets, including small rocky ones the size of Earth. But the little stars emit extremely powerful flares that can damage and strip away atmospheres.
If we’re ever going to understand red dwarf habitability, we need to understand the atmospheres of the exoplanets that orbit them.
Continue reading “GJ 367b is Another Dead World Orbiting a Red Dwarf”
Earth was once entirely molten. Planetary scientists call this phase in a planet’s evolution a magma ocean, and Earth may have had more than one magma ocean phase. Earth cooled and, over 4.5 billion years, became the vibrant, life-supporting world it is today.
Can the same thing happen to exo-lava worlds? Can studying them shed light on Earth’s transition?
Continue reading “How Do Lava Worlds Become Earth-Like, Living Planets?”
Comets are instantly recognizable by their tails of gas and dust. Most comets originate in the far, frozen reaches of our Solar System, and only visit the inner Solar System occasionally. But some are in the Main Asteroid Belt, mixed in with the debris left over after the Solar System formed.
Astronomers just found water vapour coming from one of them.
“With Webb’s observations of Comet Read, we can now demonstrate that water ice from the early Solar System can be preserved in the asteroid belt.”
Michael Kelley, University of Maryland
Back in April, NASA once again put out the call for proposals for the next generation of robotic explorers and missions. As part of the NASA Innovative Advanced Concepts (NIAC) Program, this consisted of researchers, scientists, and entrepreneurs coming together to submit early studies of new concepts that could one-day help advance NASA’s space exploration goals.
One concept that was selected for Phase III of development was a breakthrough mission and flight system called Mini Bee. This small, robotic mining craft was designed by the Trans Astronautica (
NASA’s Dawn spacecraft has been poking around Ceres since it first established orbit in March of 2015. In that time, the mission has sent back a steam of images of the minor planet, and with a level of resolution that was previously impossible. Because of this, a lot of interesting revelations have been made about Ceres’ composition and surface features (like its many “bright spots“).
In what is sure to be the most surprising find yet, the Dawn spacecraft has revealed that Ceres may actually possess the ingredients for life. Using data from the Dawn spacecraft’s Visible and InfraRed Mapping Spectrometer (VIMS), an international team of scientists has confirmed the existence of organic molecules on Ceres – a find which could indicate that it has conditions favorable to life.
These findings – which were detailed in a study titled “Localized aliphatic organic material on the surface of Ceres” – appeared in the Feb. 17th, 2017, issue of Science. For the sake of their study, the international team of researchers – which was led by Maria Cristina de Sanctis from the National Institute of Astrophysics in Rome, Italy – showed how Dawn sensor data pointed towards the presence of aliphatic compounds on the surface.
Aliphatics are a type of organic compound where carbon atoms form open chains that are commonly bound with oxygen, nitrogen, sulfur and chlorine. The least complex aliphatic is methane, which has been detected in many locations across the Solar System – including in the Martian atmosphere and in both liquid and gaseous form on Saturn’s moon Titan.
From their study, Dr. de Sanctis and her colleagues determined that spectral data obtained by the VIMS instrument corresponded to the presence of these hydrocarbons in a region outside of the Ernutet crater. This crater, which is located in the northern hemisphere of Ceres, measures about 52 km (32 mi) in diameter. The aliphatic compounds which were detected were localized in a roughly 1000 square kilometers region around it.
The team ruled out the possibility that these organic molecules were deposited from an external source – such as a comet or carbonaceous chondrite asteroid. While both have been shown to contain organic molecules in their interior in the past, the largest concentrations on Ceres were distributed discontinuously across the southwest floor and rim of the Ernutet crater and onto an older, highly degraded crater.
In addition, other organic-rich areas were spotted being are scattered to the northwest of the crater. As Dr. Maria Cristina De Sanctis told Universe Today via email:
“The composition that we see on Ceres is similar to some meteorites that has organics and thus we searched for this material. We considered both endogenous and exogenous origin, but the last one seems less likely due to several reasons including the larger abundance observed on Ceres with respect the meteorites.”
Instead, they considered the possibility that they organic molecules were endogenous in origin. In the past, surveys have shown evidence of hydrothermal activity on Ceres, which included signs of surface renewal and fluid mobility. Combined with other surveys that have detected ammonia-bearing hydrated minerals, water ice, carbonates, and salts, this all points towards Ceres having an environment that can support prebiotic chemistry.
“The overall composition of Ceres can favor the pre-biotic chemistry,” said De Sanctis. “Ceres has water ice and minerals (carbonates and phyllosilicates) derived from pervasive aqueous alteration of rocks. It has also material that we think is formed in hydrothermal environments. All these information indicate condition not hostel to biotic molecules.”
These findings are certainly significant in helping to determine if life could exist on Ceres – in a way that is similar to Europa and Enceladus, locked away beneath its icy mantle. But given that Ceres is believed to have originated 4.5 billion years ago (when the Solar System was still in the process of formation), this study is also significant in that it can shed light on the origin, evolution, and distribution of organic life in our the Solar System.
Other members of the research team include researchers from the department of Earth Planetary and Space Sciences at the University of California, the Department of Earth and Planetary Sciences at the University of Tennessee, the Department of Earth, Environmental, and Planetary Sciences at Brown University, the Southwest Research Institute (SwRI), the NASA Goddard Space Flight Center, and NASA’s Jet Propulsion Laboratory.
Further Reading: ScienceMag, SwRI
Continuing with our “Definitive Guide to Terraforming“, Universe Today is happy to present our guide to terraforming Saturn’s Moons. Beyond the inner Solar System and the Jovian Moons, Saturn has numerous satellites that could be transformed. But should they be?
Around the distant gas giant Saturn lies a system of rings and moons that is unrivaled in terms of beauty. Within this system, there is also enough resources that if humanity were to harness them – i.e. if the issues of transport and infrastructure could be addressed – we would be living in an age a post-scarcity. But on top of that, many of these moons might even be suited to terraforming, where they would be transformed to accommodate human settlers.
As with the case for terraforming Jupiter’s moons, or the terrestrial planets of Mars and Venus, doing so presents many advantages and challenges. At the same time, it presents many moral and ethical dilemmas. And between all of that, terraforming Saturn’s moons would require a massive commitment in time, energy and resources, not to mention reliance on some advanced technologies (some of which haven’t been invented yet).
Continue reading “How Do We Terraform Saturn’s Moons?”
Continuing with our “Definitive Guide to Terraforming“, Universe Today is happy to present to our guide to terraforming Jupiter’s Moons. Much like terraforming the inner Solar System, it might be feasible someday. But should we?
Fans of Arthur C. Clarke may recall how in his novel, 2010: Odyssey Two (or the movie adaptation called 2010: The Year We Make Contact), an alien species turned Jupiter into a new star. In so doing, Jupiter’s moon Europa was permanently terraformed, as its icy surface melted, an atmosphere formed, and all the life living in the moon’s oceans began to emerge and thrive on the surface.
As we explained in a previous video (“Could Jupiter Become a Star“) turning Jupiter into a star is not exactly doable (not yet, anyway). However, there are several proposals on how we could go about transforming some of Jupiter’s moons in order to make them habitable by human beings. In short, it is possible that humans could terraform one of more of the Jovians to make it suitable for full-scale human settlement someday.
Welcome back to our ongoing series, “The Definitive Guide To Terraforming”! We continue with a look at the Moon, discussing how it could one day be made suitable for human habitation.
Ever since the beginning of the Space Age, scientists and futurists have explored the idea of transforming other worlds to meet human needs. Known as terraforming, this process calls for the use of environmental engineering techniques to alter a planet or moon’s temperature, atmosphere, topography or ecology (or all of the above) in order to make it more “Earth-like”. As Earth’s closest celestial body, the Moon has long been considered a potential site.
All told, colonizing and/or terraforming the Moon would be comparatively easy compared to other bodies. Due to its proximity, the time it would take to transport people and equipment to and from the surface would be significantly reduced, as would the costs of doing so. In addition, it’s proximity means that extracted resources and products manufactured on the Moon could be shuttled to Earth in much less time, and a tourist industry would also be feasible.
Continue reading “How Do We Terraform The Moon?”