NASA recently conducted its inaugural public gathering regarding UFO sightings or "unidentified aerial phenomena" (UAPs). Taking place one year after initiating a comprehensive investigation into intriguing UFO sightings, NASA revealed numerous unsolved mysteries.
In a groundbreaking analysis utilizing the latest telescope observations, astronomers from the University of Florida have revealed that one-third of all common planets in our galaxy may be classed as 'hospitable planets'.
Using NASA’s James Webb Space Telescope to look at a rocky exoplanet known as GJ 486 b, researchers find signs of water vapour – hinting at an atmosphere.
With civilian supersonic flights over land being banned for the last 50 years due to noise complaints. NASA’s Quesst has a plan: Flying faster than sound, but with innovative technology to drastically reduce noise.
New information provided by the James Webb Space Telescope indicates six galaxies that shouldn’t exist - the telescope has revealed these earliest and largest galaxies on NASA’s radar might be even bigger and more mature than previously thought possible.
Research has revealed a new way of producing and shaping large high-quality mirrors for space telescopes allowing for them to be rolled up and stored compactly inside during launch.
For the first time, a raging dust storm has been observed by the James Webb Space Telescope on the exoplanet known as VHS 1256b, which is outside our Solar System.
The UK government are investing £113 million in hydrogen and all-electric flight technologies to revolutionise zero-emission flights that are “guilt-free”.
Combining data on the Tarantula Nebular from two different observing proposals, a team from Hubble has revealed how interstellar dust interacts with starlight in a variety of environments.
Using the QUIJOTE experiment, scientists are now producing the most accurate description until now of the polarization in the microwave emission processes in our galaxy.
![Figure 1 - The figure illustrates the diversity and multi-scale nature of the structures in the Galaxy. The first two lines are real astronomical images, which go from the galactic disk itself and down to the planet-forming disks. The last two lines are generated from numerical simulations and aim to understand and interpret the observations. [adapted from Facchini et al. 2025, Göller et al. 2025, Hennebelle et al. 2022, Lebreuilly et al. 2024, Molinari et al. 2016, 2025, Reissl et al. 2016]](https://www.openaccessgovernment.org/wp-content/uploads/2025/08/figure.png)
