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Astronomers discover a ‘Hot Neptune’ in a Tight Orbit

A Neptune-sized planet, TOI-3261 b, makes a scorchingly close orbit around its host star. Only the fourth object of its kind ever found, the planet could reveal clues as to how planets such as these form.

An international team of scientists used the NASA space telescope, TESS (the Transiting Exoplanet Survey Satellite), to discover the exoplanet, then made further observations with ground-based telescopes in Australia, Chile, and South Africa. The measurements placed the new planet squarely in the “hot Neptune desert”—a category of planets with so few members that their scarcity evokes a deserted landscape.

The team, led by astronomer Emma Nabbie of the University of Southern Queensland, published their paper on the discovery, “Surviving in the Hot Neptune Desert: The Discovery of the Ultrahot Neptune TOI-3261 b,” in The Astronomical Journal in August 2024.

Season 5, Episode 31: Meet a Webb Scientist Who Looks Back in Time

Thirty-five years ago, our Cosmic Background Explorer, or COBE, was launched! The satellite was a crucial stepping stone in understanding the cosmic microwave background — the afterglow of the earliest moments of our universe.

Launched from what’s now Vandenberg Space Force Base on Nov. 18, 1989, COBE carried three instruments to space to measure microwave and infrared light across the whole sky. COBE’s observations helped us learn how our universe started and evolved.

COBE discovered that the oldest light in the universe contained tiny temperature variations (red indicates hotter regions, blue colder). These were the seeds for the gravitational formation of structures of galaxies seen in the universe today.

S James Webb Space Telescope: + There are still many questions we want to answer about the early universe, and our missions continue to study it and refine our understanding.

Explore the universe’s baby picture: https://go.nasa.gov/3VPXWgF


TIMELAPSE OF FUTURE TECHNOLOGY 3 (Sci-Fi Documentary)

This timelapse of future technology, the 3rd year of the video series, goes on a journey exploring the human mind becoming digital. Brain chips turn memories and thoughts into data; could this data be sent out into space to live in the cosmos encoded into the magnetic fields between stars.

Other topics covered in this sci-fi documentary video include: bio-printing, asteroid habitats, terraforming Mars, the future of Teslabots, lucid dreaming, and the future of artificial intelligence and brain to computer interfaces (BCI — brain chips).

PATREON
The first and second volumes of ‘The Encyclopedia of the Future’ are now available on my Patreon.

Visit my Patreon here: / venturecity.

Created by: Jacob B
Narration by: Alexander Masters.

Addition footage: NASA’s Goddard Space Flight Center/CI Lab.

Brown dwarfs: The stars that ‘fail’

Brown dwarfs are curious celestial bodies that appear to straddle the mass divide between stars and planets. Often referred to as “failed stars,” brown dwarfs form in isolation from a collapsing cloud of gas and dust like a star.

However, while fully-fledged stars continue to gather material from the gas and dust cloud that births them, brown dwarfs are less successful at this mass harvesting. As a result, they don’t reach the masses of the smallest stars and can’t trigger the process that defines main sequence stars, like our sun.

Hubble’s ‘impossible’ planet explained? Gas giants may have formed fast in early universe

Dwarf galaxies like the SMC are often un-evolved when it comes to their chemistry because their history of star formation isn’t very extensive, so they haven’t had a chance to build up many heavy elements, such as carbon, nitrogen, oxygen, silicon or iron. NGC 346, for instance, contains about 10% the abundance of heavy elements that star-forming regions in our Milky Way galaxy have. This makes clusters such as NGC 346 great proxies for studying conditions akin to those found in the early universe.

NGC 346 is still forming lots of stars, and JWST found that many of the young ones, with ages of 20 to 30 million years, still possess planet-forming disks around them. Their existence confounds expectations.

“With Webb, we have a strong confirmation of what we saw with Hubble, and we must rethink how we create computer models for planet formation and early evolution in the young universe,” said Guido De Marchi of the European Space Research and Technology Centre (ESTEC) in the Netherlands, who led the research.

The Sublime

All 3D models created with Meshy AI
https://www.meshy.ai/?utm_source=youtube&utm_medium=fimcrux.

The sublime is an emotion described as equal parts awe and terror; a perfect description of our universe.

We created this short film concept showcasing a future vision of how humans might continue exploring that universe.

We used Meshy AI to generate all the 3D models in this film, like the ships, space probes and asteroids.

All the other VFX were created by us without the use of AI.

World first: Organic matter and water found on asteroid

Most of Earth’s meteorites also trace their origins to S-type asteroids, yet they contain minimal organic material. This scarcity has made analyzing their organic content a significant challenge. In contrast, the Hayabusa mission’s meticulously curated samples are free from terrestrial interference, enabling groundbreaking studies of organic compounds.

Among the particles returned by Hayabusa, one named “Amazon” has proven particularly revealing. Measuring just 30 micrometers wide, Amazon offers a rare opportunity to investigate both water and organic content. Its unique shape, reminiscent of the South American continent, underscores its distinctiveness.

Amazon’s mineral composition includes olivine, pyroxenes, albite, and traces of high-temperature carbonates. These minerals confirm its origin as an S-type asteroid, linking it directly to ordinary chondrites.