
Betelgeuse has a close-orbiting companion that disturbs the red supergiant into an egg-like shape. New observations show how the two stars interact and how this could help explain the varying brightness of Betelgeuse.

Betelgeuse has a close-orbiting companion that disturbs the red supergiant into an egg-like shape. New observations show how the two stars interact and how this could help explain the varying brightness of Betelgeuse.

Perhaps the biggest mystery we face is life on Earth started. One hypothesis says that comets, which are known to carry important chemicals in abiogenesis, delivered these compounds to Earth, leading to the appearance of life. But new research concludes that that is highly unlikely.

Finding an Earth-like world beyond the solar system is the Holy Grail of exoplanet research, and the field has experienced incredible technological advancements in searching for and identifying exoplanets since the first exoplanet was discovered in 1995. This includes both ground- and space-based telescopes, specifically the powerful James Webb Space Telescope. However, directly imaging exoplanets remains elusive, primarily due to the enormous technological challenge of imaging a point of light so far away.
![A view of the Taurus Molecular Cloud from the Herschel Space Observatory. The bright region at the lower left is the pre-stellar core Lynds 1544. Astronomers looked at it using radio astronomy techniques to understand what's happening in a prestellar core. [ESA/Herschel/SPIRE]](https://www.universetoday.com/article_images/Taurus_molecular_cloud_20261028_002429.jpg)
In 1985, the physicist Heinz R. Pagels wrote, "Stars are like animals in the wild. We may see the youung, but never the actual birth, which is a veiled and secret event." In the decades since then, astronomers have drawn closer and closer to figuring out what actually goes in the veiled stellar nurseries throughout the Universe. The tale of starbirth we know today invokes collapse of clouds of gas and dust into prestellar cores, but it still has many unknowns, such as the role of magnetic fields in the clouds where stars are born.

When a star like our Sun reaches its end, it becomes a kind of zombie star called a white dwarf. These bodies have left fusion behind and will radiate only remnant heat for a long, long time. Before they become white dwarfs, they expand, engulf, and destroy any nearby planets. Astronomers have spotted a debris disk around a white dwarf, made from the dust of destroyed planets. Observations show that two new resurrected planets have formed in this disk, creating dead planets orbiting a dead star.

Dense stellar environments were common in the early Universe. These environments fostered more numerous stellar collisions, and some of those would've been mergers that formed very massive stars. Those stars would've exploded as supernovae, becoming massive black holes, the potential seeds for today's supermassive black holes.

The Earth’s magnetic field is responsible for shielding us from harmful space weather, including solar radiation from the Sun but also cosmic rays originating from outside our solar system. Cosmic rays can include deep space supernovas, so the magnetic field takes the majority of the brunt from solar radiation. Without our magnetic field, the solar wind would slowly strip away our atmosphere, making life on our small, blue world impossible to exist. But where is the magnetic field doing the heaviest lifting regarding how it filters out incoming space radiation?