JWST imaging of the RPS galaxy C26 in SPT2349–56. (a) Red-green-blue image of the protocluster core (blue: NIRCam/F200W; green: NIRCam/F444W; red: MIRI/F1000W). The RPS galaxy C26 is marked by the red rectangle. The cross labels the kinematic center of the protocluster. (b–d) Zoomed images of C26 in F200W, F444W, and F1000W, respectively. credit: DOI: https://doi.org/10.48550/arXiv.2606.18229
Astronomers have spotted many “red and dead” galaxies in the early universe. These are massive systems that stopped forming stars surprisingly early in cosmic history. Now, they may have found evidence of one in the act of becoming dead: a massive galaxy being stripped of its starforming gas just 1.4 billion years after the Big Bang...
Astronomers have revealed new details about the makeup and age of a visiting comet that was born around a distant star. They conclude that the composition of 3I/Atlas is strikingly different from any object found in our solar system.
A trio of recently published studies shed light on the origins of this exotic comet. 3I/Atlas appears to have been born in a cold environment, possibly around 12 billion years ago.
The comet is an interstellar object (ISO), meaning an asteroid or comet that originated outside the solar system. It is the third such object found, after 1I/ʻOumuamua and 2I/Borisov. It was discovered almost exactly one year ago, traveling inbound on a trajectory that has taken it through the inner solar system and out the other side.
This animation illustrates the concept of gravitational microlensing. When one star in the sky appears to pass nearly in front of another, the light rays of the background source star become bent due to the warped space-time around the foreground star. This star acts like a virtual magnifying glass, amplifying the brightness of the background source star. If the nearer star harbors a planetary system, then those planets can also act as lenses, each one producing a short deviation in the brightness of the source. When astronomers find planets this way, they can measure their mass and orbital distance from their host star. Credit: NASA’s Goddard Space Flight Center/CI Lab
For the first time, NASA’s TESS (Transiting Exoplanet Survey Satellite) mission has identified a planet orbiting a ...
Artist’s conception of the view from the surface of the habitable-zone super-Earth exoplanet GJ 3378b. The planet has a minimum mass just over twice that of Earth and orbits its star at a distance that causes it to receive almost the same amount of starlight as Earth does. The planet joins a growing population of potential hosts for life in the nearby universe. Image credit: Nikolai Berman/UC Irvine.
Using the Hobby-Eberly Telescope at McDonald Observatory, astronomers have taken a closer look at a nearby exoplanet and discovered it may be more Earth-like than previously thought. The planet, known as GJ 3378b, orbits a small, cool star called a red dwarf...
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