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Did ancient space weather influence how early humans lived?
In an exciting blend of archaeology and geophysics, researchers are uncovering how ancient cosmic events shaped human progress. Did spectacular auroras and invisible radiation 41,000 years ago push our ancestors to change their very lifestyles and survival strategies? Let’s explore the profound effects of space weather on early human existence.

Sandeep K S
Jul 20
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Meet Virgil, the galaxy that is rewriting black hole history
In visible light, it looks like a normal galaxy. In infrared, it reveals a monster. Meet Virgil, the galaxy that is rewriting black hole history.
Before JWST, astronomers believed galaxies grew first, nurturing small black holes that grew slowly over time.
Virgil breaks this rule. Its black hole is "Overmassive"—far larger than its host galaxy should be able to support. It's like finding a skyscraper engine inside a compact car.


JWST has found evidence of a thick atmosphere on the ultra-hot Super-Earth TOI-561 b
JWST has found evidence of a thick atmosphere on the ultra-hot Super-Earth TOI-561 b, challenging the idea that such close-in worlds are barren rocks.
TOI-561 b is an "Ultra-Short Period" planet, orbiting its star in less than 11 hours. It is tidally locked, meaning one side faces the star forever.


Westerlund 1 is the biggest star cluster in our galaxy.
Westerlund 1 is the biggest star cluster in our galaxy. New data reveals it acts as a colossal particle accelerator, blasting a hole through the Milky Way's disk.


A supernova from 10 billion years ago solved the mystery of the universe's expansion rate
A rare, magnified supernova from 10 billion years ago might finally solve the mystery of the universe's expansion rate.
We know the universe is expanding, but we don't agree on how fast. This disagreement is called the Hubble Tension.
Early Universe (CMB): Says ~67 km/s/Mpc.
Late Universe (Supernovae): Says ~73 km/s/Mpc.
SN 2025wny is a "Goldilocks" object. It's an independent test. By measuring the time delay between its lensed images, we can calculate the expansion rate d


Galaxies aren't always flat disks. Many are warped, bent by invisible forces.
Galaxies aren't always flat disks. Many are warped, bent by invisible forces. New research links these shapes to the satellite galaxies that surround them.
Using data from the Sloan Digital Sky Survey, researchers led by Prof. Woong-bae Zee examined hundreds of warped galaxies. They compared them to a "control group" of flat galaxies.
The goal: To see if the neighbors (satellite galaxies) had anything to do with the warping.
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