Category Astronomy/Space

Metal-poor Stars are more Life-friendly

A star’s chemical composition strongly influences the ultraviolet radiation it emits into space and thus the conditions for the emergence of life in its neighborhood.

Stars that contain comparatively large amounts of heavy elements provide less favourable conditions for the emergence of complex life than metal-poor stars, as scientists from the Max Planck Institutes for Solar System Research and for Chemistry as well as from the University of Göttingen have now found. The team showed how the metallicity of a star is connected to the ability of its planets to surround themselves with a protective ozone layer. Crucial to this is the intensity of the ultraviolet light that the star emits into space, in different wavelength ranges...

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Could this Copycat Black Hole be a New type of Star?

Could this copycat black hole be a new type of star?
Credit: Pierre Heidmann / Johns Hopkins University

It looks like a black hole and bends light like a black hole, but it could actually be a new type of star.

Though the mysterious object is a hypothetical mathematical construction, new simulations by Johns Hopkins researchers suggest there could be other celestial bodies in space hiding from even the best telescopes on Earth. The findings are set to publish in Physical Review D.

“We were very surprised,” said Pierre Heidmann, a Johns Hopkins University physicist who led the study. “The object looks identical to a black hole, but there’s light coming out from its dark spot.”

The detection of gravitational waves in 2015 rocked the world of astrophysics because it confirmed the existence of black holes...

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From Platypus to Parsecs and MilliCrab: Why do Astronomers use such Weird Units?

A bright, multi-coloured supernova remnant with dusty, wispy filaments and something resembling a tornado (the pulsar wind nebula) in the centre.
Image of the Crab Nebula where red is radio from the Very Large Array, yellow is infra-red from the Spitzer Space Telescope, green is visible from the Hubble Space Telescope, and blue and purple are X-ray from the XMM-Newton and Chandra X-ray Observatories respectively. NASA, ESA, G. Dubner (IAFE, CONICET-University of Buenos Aires) et al.; A. Loll et al.; T. Temim et al.; F. Seward et al.; VLA/NRAO/AUI/NSF; Chandra/CXC; Spitzer/JPL-Caltech; XMM-Newton/ESA; and Hubble/STScI

You may have heard about an asteroid set to fly near Earth that is the size of 18 platypus, or maybe the one that’s the size of 33 armadillos, or even one the size of 22 tuna fish.

These outlandish comparisons are the invention of Jerusalem Post journalist Aaron Reich (who bills himself as “creator of the giraffe...

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PSR J0901-4046 is the Most Magnetized Radio Pulsar known, study finds

PSR J0901-4046 is the most magnetized radio pulsar known, study finds
The background for both images shows the 1.28 GHz radio continuum emission from the nebula surrounding the high-mass X-ray binary system Vela X-1, and its newly-discovered radio bow shock (van den Eijnden et al. 2022). On the left and right we can see the MeerKAT images of the pulsar PSR J0901-4046 before and during a pulse, respectively. Credit: Ian Heywood.

Astronomers have investigated an ultraslow radio pulsar known as PSR J0901-4046, finding that it has an extremely high magnetic field—at a level of 30 quadrillion Gauss. The discovery, published April 7 in Physical Review D, makes PSR J0901-4046 the most magnetized radio pulsar known to date.

Extraterrestrial sources of radiation with a regular periodicity, known as pulsars, are usually detected in the form of short bursts of...

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