Category Astronomy/Space

Our Galaxy’s Black Hole Not as Sleepy as thought

The first ever image of Sagittarius A*, the supermassive black hole that sit at the centre of the Milky Way galaxy
The first ever image of Sagittarius A*, the supermassive black hole that sit at the centre of the Milky Way galaxy.

The supermassive black hole lurking at the center of our Milky Way galaxy is not as dormant as had been thought, a new study shows.

The slumbering giant woke up around 200 years ago to gobble up some nearby cosmic objects before going back to sleep, according to the study published in the journal Nature on Wednesday.

NASA’s IXPE space observatory spotted an Xray echo of this powerful resurgence of activity, the researchers said.

The supermassive black hole Sagittarius A—abbreviated to Sgr A—is four million times more massive than the Sun. It sits 27,000 light years from Earth at the center of the Milky Way’s spiral.

Last year astronomers revealed the first...

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Astronomers explore the Properties of Ultra-Diffuse Galaxy UGC 9050-Dw1

Study explores the properties of ultra-diffuse galaxy UGC 9050-Dw1
HST ACS/WFC F555W/F814W composite color image of UGC 9050-Dw1, which consists of very diffuse stellar light and an amorphous blue central clump of a relatively higher surface brightness. The inset at the lower left depicts a high contrast zoom-in of the central region of the UDG. Credit: Fielder et al, 2023

Using the Hubble Space Telescope (HST) and Jansky Very Large Array (VLA), astronomers have investigated an ultra-diffuse galaxy known as UGC 9050-Dw1. Results of the study, published June 9 on the pre-print server arXiv, yield important insights into the properties of this galaxy.

Ultra-diffuse galaxies (UDGs) are extremely-low-density galaxies. The largest UDGs have sizes similar to the Milky Way, but have only about 1% as many stars as our home galaxy...

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Exoplanet may reveal Secrets about the Edge of Habitability

Carl Sagan Institute/R. Payne
Artist impression showing the exoplanet LP 890-9c’s potential evolution from a hot Earth to a desiccated Venus.

How close can a rocky planet be to a star, and still sustain water and life? A recently discovered exoplanet may be key to solving that Edge of Habitabilitymystery.

“Super-Earth” LP 890-9c (also named SPECULOOS-2c) is providing important insights about conditions at the inner edge of a star’s habitable zone and why Earth and Venus developed so differently, according to new research led by Lisa Kaltenegger, associate professor of astronomy at Cornell University.

Her team found LP 890-9c, which orbits close to the inner edge of its solar system’s habitable zone, would look vastly different depending on whether it still had warm oceans, a ste...

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Discovery of a Brown Dwarf Hotter than the Sun

Discovery of a space object hotter than the sun
Phased radial-velocity curves of WD 0032−317. a, trailed UVES spectrum for the H𝛼 line of WD 0032−317 (blue represents lower fluxes, and yellow represents higher fluxes), folded over the orbital period (𝑃 = 8340.9090 s). The primary absorption is clearly seen in blue. The emission from the companion (in yellow) appears in anti-phase with the primary, and is visible only from the irradiated day side, between orbital phases ∼ 0.2–0.8. Its “inverted” shape, evident especially near quadrature, is the result of non-local thermodynamic equilibrium (NLTE) effects [40]. b, radial velocity curves (top panel) of the white dwarf (blue circles) and the irradiated companion (red diamonds), folded over the orbital period (𝑃 = 8340.9090 s)...
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