Tag Archive for 'Milky Way'

This Hubble image shows Terzan 1, a globular cluster located some 21,800 light-years away in the constellation of Scorpius. Image credit: NASA / ESA / Hubble / R. Cohen.

Hubble Captures Brilliant New Image of Globular Cluster Terzan 1

Oct 10, 2022 by Enrico de Lazaro

Terzan 1 is a globular cluster about 21,800 light-years from Earth in the constellation of Scorpius. This Hubble image shows Terzan 1, a globular cluster...

Shown here in purple, the Magellanic Corona stretches more than 100,000 light-years from the main mass of stars, gas, and dust that make up the Magellanic Clouds, intermingling with the hotter and more extensive corona that surrounds the Milky Way. Image credit: Leah Hustak, STScI.

Magellanic Corona: Astronomers Detect Protective Shield around Small and Large Magellanic Clouds

Oct 4, 2022 by News Staff

The Small and Large Magellanic Clouds — satellite galaxies of the Milky Way Galaxy — are surrounded by a diffuse halo of hot, supercharged...

This artist’s illustration indicates where the modeling of the ALMA data predicts the hot spot to be and its orbit around Sagittarius A*. Image credit: ESO / M. Kornmesser / M. Wielgus / Event Horizon Collaboration.

ALMA Spots Bubble of Hot Gas in Orbit around Milky Way’s Central Black Hole

Sep 22, 2022 by News Staff

Sagittarius A*, the 4.3-million-solar-mass black hole at the center of our Milky Way Galaxy, was observed with the Atacama Large Millimeter/submillimeter...

An artist’s impression of the fireball around a white dwarf. Image credit: ROSITA Collaboration / Annika Kreikenbohm.

eROSITA Detects X-rays from Nova in Fireball Phase

Sep 22, 2022 by News Staff

Novae are caused by runaway thermonuclear burning in the hydrogen-rich atmospheres of accreting white dwarfs, which leads to a rapid expansion of the atmosphere...

Crocker et al. reveal that the Fermi cocoon is actually due to emission from the Sagittarius dwarf spheroidal galaxy. Image credit: O. Macias.

Astronomers Detect Gamma Rays from Sagittarius Dwarf Spheroidal Galaxy

Sep 6, 2022 by Enrico de Lazaro

The significant gamma-ray emission is coming from a population of millisecond pulsars within the Sagittarius dwarf spheroidal galaxy, an elliptical loop-shaped...

This image, taken with the HAWK-I infrared instrument on ESO’s Very Large Telescope, shows the Sagittarius B1 region. Image credit: ESO / Nogueras-Lara et al.

Astronomers Detect Excess of Young Stars in Sagittarius B1

Aug 29, 2022 by Natali Anderson

Sagittarius B1, a region close to the center of our Milky Way Galaxy, hosts more than 100,000 solar masses of young stars. This image, taken with the...

(A) the Milky Way Galaxy with superimposed spiral arms and geological events: the arm and the Solar System rotate clockwise at different rates; the ‘+’ number denotes the number of times Earth has passed through that arm; (B) model of the Oort cloud showing cometary nuclei; (C) schematic reconstruction of early Earth impact process; (D) early crustal nuclei development. Image credit: NASA / JPL-Caltech / ESO / R. Hurt / Kirkland et al., doi: 10.1130/G50513.1.

Transits through Milky Way’s Spiral Arms Helped Form Early Earth’s Continental Crust, Study Says

Aug 24, 2022 by News Staff

New research led by Curtin University geologists suggests that regions of space with dense interstellar clouds may send more high-energy comets crashing...

On August 31, 2012, a long filament of solar material that had been hovering in the Sun’s atmosphere, the corona, erupted out into space at 4:36 p.m. EDT. The CME traveled at over 900 miles per second. It did not travel directly toward Earth, but did connect with Earth’s magnetic environment, or magnetosphere, with a glancing blow, causing aurora to appear on the night of September 3. Image credit: NASA’s Goddard Space Flight Center.

ESA’s Gaia Mission Sheds New Light on Past and Future of Our Sun

Aug 12, 2022 by News Staff

With an age of 4.57 billion years, the Sun is currently in its comfortable middle age, fusing hydrogen into helium and generally being rather stable; staid...

In this multiwavelength view, radio emission from SNR G106.3+2.7 is blue and green, while yellow, orange, and red reveal radio waves from a vast cloud of interstellar gas; at center, the pink region shows where protons boosted by the supernova’s shock wave strike the gas, emitting a tell-tale glow of gamma rays. Image credit: Jayanne English, University of Manitoba / NASA / Fermi / Fang et al. / Canadian Galactic Plane Survey / DRAO / FCRAO.

Supernova Remnants are Sources of Extreme PeVatron Particles: Study

Aug 10, 2022 by News Staff

SNR G106.3+2.7, a supernova remnant located about 2,600 light-years away in the constellation of Cepheus, is producing protons with energies 10 times greater...

A simulated star-forming region where massive stars destroy their parent cloud. Image credit: STARFORGE.

Star Formation is Self-Regulatory Process, New Research Suggests

Aug 8, 2022 by News Staff

Although star formation is one of the most fundamental processes of astrophysics, there is no widely accepted theory of star formation, despite decades...

This Hubble image shows the bulge metal-rich globular cluster NGC 6638. Image credit: NASA / ESA / Hubble / R. Cohen.

Hubble Spots Young Globular Cluster in Milky Way Galaxy’s Bulge

Aug 1, 2022 by Enrico de Lazaro

The NASA/ESA Hubble Space Telescope has taken a very detailed image of the bulge globular cluster NGC 6638. This Hubble image shows the bulge metal-rich...

Images of WISE 1810 from the UKIDSS Galactic Plane Survey (left) and NOT ALFOSC (right). The object is indicated by a red arrow. North is up and east left. Each image is about 80 arcsec across. Image credit: Lodieu et al., doi: 10.1051/0004-6361/202243516.

Astronomers Find Ancient Brown Dwarf in Solar Neighborhood

Jul 22, 2022 by Natali Anderson

WISE 1810055-1010023 (WISE 1810 for short), a metal-poor brown dwarf located 8.9 parsecs (29 light-years) away, is nearly 10 billion years old. Images...

The view of the Galactic center observed with the NIRC2 instrument on the Keck II telescope at the W.M. Keck Observatory. This image is high-pass filtered and shows the position of several S stars close to Sgr A*, which is indicated by a black cross. The star in the white dashed circle shows a magnitude of 16.3 mag, while the star in the blue circle is 17 mag faint. Here north is up and east is to the left. Image credit: Peissker et al., doi: 10.3847/1538-4357/ac752f.

Fast-Moving Star Orbits Milky Way’s Central Black Hole in Just Four Years

Jul 6, 2022 by Natali Anderson

The newly-found star, named S4716, reaches a speed of 8,000 km/sec and comes as close as 98 astronomical units (AU) to Sagittarius A*, a supermassive black...

Sagittarius B2 is a giant molecular cloud of gas and dust that is located about 390 light-years from the center of the Milky Way Galaxy. Sagittarius B2 is the bright orange-red region to the middle left of the image, which is centered on the Galactic center. Image credit: ESO / APEX / MSX / IPAC / NASA.

ALMA Detects Interstellar Propanol and Its Isomer in Milky Way’s Center

Jul 5, 2022 by Natali Anderson

Astronomers using the Atacama Large Millimeter/submillimeter Array (ALMA) have detected two complex organic molecules — isopropanol (i-C3H7OH) and...

This Hubble image shows NGC 6569, a globular cluster located in the constellation of Sagittarius. The color image was made from separate exposures taken in the visible and infrared regions of the spectrum with Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Three filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / R. Cohen.

Hubble Sees Sparkling Globular Cluster in Milky Way’s Bulge

Jun 27, 2022 by Enrico de Lazaro

The NASA/ESA Hubble Space Telescope has produced a spectacularly detailed image of the Galactic bulge globular cluster NGC 6569. This Hubble image shows...

A schematic view of the history of the accretion disk and the flyby object: the three plots starting from the bottom left are snapshots from the numerical simulation, capturing the system right at the flyby event, 4,000 years after, and 8,000 years after, respectively; the top right image is from the ALMA observations, showing the disk with spirals and the two objects around it, corresponding to the system at 12,000 years after the flyby event. Image credit: Lu et al., doi: 10.1038/s41550-022-01681-4.

ALMA Images Spiral Protostellar Disk near Milky Way’s Center

Jun 21, 2022 by News Staff

Using the Atacama Large Millimeter/submillimeter Array (ALMA), astronomers have discovered a massive accretion disk with two spiral arms around a 32-solar-mass...

The interstellar dust map made with Gaia’s data release 3. Image credit: ESA / Gaia / DPAC.

ESA’s Gaia Mission Releases Its Third Full Dataset

Jun 14, 2022 by News Staff

Gaia’s data release 3 (DR3) contains new and improved details for almost 2 billion stars in our Milky Way Galaxy as well as for a subset of solar system...

The star-filled sky in this Hubble photo lies in the direction of the Galactic center. The light from stars is monitored to see if any change in their apparent brightness is caused by a foreground object drifting in front of them. The warping of space by the interloper would momentarily brighten the appearance of a background star, an effect called gravitational lensing. One such event, OB110462, is shown in the four close-up frames at the bottom. The arrow points to a star that momentarily brightened, as first captured by Hubble in August 2011. This was caused by a foreground black hole drifting in front of the star, along our line of sight. The star brightened and then subsequently faded back to its normal brightness as the black hole passed by. Because a black hole doesn’t emit or reflect light, it cannot be directly observed. But its unique thumbprint on the fabric of space can be measured through these so-called microlensing events. Image credit: NASA / ESA / Hubble / K. Sahu, STScI / J. DePasquale, STScI.

Hubble Detects Free-Floating Compact Object 5,000 Light-Years Away

Jun 13, 2022 by Enrico de Lazaro

Astronomers have for the first time discovered what may be an isolated stellar-mass black hole using the astrometric microlensing technique. They estimate...

This Hubble image shows the globular cluster Terzan 9, a relic of a generation of long-lived stars that formed in the early Galaxy. The color image was made from separate exposures taken in the visible and infrared regions of the spectrum with Hubble’s Advanced Camera for Surveys (ACS) and Wide Field Camera 3 (WFC3). Three filters were used to sample various wavelengths. The color results from assigning different hues to each monochromatic image associated with an individual filter. Image credit: NASA / ESA / Hubble / R. Cohen.

Hubble Spots Ancient Star Cluster near Milky Way’s Center

Jun 13, 2022 by Enrico de Lazaro

This new image from the NASA/ESA Hubble Space Telescope is one of the best ever views of Terzan 9, one of the most central globular clusters in our Milky...

This image of the Carina Nebula reveals the dynamic cloud of interstellar matter and thinly spread gas and dust as never before; the massive stars in the interior of this cosmic bubble emit intense radiation that causes the surrounding gas to glow; by contrast, other regions of the nebula contain dark pillars of dust cloaking newborn stars. Image credit: ESO / J. Emerson / M. Irwin / J. Lewis.

Astronomers Discover 116,027 New Variable Stars

Jun 1, 2022 by News Staff

Using machine learning techniques and data from the All-Sky Automated Survey for Supernovae (ASAS-SN) and several other surveys, astronomers have identified...

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