Face-on View of Galaxy NGC 4303 Reveals its Arms are Filled with Active Star Formation

NGC 4303, a galaxy rich in star formation. It lies about 55 million light-years away in the Virgo Cluster. This view shows both visible-light and millimeter-wavelength views of the galaxy. Credit: ESO/ALMA (ESO/NAOJ/NRAO)/PHANGS

Galaxies fill a lot of roles in the universe. The most obvious one is star formation factories. Without that activity, the cosmos would be a very different place. The European Southern Observatory and the Atacama Large Millimeter Array recently zeroed in on the galaxy NGC 4303. Their goal: to take a multi-wavelength view of its star formation activity.

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A.I. Finds a New Way to Build Multiple-Star Systems

A false-color image of NGC 6334 from multiple telescopes. The area is believed to be a hotspot of furious star birth. Credit: S. Willis (CfA+ISU); ESA/Herschel; NASA/JPL-Caltech/ Spitzer; CTIO/NOAO/AURA/NSF

Over over 50% of high mass stars reside in multiple star systems. But due to their complex orbital interactions, physicists have a difficult time understanding just how stable and long-lived these systems are. Recently a team of astronomers applied machine learning techniques to simulations of multiple star systems and found a new way that stars in such systems can arrange themselves.

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Molecular Clouds Have Long Lives By Constantly Reassembling Themselves

This is a two-panel mosaic of part of the Taurus Giant Molecular Cloud, the nearest active star-forming region to Earth. The darkest regions are where stars are being born. Inside these vast clouds, complex chemicals are also forming. Image Credit: Adam Block /Steward Observatory/University of Arizona

Astronomers have recently discovered that giant clouds of molecular hydrogen, the birthplace of stars, can live for tens of millions of years despite the facts that individual molecules are constantly getting destroyed and reassembled. This new research helps place a crucial piece of understanding in our overall picture of how stars are born.

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Astronomers Spot an Orphaned Protostar

The HH 24 Complex (image credit: Reipurth et al.)

Astronomers have performed an impressive suite of observations at multiple wavelengths of the same system, dubbed the HH 24 complex. This complex hosts stars in the process of being born and the impacts of their violent interactions with each other, including the ejection of one of their siblings.

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It’s Feeding Time For This Baby Star in Orion

This new image of the Orion Nebula produced using previously released data from three telescopes shows two enormous caverns carved out by unseen giant stars that can release up to a million times more light than our Sun. All that radiation breaks apart dust grains there, helping to create the pair of cavities. Much of the remaining dust is swept away when the stars produce wind or when they die explosive deaths as supernovae. Image Credit: ESA/NASA/JPL-Caltech

Young protostars are wrapped in what could be called a womb of gas and dust. The gas and dust nearest to them form a circumstellar disk as the stars grow. The disk is a reservoir of material that the star accretes as it grows.

But these stars don’t feed in a predictable rhythm. Sometimes, they experience feeding frenzies, periods of time they accrete lots of material from the disk at once. When that happens, they flare in bright bursts, “burping” as they absorb more material.

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Baby Gas Giants Cast Shadows on Their Siblings

A computer-generated image depicting a dark protostellar disk seen edge-on at 90 degrees to jets (orange) emanating from the poles of a young star. Such disks are thought to be the precursors of planetary systems, with planets forming as the dust coalesces. RIKEN researchers may have spotted embryos of gas giant planets in one protostellar disk. Credit: Mark Garlick/Science Photo Library

A team of astronomers has caught glimpses of gas giants forming around a very young star.

The nascent giants are having a chilling effect on their potential siblings.

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Hubble Sees a Dense Cloud of Gas and Dust That’s About to Become a Star

A small, dense cloud of gas and dust called CB 130-3 blots out the center of this image from the NASA/ESA Hubble Space Telescope.
A small, dense cloud of gas and dust called CB 130-3 blots out the centre of this HST image. Courtesy NASA/ESA/STScI

The process of star birth begins in a shroud of gas and dust. Hubble Space Telescope (HST) excels in showing detailed views of these stellar crêches because there’s still a lot to learn about them. Its latest image shows an object called a “dense core”, where a stellar embryo could already exist.

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The Latest JWST Image Shows a Star in the Earliest Stage of Formation

The NASA/ESA/CSA James Webb Space Telescope has revealed the once-hidden features of the protostar within the dark cloud L1527 with its Near Infrared Camera (NIRCam), providing insight into the formation of a new star. These blazing clouds within the Taurus star-forming region are only visible in infrared light, making it an ideal target for Webb. Image Credit: NASA, ESA, CSA, and STScI, J. DePasquale (STScI), CC BY-SA 3.0 IGO

What’s the most exciting thing about the James Webb Space Telescope? The stunning images? The completion of its torturous path from concept to launch?

Or is it because it provides such compelling visual evidence of objects and processes long theorized about but difficult to observe?

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Too Many Supernovae Can Slow Star Formation in a Galaxy

star formation regions in M33 are disrupted by cosmic-ray driven winds
Artist's illustration of cosmic ray-driven winds (blue and green) superimposed on a visible-light image of the Triangulum galaxy M33 (red and white) observed with VLT Survey Telescope at ESO’s Paranal Observatory in Chile. Credit: Institute for Research in Fundamental Sciences- IPM & European Southern Observatory (ESO)

Interstellar winds are powerful agents of change. For one thing, they can interrupt or shut down the process of star birth completely. That’s what a team of astronomers using the Karl Jansky Very Large Array in New Mexico found when they studied the galaxy M33. They also learned that speedy cosmic rays play a huge role in pushing those winds across interstellar space.

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Another Version of the Pillars of Creation from Webb

pillars of creation
The NASA/ESA/CSA James Webb Space Telescope’s mid-infrared view of the Pillars of Creation. Credit: NASA, ESA, CSA, STScI, J. DePasquale (STScI), A. Pagan (STScI)

The hits just keep on streaming back to Earth from James Webb Space Telescope (JWST). This time, arriving to help celebrate Hallowe’en, data from the MIRI mid-infrared instrument onboard JWST shows another view of the Pillars of Creation. Thousands of stars are embedded in those pillars, but many are “invisible” to MIRI.

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