Triggered Star Birth in the Nessie Nebula

A three-color composite of a portion of the Nessie Nebula that shows infrared observations from two Spitzer instruments. The bright red circular region in the center is the site of triggered star formation. Courtesy NASA/JPL.
A three-color composite of a portion of the Nessie Nebula that shows infrared observations from two Spitzer instruments. The bright red circular region in the lower center is the site of triggered star formation. Courtesy NASA/JPL.

Star formation is one of the oldest processes in the Universe. In the Milky Way and most other galaxies, it unfolds in cold, dark creches of gas and dust. Astronomers study sites of star formation to understand the process. Even though they know much about it, some aspects remain mysterious. That’s particularly true for the “Nessie Nebula” in the constellation Vulpecula. An international team led by astronomer James Jackson studies the nebula and its embedded star-birth regions. They found that it experienced a domino effect called “triggered star formation.”

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It Took Five Years and A Million Images to Make this Atlas of Stellar Nurseries

This image shows the HH 909 A object in the Chamaeleon constellation. New stars are born in the colourful clouds of gas and dust seen here. The infrared observations underlying this image reveal new details in the star-forming regions that are usually obscured by the clouds of dust. Image Credit: ESO/Meingast et al.

Star formation is an intricate process governed by a swarm of variables, and it all happens behind a thick veil of dust. Astrophysicists understand it to a certain degree. But this is nature, and nature doesn’t give up its intimate secrets without a concentrated effort.

To learn more about the star formation process, astronomers imaged five star-forming regions in the southern hemisphere with the ESO’s VISTA telescope. It took five years and over one million images, and the result is the VISIONS survey.

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Newborn Star Surrounded By Planet-Forming Disks at Different Angles

This artist's concept is based on Hubble Space Telescope images of gas-and-dust disks around the newborn star TW Hydrae. HST images show shadows sweeping across the disks encircling the system. These shadows are probably from slightly inclined inner disks that block starlight from reaching the outer disk. The disks are slightly inclined to each other due to the gravitational pull of unseen planets warping the disk structure. Credits ARTWORK: NASA, AURA/STScI for ESA, Leah Hustak (STScI)
This artist's concept is based on Hubble Space Telescope images of gas-and-dust disks around the newborn star TW Hydrae. HST images show shadows sweeping across the disks encircling the system. These shadows are probably from slightly inclined inner disks that block starlight from reaching the outer disk. The disks are slightly inclined to each other due to the gravitational pull of unseen planets warping the disk structure. Credits ARTWORK: NASA, AURA/STScI for ESA, Leah Hustak (STScI)

One of the great questions about our solar system is: what was it like as it formed? We know that a protosolar nebula birthed the Sun and planets. And, we know planets in our solar system have slightly different orbital inclinations, probably due to some interesting dynamics in the birth crèche. Why is that? The answer may be in a slightly weird-looking protoplanetary disk circling the newborn star TW Hydrae.

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Mother of Dragons: Astronomers Peer Inside the “Dragon Cloud”

The inner core of the "dragon cloud" complex. Image credit: Barnes et al.
The inner core of the "dragon cloud" complex. Image credit: Barnes et al.

How did the most massive stars form? Astronomers have debated their origins for decades. One of the biggest problems facing these theories is the lack of observations. Massive stars are relatively rare, and so it’s hard to catch them in the act of formation. But new observations of the so-called Dragon cloud may hold the clue to answering this mystery.

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When Clouds Collide, Destruction and Creation Go Hand-in-Hand

New stars seen by the Hubble Space Telescope in the Orion Nebula. ESA/Hubble & NASA, J. Bally; Acknowledgment: M. H. Özsaraç.

All stars are born from the collapse of clouds of dust and gas. But triggering star formation is a tricky process, because these gas clouds can just hang out doing nothing for billions of years. A pair of researchers have found a precise recipe for getting gas clouds to trigger star formation. It involves a lot of collision.

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Astronomers Find 1,179 Previously Unknown Star Clusters in Our Corner of the Milky Way

Some of the most exciting things that happen in a telescope’s lifetime are its data releases. Gaia, which has been operating since 2013, recently released its third major dataset, and astronomers that weren’t intimately involved in the operation and planning for the project have had some time to pull over. Their studies are starting to pop up in journals everywhere. For example, a new one from a research team, mainly from Guangzhou University, catalogs over 1100 new star clusters, significantly increasing the overall total of these critical components in the structure of the Milky Way.

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Water’s Epic Journey to Earth Began Before the Sun Formed

This artist’s impression shows the planet-forming disc around the star V883 Orionis. New research shows how water starts its journey in the gas cloud that forms the star, and eventually ends its journey on Earth. Image Credit: ESO/L. Calçada

The origins of Earth’s water is a complicated mystery that scientists have been untangling for decades. Life is impossible without water, so the origin of Earth’s life-giving water is a foundational question. As the power of our telescopes grows, researchers have made meaningful headway on the question.

Previous research uncovered links between Earth’s water and the Solar System’s comets and icy planetesimals. But newer research follows the chain back even further in time to when the Sun itself had yet to form.

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Speedrunning Star Formation in the Cygnus X Region

Cygnus X is a massive star formation region about 4600 light-years away. New research shows star formation occurring very rapidly. Image Credit: By NASA - http://www.nasa.gov/mission_pages/spitzer/multimedia/pia15253.html, Public Domain, https://commons.wikimedia.org/w/index.php?curid=19475200

Stars are born in molecular clouds, massive clouds of hydrogen that can contain millions of stellar masses of material. But how do molecular clouds form? There are different theories and models of that process, but the cloud formation is difficult to observe.

A new study is making some headway, and showing how the process occurs more rapidly than thought.

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Galaxies Aren’t Just Stars. They’re Intricate Networks of Gas and Dust

This image taken by the NASA/ESA/CSA James Webb Space Telescope shows the spiral galaxy NGC 1433. Image Credit: NASA, ESA, CSA, and J. Lee (NOIRLab), A. Pagan (STScI)

Astronomers have studied the star formation process for decades. As we get more and more capable telescopes, the intricate details of one of nature’s most fascinating processes become clearer. The earliest stages of star formation happen inside a dense veil of gas and dust that stymies our observations.

But the James Webb Space Telescope sees right through the veil in its images of nearby galaxies.

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Hubble’s New View of the Tarantula Nebula

A snapshot of the Tarantula Nebula (also known as 30 Doradus) is the most recent Picture of the Week from the NASA/ESA Hubble Space Telescope. Image Credit: ESA/Hubble & NASA, C. Murray, E. Sabbi; Acknowledgment: Y. -H. Chu

The Tarantula Nebula, also called 30 Doradus, is the brightest star-forming region in our part of the galaxy. It’s in the Large Magellanic Cloud (LMC) and contains the most massive and hottest stars we know of. The Tarantula Nebula has been a repeat target for the Hubble since the telescope’s early years.

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