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Even Stars Can Get the Hiccups: Exploring Cosmic Anomalies and Their Causes

The concept of “stellar hiccups” reveals a fascinating phase in the lives of massive stars, where rapid core expansions and contractions can precede supernova explosions. This newly observed phenomenon, known as “pulsational pair-instability,” enhances our understanding of stellar evolution and the cosmic processes that shape the universe.

Summary

  • Stellar hiccups are rare, observable pre-supernova phases in stars with masses ranging between 60-150 times that of the Sun.
  • The phenomenon is caused by pulsational pair-instability (PPI), where the stellar core rapidly contracts and expands under extreme temperatures.
  • Massive stars nearing the end of their lifespans eject shells of material during these “hiccup” events, creating bursts of energy visible from Earth.
  • These “hiccups” help scientists understand how massive stars shed mass and transition to the supernova stage.
  • The discovery of SN2020acct in the NGC2981 galaxy provided the first-ever observation of this phenomenon.
  • The core mechanism involves material ejection due to unstable thermonuclear reactions in massive stars, followed by collisions between ejected shells of gas.
  • This process was theorized for decades but remained unobserved due to its rarity and faintness.
  • Observing hiccups can aid in predicting supernova occurrences and understanding element distribution in the universe.
  • The remnants of these massive explosions create neutron stars or black holes, depending on the progenitor’s mass.
  • The study also sheds light on the role of supernovae in spreading heavy elements critical for forming planets and life.
Even Stars Can Get the Hiccups Exploring Cosmic Anomalies and Their Causes
This new picture comes from the VLT Survey Telescope (VST) at ESO’s Paranal Observatory. It shows the impressive super star cluster called Westerlund 1. This bright cluster is about 16,000 light-years from Earth. It is located in the southern constellation of Ara, also known as The Altar. The cluster contains hundreds of very large and bright stars. These stars are only a few million years old, which is very young for stars.
However, we can’t see this cluster clearly because gas and dust block most of its visible light from reaching Earth. Recently, astronomers found something unexpected while studying images of Westerlund 1. These images are from a new survey of the southern skies. They discovered clouds of glowing hydrogen gas around one of the stars in the cluster. This star is called W26. W26 is a red supergiant and might be the biggest star known.
Glowing clouds around massive stars are very rare. They are even rarer around a red supergiant. In fact, this is the first ionised nebula found around such a star. An ionised nebula is a glowing cloud of gas that usually surrounds stars. W26 is too cool to make the gas glow by itself. The astronomers think that the gas glows due to radiation from somewhere else. The source might be hot blue stars elsewhere in the cluster or a much hotter companion star to W26.
W26 will eventually explode as a supernova. A supernova is a powerful explosion that happens when a star dies. The nebula around W26 is similar to the one that surrounded SN1987A. SN1987A is the remains of a star that became a supernova in 1987. It was the closest supernova to Earth observed since 1604. This gave astronomers a chance to learn more about these explosions.
By studying objects like the new nebula around W26, astronomers can understand how massive stars lose mass before exploding. Understanding these processes helps scientists learn more about the life and death of stars.
This picture is part of a detailed survey of a large part of the Milky Way. The survey is called VPHAS+ and uses the VST’s power to find new objects like young stars and planetary nebulae. A planetary nebula is a glowing shell of gas and dust around an old star. A recent picture of the Prawn Nebula also came from this survey.

Cosmic Context of Stellar Hiccups

Stars are colossal nuclear furnaces, responsible for producing and dispersing heavy elements essential for the formation of planets and life. Among these stars, massive ones often live dramatically short lives, culminating in supernova explosions that distribute their materials into space. However, before the grand finale of a supernova, some stars exhibit unique “hiccups” due to a rare process called pulsational pair-instability (PPI).

What Are Stellar Hiccups?

PPI causes the cores of massive stars to rapidly expand and contract, ejecting shells of material in the process. These hiccups are short-lived, occurring just years, or even days, before a supernova.

In December 2020, astronomers discovered one such hiccup in the galaxy NGC2981, marking the first observation of this fascinating event.

The Science Behind Pulsational Pair-Instability

The term pulsational pair-instability refers to a rare phenomenon where conditions in a star’s core destabilize due to:

  1. Extreme Heat: Stars exceeding 60 times the Sun’s mass reach temperatures high enough to produce electron-positron pairs, reducing radiation pressure.
  2. Core Collapse: Reduced pressure causes the core to collapse under gravity.
  3. Rapid Expansion: Nuclear reactions reignite, causing the core to expand and eject material in violent bursts.

How PPI Affects Stellar Evolution

Each hiccup expels part of the star’s mass, lowering its overall size and altering its eventual fate. Over time, the remaining core becomes unstable enough to collapse into either a neutron star or a black hole.

Observed Phenomenon: The Case of SN2020acct

The Fred Lawrence Whipple Observatory detected SN2020acct, initially classified as a supernova. However, astronomers later discovered that the light emitted was not a supernova but the result of material shells colliding near the star.

Observation Timeline Key Events
December 2020 SN2020acct discovered in NGC2981
February 2021 Unusual light reappeared in the same region
Detailed Analysis Confirmed “hiccups” as the cause

Why Are Stellar Hiccups Important?

Stellar hiccups provide insights into the processes that precede supernovae, which are critical for understanding:

  • Elemental Formation: The heavy elements necessary for life are created during these events.
  • Massive Star Evolution: PPI events help explain how massive stars lose mass before exploding.
  • Supernova Prediction: Observing hiccups can refine supernova timelines, aiding astronomical studies.
Even Stars Can Get the Hiccups Exploring Cosmic Anomalies and Their Causes
The 48-inch telescope at the Fred Lawrence Whipple Observatory captured this visible-light image of the Pinwheel galaxy (Messier 101) in June 2023. The image shows the location of supernova 2023ixf, which is highlighted with a circle. The observatory is on Mount Hopkins in Arizona. The Center for Astrophysics | Harvard & Smithsonian operates the observatory. Hiramatsu and others reported this in 2023. Sebastian Gomez from the Space Telescope Science Institute (STScI) also contributed.

Supernovae: The Aftermath of Stellar Hiccups

Supernovae are categorized into two primary types:

Supernova Type Key Features
Type I Occurs in binary star systems; involves the accumulation of matter on a white dwarf.
Type II Marks the death of a massive star; involves core collapse and violent expulsion of outer layers.

Facts About Stellar Hiccups

  • Stellar hiccups are believed to occur in stars 60-150 times the mass of the Sun.
  • The phenomenon was only theorized until its first observation in 2020.
  • Hiccups can lead to repetitive light bursts from stars before they die.
  • The Pinwheel Galaxy (Messier 101) recently hosted one of the brightest supernova events related to stellar hiccups.

Applications and Future Research

Astronomers aim to leverage telescopic advancements to:

  • Detect more stars exhibiting hiccups.
  • Study their frequency and duration.
  • Develop models predicting supernova timings.

Stellar hiccups provide a rare glimpse into the chaotic lives of massive stars nearing their end. Observing these events enhances our understanding of supernovae, the creation of heavy elements, and the intricate processes that govern our universe.

The discovery of SN2020acct marked a pivotal moment in astronomy, highlighting the importance of continued research into cosmic anomalies. As technology advances, astronomers hope to unlock more secrets of the universe, expanding humanity’s understanding of the cosmos.

References

  1. Hiccuping Stars Caught in Action – Queen’s University Belfast
  2. Fred Lawrence Whipple Observatory – Center for Astrophysics
#cosmicphenomena, #stellarhiccups, #astronomyresearch, #supernovaexploration, #universesecrets, #astronomydiscoveries, #NASA, #ESO, #cosmicevents, #galaxies, #astronomicalscience, #stars, #universe, #spaceexploration, #astrophysics

How Many Stars Exist in the Universe?

Key Takeaway

The Universe contains an astonishingly large number of stars, estimated to be between 10^22 to 10^24 stars, gathered into billions of galaxies, with our Milky Way galaxy alone containing about 100 billion stars. Attempting to count the stars in the universe has been likened to trying to count the grains of sand on a beach on Earth. Just as we might estimate the number of sand grains by measuring the surface area and depth of the beach, astronomers employ ingenious methods to approximate the number of stars.

Summary

  • The number of stars in the Universe has been a subject of fascination for scientists, philosophers, and dreamers throughout history.
  • With the naked eye, a few thousand stars are visible on a clear night, but even modest telescopes reveal millions more.
  • Stars are not scattered randomly but are grouped into vast galaxies, with our Milky Way galaxy alone estimated to contain about 100 billion stars.
  • There are millions upon millions of other galaxies in the Universe, each containing billions of stars.
  • A rough estimate suggests there could be between 10^22 to 10^24 stars in the entire Universe, although this is an approximation as galaxies vary in size and number of stars.
  • Counting individual stars is impractical; instead, scientists measure integrated quantities like the number and luminosity of galaxies.
  • ESA’s Herschel space observatory contributed by ‘counting’ galaxies in the infrared and measuring their luminosity in this range, providing insight into star formation rates.
  • Herschel revealed that early star formation was hidden by thick dust clouds, which block visible light but emit infrared radiation, indicating more stars than previously thought.
  • The Hubble Space Telescope suggested a peak in star formation around 7 billion years ago, but infrared observations from Herschel revealed more stars forming in the early Universe.
  • The Gaia mission is studying one billion stars in the Milky Way, charting their positions, distances, movements, and brightness changes, building an unprecedented picture of our Galaxy’s structure and evolution.
  • Missions like Herschel, Hubble, Hipparcos, and Gaia are helping astronomers refine their estimates of the total number of stars in the Universe.

How Many Stars Exist in the Universe

Uncovering the Mind-Boggling Number of Stars in the Universe

When we gaze up at the night sky, the twinkling stars seem countless, yet they represent merely a fraction of what the cosmos truly harbors. For centuries, the enigma of quantifying the stars has captured the imagination of scientists, philosophers, and dreamers alike.

Imagine standing under a dark, pristine sky, away from the artificial glow of city lights. With the naked eye, you can discern a few thousand shimmering stars, each a celestial beacon in the vast expanse. However, this is merely the tip of the iceberg. Even modest amateur telescopes reveal millions more, hinting at the unimaginable vastness that awaits beyond our limited perceptions.

Stars are not scattered randomly throughout the universe; instead, they congregate into vast, gravitationally bound structures called galaxies. Our cosmic home, the Milky Way, is one such galaxy, and it alone is estimated to harbor a staggering 100 billion stars. But the Milky Way is merely a speck in the grand fabric of the universe, for it is accompanied by millions upon millions of other galaxies, each a colossal metropolis of stars in its own right.

Attempting to count the stars in the universe has been likened to trying to count the grains of sand on a beach on Earth. Just as we might estimate the number of sand grains by measuring the surface area and depth of the beach, astronomers employ ingenious methods to approximate the number of stars.

By studying a representative sample of galaxies and extrapolating their star counts, scientists have arrived at a mind-boggling estimate: the universe could contain anywhere between 10^22 to 10^24 stars. This range, covering from a trillion trillion to a quadrillion trillion stars, is a testament to the sheer immensity of the cosmos and the limitations of our comprehension.

One of the challenges in accurately estimating the number of stars lies in the obscuring effects of cosmic dust. These opaque clouds, composed of gas and microscopic particles, can block the visible light emitted by stars, rendering them invisible to telescopes operating in the optical wavelengths.

Enter the Herschel Space Observatory, a pioneering infrared telescope launched by the European Space Agency (ESA). By observing in the infrared spectrum, Herschel could peer through the veil of cosmic dust, unveiling a hidden universe of stars that had remained elusive to previous telescopes.

Herschel’s groundbreaking observations revealed that early star formation was more prolific than previously thought, with thick dust clouds obscuring much of the stellar activity in the universe’s younger epochs. This newfound insight challenged the notion that star formation peaked around 7 billion years ago, as suggested by the iconic Hubble Deep Field image.

While space telescopes like Herschel and Hubble have expanded our understanding of the universe’s stellar populations, the Gaia mission focuses its gaze closer to home, studying one billion stars within our galactic neighborhood, the Milky Way.

Launched in 2013, Gaia is meticulously charting the positions, distances, movements, and brightness changes of these stars, building an unprecedented map of our galaxy’s structure and evolution. By precisely tracking each of its one billion target stars multiple times during its mission, Gaia is providing astronomers with invaluable data to unravel the mysteries of our cosmic home and refine our estimates of its stellar inhabitants.

As we stand on the shoulders of these groundbreaking space missions, we inch closer to answering the age-old question: “How many stars are there in the universe?” Yet, with each new discovery, the cosmos reveals itself to be more vast, more complex, and more awe-inspiring than we ever imagined.

The astonishing estimates of stars in the universe not only challenge our comprehension but also ignite a sense of wonder and humility within us. We are but tiny specks in a cosmos teeming with uncountable celestial beacons, each a potential harbinger of life, and each a testament to the greatness and majesty of the universe we call home.

HASHTAGS:

#astronomy, #universe, #stars, #galaxies, #cosmology, #space, #science, #exploration, #wonders, #vastness, #MilkyWay, #Herschel, #Hubble, #Gaia, #HubbleDeepField #How Many Stars Exist in the Universe?

Source: ESA – European Space Agency Link: Read more

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