RSS Amplifier

www.saltwire.com RSS Feed · Aug 20, 2026

A black hole masquerading as a star

0
Sign in to vote or save

Glenn Roberts · pniatlantic

Skip to Content
  1. Home
  2. Atlantic Canada
  3. Cape Breton
  4. Newfoundland & Labrador
  5. Newfoundland and Labrador Lifestyle
  6. Nova Scotia
  7. Prince Edward Island
  8. PEI Lifestyle

A black hole masquerading as a star 

James Webb Space Telescope observations reveal an extraordinary object challenging what astronomers know about the early universe

Last updated 19 hours ago
This image from NASA's Spitzer Space Telescope shows the elliptical galaxy Messier 87 (M87), the home galaxy of the supermassive black hole imaged in 2019 by the Event Horizon Telescope (EHT). Spitzer's infrared view shows a faint trace of a jet of material spewing to the right of the galaxy - a feature that was previously one key indicator that a supermassive black hole lived at the galaxy's center. More prominent in the image is the shockwave created by that jet. The inset in the image below shows a close-up view of the shockwave on the right side of the galaxy, as well as the shockwave from a second jet traveling to the left of the galaxy. Located about 55 million light-years from Earth, M87 has been a subject of astronomical study for more than 100 years.
This image from NASA's Spitzer Space Telescope shows the elliptical galaxy Messier 87 (M87), the home galaxy of the supermassive black hole imaged in 2019 by the Event Horizon Telescope (EHT). Spitzer's infrared view shows a faint trace of a jet of material spewing to the right of the galaxy - a feature that was previously one key indicator that a supermassive black hole lived at the galaxy's center. More prominent in the image is the shockwave created by that jet. The inset in the image below shows a close-up view of the shockwave on the right side of the galaxy, as well as the shockwave from a second jet traveling to the left of the galaxy. Located about 55 million light-years from Earth, M87 has been a subject of astronomical study for more than 100 years. NASA/JPL-Caltech/IPAC/Event Hori

Black holes are some of the most enigmatic objects in the universe. First conceptualized by the German-born theoretical physicist Albert Einstein (1879-1955) in his theory of general relativity, black holes have only recently been photographed.  

Subscribe now to access this story and more:

  • Unlimited access to the website and app
  • Exclusive access to premium content, newsletters and podcasts
  • Full access to the e-Edition app, an electronic replica of the print edition that you can share, download and comment on
  • Enjoy insights and behind-the-scenes analysis from our award-winning journalists
  • Support local journalists and the next generation of journalists

Subscribe or sign in to your account to continue your reading experience.

  • Unlimited access to the website and app
  • Exclusive access to premium content, newsletters and podcasts
  • Full access to the e-Edition app, an electronic replica of the print edition that you can share, download and comment on
  • Enjoy insights and behind-the-scenes analysis from our award-winning journalists
  • Support local journalists and the next generation of journalists

Create an account or sign in to continue your reading experience.

  • Access additional stories every month
  • Share your thoughts and join the conversation in our commenting community
  • Get email updates from your favourite authors

Sign In or Create an Account

or

While it is impossible to optically image a black hole itself, the bright band of light referred to as the “accretion disk” swirling around a black hole can be photographed, as it was in 2019, when the first image of the massive black hole at the center of the M87 galaxy was captured.  

Very little is known about the origin and nature of black holes, other than that they are objects having such immense density and gravity that not even light can escape from them; the “black” refers to the absence of light coming from them. It is theorized that black holes exist in a multitude of sizes, ranging from small enough to pass through any object in the universe, to such massive objects as Phoenix A, a black hole having billions of solar masses located in the constellation of Phoenix. 

In 2023, the James Webb Space Telescope (JWST) imaged an intriguing object located billions of light-years from Earth in a low-mass dwarf galaxy in the constellation of Cetus – the Sea Monster. As this newly discovered object defied all known cosmic categories, it was labelled as a “black hole star,” an object that resembles both a black hole and a star.   

It was discovered during the JWST “Mirage or Miracle” (MoM) survey of galaxies in the early universe. Consequently, it was named MoM-BH*-1 (“black hole star – one”).  The object is believed to have formed approximately 660 million years after the Big Bang, when the core of a supermassive protostar collapsed into a stellar-mass black hole.  

Astronomers uncover an extraordinarily unusual cosmic object 

MoM-BH*-1 (MoM-1) first appeared as a bright red source of light in the JWST images. It had an extremely unusual colour profile, in that it was nearly invisible when viewed through blue filters, but highly visible when viewed through red filters; it was, in fact, one of the reddest distant objects ever recorded. Spectroscopic analysis of MoM-1 indicates that it contains the strongest Balmer break of any known astronomical objects measured in redshift.  

A Balmer break, also known as a Balmer jump, is the difference in the intensity of the stellar spectrum on either side of the limit of the Balmer series of hydrogen – one of a set of six named series respecting the spectral line emissions of the hydrogen atom. The strong Balmer break of MoM-1 indicates the presence of very dense hydrogen gas. 

An analysis of MoM-1’s chemical composition found vast amounts of hydrogen and helium, but no evidence of metals or heavier elements; this discovery excludes ordinary stars as the object’s light source. Also, although its spectrum links it to hydrogen absorption, MoM-1’s Balmer break far exceeds what normal stars or normal star populations typically produce; even the reddest stellar populations discovered to date show a Balmer break less than one-third that of MoM-1. Its broad emission lines combined with deep absorption features indicate that MoM-1 exists in an environment of unusually dense gas.  

At first, astronomers thought they might have found a new type of stellar atmosphere, as MoM-1’s brightness exceeded that which a stellar body of that scale could generate from nuclear fusion. To understand MoM-1 formation, astronomers developed a computer model in which MoM-1 contained a massive black hole surrounded by a dense cocoon of gas, giving MoM-1 the appearance of a huge star-like object.  

The model demonstrated that the dense envelope of hydrogen would absorb and scatter the object’s radiation, thereby producing its unusual red shift colour and distinctive spectral pattern. The black hole’s immense radiation would also be strong enough to be able to pass through the dense cloud of gas, and to be detected by the JWST. 

MoM-1 may be related to unexplained ‘little red dots’

Astronomers also discovered evidence that MoM-1 may have increased in brightness by approximately 30 per cent over a two-month period, behaviour typical of massive black holes rapidly feeding on surrounding material, confirming their theory that MoM-1 was, in fact, a black hole masquerading as a star.  

This image shows the location of galaxy CANUCS-LRD-z8.6 in galaxy cluster MACS J1149.5+2223, as seen by the NASA/ESA/CSA James Webb Space Telescope's Near-Infrared Camera (NIRCam). CANUCS-LRD-z8.6 is part of a class of small, very distant and strikingly red galaxies called Little Red Dots (LRDs), which have been spotted in increasing numbers by Webb's surveys of the early Universe. It is located in the constellation Leo (the Lion), and is seen by Webb just 570 million years after the Big Bang.
This image shows the location of galaxy CANUCS-LRD-z8.6 in galaxy cluster MACS J1149.5+2223, as seen by the NASA/ESA/CSA James Webb Space Telescope’s Near-Infrared Camera (NIRCam). CANUCS-LRD-z8.6 is part of a class of small, very distant and strikingly red galaxies called Little Red Dots (LRDs), which have been spotted in increasing numbers by Webb’s surveys of the early Universe. It is located in the constellation Leo (the Lion), and is seen by Webb just 570 million years after the Big Bang. ESA/Webb, NASA & CSA, G. Rihtar

There is a theory that the MoM-1 object might possibly be related to a yet-as-unexplained group of astronomical sources referred to as “little red dots”. Little red dots are mysterious red sources of light found in photographs of the early universe that are believed to be black holes surrounded by dense ionized gas. Interestingly, these little red dots do not appear in astro-photographs from more recent cosmic periods. 

Whatever their origin, little red dots and black hole stars such as MoM-1 are proof that the universe is still quite capable of demonstrating how very little we know and, more importantly, understand the universe in which we dwell. No doubt, there are many more astronomical mysteries such as MoM-1 waiting to be discovered.  

This week’s sky 

Mercury (mag. -1.4, in Cancer – the Crab) will pass behind the sun (superior solar conjunction) on Aug. 27 and therefore will not be observable this coming week. On Aug. 27, Mercury will begin its passage around the far side of the sun, referred to as superior solar conjunction. 

Venus (mag. -4.4, in Virgo – the Maiden) becomes visible around 8:25 p.m. ADT, 8 degrees above the southwest horizon as dusk gives way to darkness, before sinking towards the horizon and setting about 9:25 p.m. ADT.  

Mars (mag. +1.3, in Gemini – the Twins) rises in the eastern, predawn sky around 1:45 a.m. ADT, reaching 36 degrees above the eastern horizon, before fading from view by about 5:30 a.m. ADT.  

Jupiter (mag. -1.8, in Cancer) rises around 4:35 a.m. ADT, reaching 12 degrees above the eastern horizon, before fading from view by about 6 a.m. ADT. 

Saturn (mag. +0.4, in Pisces – the Fish) becomes accessible 10 degrees above the eastern horizon around 10:45 p.m. ADT, reaching its highest point in the sky 46 degrees above the southern horizon shortly before 4 a.m. ADT, before being lost to the dawn twilight 40 degrees above the southwest horizon around 5:45 a.m. ADT. Saturn and the Moon will make an apparent close approach (an appulse) with one another, as viewed from Earth, at 11:32 p.m. ADT on Aug. 30. 

Uranus (mag. +5.7, in Taurus – the Bull) rises around 11:35 p.m. ADT, reaching 52 degrees above the southeast horizon, before fading from view in the dawn twilight by about 5 a.m. ADT. 

Neptune (mag. +7.8 in Pisces), now approaching opposition, becomes accessible 21 degrees above the southeast horizon by about 11:30 p.m. ADT, before reaching its highest point in the sky 43 degrees above the southern horizon around 3:15 a.m. ADT, and then disappearing into the dawn twilight around 5 a.m. ADT, 38 degrees above the southwest horizon.  

Partial lunar eclipse coming 

On Aug. 27, there will be a partial lunar eclipse. It will begin at 10:25 p.m. ADT, and finish at 4:02 a.m. ADT on the Aug. 28. A maximum eclipse will occur at 1:14 a.m. ADT, with 93 per cent of the lunar surface covered by the Earth’s shadow. August’s Full Moon at 1:18 a.m. ADT on the Aug. 28 is often referred to as the “Sturgeon Moon,” in reference to the time of the year when sturgeon, North America’s largest fish, run up the rivers of the Great Lakes. 

Errata: I mixed up my distance figures in last week’s article. One astronomical unit (AU) is equal to 148,800,000 kilometres (not 93,000,000). As a consequence, Jupiter orbits the sun at an average distance of 774,206,400 km or 5.203 AU. My apologies. Thanks to my sharp-eyed readers who caught the error. 

Until next week, clear skies. 

Events: 

Aug. 25 – Moon at aphelion (farthest point from the sun); 5:21 p.m. ADT; 150,749,280 km or 1.0131 AU 

Aug. 27 – Mercury at superior solar conjunction at 2:11 p.m. ADT; partial lunar eclipse starts at 10:25 p.m. ADT (see above) 

Aug. 28 – Partial lunar eclipse maximum at 1:14 a.m. ADT; full “Sturgeon Moon” at 1:18 a.m. ADT 

Aug. 30 – Close approach of the moon and Saturn at 11:32 p.m. ADT 

This website uses cookies to personalize your content (including ads), and allows us to analyze our traffic. Read more about cookies here. By continuing to use our site, you agree to our Terms of Use and Privacy Policy.

Read the original on saltwire.com

Comments

Nothing yet. Say the first thing.

    Sign in to join the conversation.