Skip to main content

Is T Coronae Borealis About to Light Up?

Late is better than never for the ‘Blaze Star’ T Coronae Borealis.

It was on track to be the top astronomical event for 2024… and here we are in 2025, still waiting. You might remember around this time last year, when a notice went out that T Coronae Borealis (‘T CrB’) might brighten into naked eye visibility. Well, the bad news is, the ‘Flare Star’ is officially late to the celestial sky show… but the good news is, recent research definitely shows us that something is definitely afoot.

The outburst occurs once every 80 years. First noticed by astronomer John Birmingham in 1866, T Coronae Borealis last brightened in February 1946. That’s 80 years ago, this month. Located about 2,000 light-years distant on the Hercules/Corona Borealis/Serpens Caput constellation junction border, the star spends most of its time below +10th magnitude. Typically during outburst, the star flares and tops out at +2nd magnitude, rivaling the lucida of its host constellation, Alpha Coronae Borealis (Alphecca).

Finding T Corona Borealis in the Sky

We’re fortunate that T CrB currently rises in the east around local midnight. T CrB then rides high in the pre-dawn sky. Late November would be the worst time for the nova to pop, when the Sun lies between us and the star. The situation only improves as early 2025 goes on, and the region moves into the evening sky.

Sky
The constellation Corona Borealis and the location of the ‘Blaze Star.’ Credit: Stellarium

The coordinates for T CrB are:

Declination: +25 degrees, 54’ 58”

Right Ascension: 15 Hours 59’ 30”

Blaze
Looking eastward in early March, two hours after local midnight. Credit: Stellarium

Rare Recurrent Novae

T CrB and other recurrent novae are typically part of a two-star system, with a cool red giant star dumping material on a hot white dwarf companion. This accretion builds up to a runaway flash point, and a nova occurs.

Chart
A chart of known recurrent novae. Adapted from The Backyard Astronomer’s Deep-Sky Field Guide by David Dickinson.

Two recent notices caught our eye concerning T Coronae Borealis: one titled T CrB on the Verge of an Outburst: H-Alpha Profile Evolution and Accretion Activity and A Sudden Increase of the Accretion Rate of T Coronae Borealis. Both hint that we may soon see some action from the latent flare star.

“My spectral analysis showed a considerable change in the strength of the H-alpha line profile, which could be considered an indicator of the possible eruption of T CrB in the near future. This change posibly resulted from a significant increase in the temperature and accretion rate,” Gesesew Reta (S.N. Bose National Centre for Basic Sciences) told Universe Today. “However, this cannot serve as definitive confirmation of the expected eruption. Novae are inherently unpredictable, and a more detailed analysis, considering broader parameters, is needed for a more accurate prediction.”

T CrB
An artist’s conception of T Corona Borealis in outburst. Credit: NASA’s Visualization Studio/Adriana Manrique Gutierrez/Scott Wiessinger

What to expect in 2025

First, I would manage expectations somewhat; while +2nd magnitude is bright enough to see with the naked eye, it’s not set to be the “Brightest Star…. Ever!” as touted around the web. We get naked eye galactic novae every decade or so, though recurrent novae are a rarity, with only about half a dozen known examples.

Certainly, the familiar ring-shaped northern crown asterism of Corona Borealis will look different for a few weeks, with a new rival star. Certainly, modern astrophysicists and astronomers won’t pass up the chance to study the phenomenon… I would fully expect assets including JWST and Hubble to study the star.

Variable Star Resources

The American Association of Variable Star Observers (AAVSO) also posted a recent article on current prospects for T CrB… another good quick look for the brightness of flare star is Space Weather, which posts a daily tracker for its magnitude.

Or you could simply step outside every clear March morning, and look up at Corona Borealis with your ‘Mark-1 eyeballs’ and see if anything is amiss. Hey, you might be the very first one to catch the ‘new star’ adorning the Northern Crown, during its current once-in-a-lifetime apparition.

The post Is T Coronae Borealis About to Light Up? appeared first on Universe Today.



from Universe Today https://ift.tt/w057vK2
via IFTTT

Comments

Popular posts from this blog

More Data and Machine Learning has Kicked SETI Into High Gear

For over sixty years, astronomers and astrophysicists have been engaged in the Search for Extraterrestrial Intelligence (SETI). This consists of listening to other star systems for signs of technological activity (or “technosignatures), such as radio transmissions. This first attempt was in 1960, known as Project Ozma, where famed SETI researcher Dr. Frank Drake (father of the Drake Equation) and his colleagues used the Robert C. Byrd Green Bank Telescope in West Virginia to conduct a radio survey of Tau Ceti and Epsilon Eridani. Since then, the vast majority of SETI surveys have similarly looked for narrowband radio signals since they are very good at propagating through interstellar space. However, the biggest challenge has always been how to filter out radio transmissions on Earth – aka. radio frequency interference (RFI). In a recent study, an international team led by the Dunlap Institute for Astronomy and Astrophysics (DIAA) applied a new deep-learning algorithm to data collecte...

The First Close-Up Picture of Star Outside the Milky Way

Like a performer preparing for their big finale, a distant star is shedding its outer layers and preparing to explode as a supernova. Astronomers have been observing the huge star, named WOH G64, since its discovery in the 1970s. It’s one of the largest known stars, and also one of the most luminous and massive red supergiants (RSGs). The star is surrounded by an envelope of expelled star-stuff, which could indicate it’s getting ready to explode. WOH G64 isn’t in the Milky Way; it’s in the Large Magellanic Cloud (LMC), the Milky Way’s largest satellite galaxy. Getting these detailed image is quite a feat for the ESO’s Very Large Telescope Interferometer. It’s also quite an accomplishment for the team of scientists behind the image. They’ve published their images and the results of their observations of the star in the journal Astronomy and Astrophysics. Their research is titled “ Imaging the innermost circumstellar environment of the red supergiant WOH G64 in the Large Magellanic ...

eROSITA Sees Changes in the Most Powerful Quasar

After almost seventy years of study, astronomers are still fascinated by active galactic nuclei (AGN), otherwise known as quasi-stellar objects (or “quasars.”) These are the result of supermassive black holes (SMBHs) at the center of massive galaxies, which cause gas and dust to fall in around them and form accretion disks. The material in these disks is accelerated to close to the speed of light, causing it to release tremendous amounts of radiation in the visible, radio, infrared, ultraviolet, gamma-ray, and X-ray wavelengths. In fact, quasars are so bright that they temporarily outshine every star in their host galaxy’s disk combined. The brightest quasar observed to date, 100,000 billion times as luminous as our Sun, is known as SMSS J114447.77-430859.3 (J1144). This AGN is hosted by a galaxy located roughly 9.6 billion light years from Earth between the constellations Centaurus and Hydra. Using data from the eROSITA All Sky Survey and other space telescopes, an international t...