Wednesday, February 4, 2026

2025: Where to Spot Star’s Supernova Every 80 Years

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Universe Today, has now spilled over into 2025, still keeping us in anticipation.

Around this time last year, speculations arose about the potential brightening of T Coronae Borealis (‘T CrB’) to naked-eye visibility, however, the celestial show is running fashionably late. Yet, recent research unveils promising signs of an upcoming event.

Every 80 years, the star experiences an outburst – a phenomenon first observed by astronomer John Birmingham in 1866, with its previous brightening recorded in February 1946. Now, as we mark 80 years since that event, all eyes are on T Coronae Borealis in the Hercules/Corona Borealis/Serpens Caput constellation.

Situated 2,000 light-years away, the star typically rests below +10th magnitude but during its peak, it dazzles at +2nd magnitude, rivaling the brightness of Alpha Coronae Borealis (Alphecca), its host constellation.

Locating T Coronae Borealis in the Night Sky

Currently, T CrB rises in the east around midnight, ascending to the pre-dawn sky, with late November posing the least favorable conditions due to solar interference. However, as we progress through early 2025, the star will transition into the evening sky, offering better viewing opportunities.

Position of T CrB in red within the Corona Borealis constellation. (IAU and Sky & Telescope magazine/Roger Sinnott & Rick Fienberg/Wikimedia commons/CC-BY-SA 3.0/ScienceAlert)

The celestial coordinates for T CrB are:

  • Declination: +25 degrees, 54? 58?
  • Right Ascension: 15 Hours 59? 30?
constellations
Eastern view in early March, post-midnight. (Stellarium)

Exceptional Recurrent Novae

Often found within dual-star systems, recurrent novae like T CrB involve a red giant star transferring material onto a white dwarf companion. This intricate accretion process culminates in an explosive nova event.

Exceptional Recurrent Novae

In recent studies, Gesesew Reta from the S.N. Bose National Centre for Basic Sciences noted significant variations in the H-alpha line profile of T CrB, hinting at a potential eruption. While this shift may not confirm an imminent outburst, it suggests a surge in temperature and accretion rate, signaling a possible event on the horizon.

Anticipated Events in 2025

While hopes are high for a spectacular +2nd magnitude display, this phenomenon might not outshine the brightest stars as hyped. Galactic novae occur every decade, but recurrent novae are scarce, with only a handful recorded.

During this period, the familiar Corona Borealis asterism will assume a different look as T Coronae Borealis adds its radiance. Astrophysicists and astronomers are eagerly awaiting this unique opportunity to study the star, utilizing tools like JWST and Hubble.

Resources on Variable Stars

The American Association of Variable Star Observers (AAVSO) recently shared insights on T CrB’s status, while Space Weather offers daily updates on its magnitude. So, whether you choose to follow online updates or rely on your own observations, the awaited stellar phenomenon promises a captivating experience.

So, keep your eyes peeled, as you might just witness a once-in-a-lifetime celestial affair, adorning the Northern Crown. Who knows, you could be the first to spot this celestial marvel during its grand reveal.

This article was initially featured on Universe Today. To read the full article, click here.


Vocabulary List:

  1. Anticipation /ænˌtɪsɪˈpeɪʃən/ (noun): The act of looking forward to something.
  2. Phenomenon /fəˈnɒɡənən/ (noun): An observable event or occurrence.
  3. Magnitude /ˈmæɡnɪtjuːd/ (noun): The size extent or importance of something.
  4. Accretion /əˈkriːʃən/ (noun): The process of growth or increase typically in terms of size or amount.
  5. Eruption /ɪˈrʌpʃən/ (noun): The sudden occurrence of something typically a violent release of energy.
  6. Celestial /sɪˈlɛs.tɪ.əl/ (adjective): Relating to the sky or outer space.

How much do you know?

Where can T Coronae Borealis be located in the night sky?
In the east around midnight
In the west during the day
Below the horizon at all times
At the North Pole
What event is T Coronae Borealis anticipated to be the highlight of?
2019
2020
2024
2026
What is the typical magnitude of T Coronae Borealis?
Below +5th magnitude
Around +10th magnitude
+2nd magnitude during peak
+20th magnitude
What process leads to an explosive nova event in recurrent novae like T Coronae Borealis?
Material transfer from a white dwarf to a red giant
Material transfer from a red giant to a white dwarf
Material transfer from a star to a black hole
Material transfer from a neutron star to a white dwarf
Which organization provides daily updates on the magnitude of T Coronae Borealis?
NASA
AAVSO
ESA
SpaceX
How often do galactic novae occur?
Every 5 years
Every decade
Every century
Every millennium
T Coronae Borealis is expected to outshine the brightest stars in 2025.
T Coronae Borealis is currently visible in the late November sky.
Recurrent novae like T Coronae Borealis involve a red giant star transferring material onto a white dwarf companion.
Astrophysicists and astronomers are not interested in studying the upcoming event of T Coronae Borealis.
Only a few recurrent novae have been recorded in history.
The celestial coordinates for T Coronae Borealis include a declination of +25 degrees, 54? 58?.
T Coronae Borealis typically rests below + magnitude but during its peak, it dazzles at +2nd magnitude.
The outburst of T Coronae Borealis was first observed by astronomer John Birmingham in .
Recurrent novae like T Coronae Borealis involve material transfer from a giant star to a white dwarf companion.
The anticipated highlight year for T Coronae Borealis, according to Universe Today, was .
T Coronae Borealis rises in the , ascending to the pre-dawn sky as early as 2025.
The star T Coronae Borealis is situated light-years away.
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