• Home
  • Introduction
  • Smart Scope Reviews
  • Corona Borealis Variables
  • Messier Marathon Part 1
  • Messier Marathon Part 2
  • Messier Marathon Part 3
  • Asterisms
  • Variable 1 Persei
  • 7 & 8 Persei, NGC 869
  • S CrB Mira Variable
  • Blaze Star T CrB
  • Open Cluster NGC 6611
  • Rosette Nebula
  • Galaxies - Canes Venatici
  • NGC 2523 Barred Galaxy
  • Comet (Tsuchinshan-ATLAS)
  • Tracking Planets
  • Lunar Eclipse 14 Mar 2025
  • Halo Artifacts
  • Cold Weather Performance
  • Scientific American
  • Bay of Fundy Life
  • Illustrated Biography
  • Music Notes
  • Heart & Stroke Fundraiser
  • Sports Notes
  • Song Repertoire
  • Contact Us
  • More
    • Home
    • Introduction
    • Smart Scope Reviews
    • Corona Borealis Variables
    • Messier Marathon Part 1
    • Messier Marathon Part 2
    • Messier Marathon Part 3
    • Asterisms
    • Variable 1 Persei
    • 7 & 8 Persei, NGC 869
    • S CrB Mira Variable
    • Blaze Star T CrB
    • Open Cluster NGC 6611
    • Rosette Nebula
    • Galaxies - Canes Venatici
    • NGC 2523 Barred Galaxy
    • Comet (Tsuchinshan-ATLAS)
    • Tracking Planets
    • Lunar Eclipse 14 Mar 2025
    • Halo Artifacts
    • Cold Weather Performance
    • Scientific American
    • Bay of Fundy Life
    • Illustrated Biography
    • Music Notes
    • Heart & Stroke Fundraiser
    • Sports Notes
    • Song Repertoire
    • Contact Us
  • Sign In
  • Create Account

  • My Account
  • Signed in as:

  • filler@godaddy.com


  • My Account
  • Sign out

Signed in as:

filler@godaddy.com

  • Home
  • Introduction
  • Smart Scope Reviews
  • Corona Borealis Variables
  • Messier Marathon Part 1
  • Messier Marathon Part 2
  • Messier Marathon Part 3
  • Asterisms
  • Variable 1 Persei
  • 7 & 8 Persei, NGC 869
  • S CrB Mira Variable
  • Blaze Star T CrB
  • Open Cluster NGC 6611
  • Rosette Nebula
  • Galaxies - Canes Venatici
  • NGC 2523 Barred Galaxy
  • Comet (Tsuchinshan-ATLAS)
  • Tracking Planets
  • Lunar Eclipse 14 Mar 2025
  • Halo Artifacts
  • Cold Weather Performance
  • Scientific American
  • Bay of Fundy Life
  • Illustrated Biography
  • Music Notes
  • Heart & Stroke Fundraiser
  • Sports Notes
  • Song Repertoire
  • Contact Us

Account

  • My Account
  • Sign out

  • Sign In
  • My Account

Corona Borealis 'Fab Four' Variables

Variables R, S, T & U Coronae Borealis

I am monitoring variables R, S, T, and U Coronae Borealis over a multi-year period that began in the summer of 2024 when I acquired Origin. From the beginning I have used 10-second exposures and 10-minute integration times. The approximate positions of these 4 stars are shown as red dots in my drawing.


Recent Magnitudes (AAVSO)

  • R CrB, 5.9 V, August 13, 2025
  • S CrB, 8.0 V, August 13, 2025
  • T CrB, 9.6 V, August 13, 2025
  • U CrB, 7.8 V, August 9, 2025

References

  1. "Stellar Opposites: R and T Coronae Borealis", Sky & Telescope, 72(2), August 1986, p. 161.
  2. "S and U Coronae Borealis", Sky & Telescope, 75(6), June 1988, p. 631.

R Coronae Borealis

Discussion

On this date, the visual magnitude of this peculiar variable was approximately 6.1 according to AAVSO data. You can see that it is significantly brighter than HD 141352 (7.4)  in the image. This giant can randomly drop in brightness to 15 every few years. Since that hasn't occurred since sometime before August 2023, it could happen any day this fall (2025).

Logbook

  • Date & Time: August 7, 2024, 9:24 pm
  • Location: Kempt Shore, Nova Scotia, Canada, 45°N
  • Conditions: Partly cloudy
  • Sunset: 8:35 pm
  • Moonset: 10:05 pm
  • Moon Phase: Waxing crescent (12%)
  • Technical: 10-sec exposures, 10-min integration, line power, no filter, no post-processing

R CrB in Simbad Database

    S Coronae Borealis

    Discussion

    On this date, the visual magnitude of this Mira long-period variable was approximately 7.8 according to AAVSO data. This is dimmer than nearby HD 136654 at 6.88 even though it appears brighter here. Note that these two stars are different in colour, orange (+1.30) versus yellow (+0.54), respectively. S CrB has a period of 360 days and a visual magnitude range of about 7 to 13. 

    Logbook

    • Date & Time: August 11, 2024, 10:46 pm
    • Location: Kempt Shore, Nova Scotia, Canada, 45°N
    • Conditions: Clear
    • Sunset: 8:27 pm
    • Moonset: 11:38 pm
    • Moon Phase: First quarter (54%)
    • Technical: 10-sec exposures, 10-min integration, line power, no filter, no post-processing

    S CrB in Simbad Database

      Copyright © 2025 Celestron Origin Images And Technology - All Rights Reserved.

      Powered by

      • Home
      • Introduction
      • Smart Scope Reviews
      • Corona Borealis Variables
      • Messier Marathon Part 1
      • Messier Marathon Part 2
      • Messier Marathon Part 3
      • Asterisms
      • Variable 1 Persei
      • 7 & 8 Persei, NGC 869
      • S CrB Mira Variable
      • Blaze Star T CrB
      • Open Cluster NGC 6611
      • Rosette Nebula
      • Galaxies - Canes Venatici
      • NGC 2523 Barred Galaxy
      • Comet (Tsuchinshan-ATLAS)
      • Tracking Planets
      • Lunar Eclipse 14 Mar 2025
      • Halo Artifacts
      • Cold Weather Performance
      • Scientific American
      • Bay of Fundy Life
      • Illustrated Biography
      • Music Notes
      • Sports Notes
      • Contact Us

      This website uses cookies.

      We use cookies to analyze website traffic and optimize your website experience. By accepting our use of cookies, your data will be aggregated with all other user data.

      Accept