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Ephemeris: 11/11/2025 – The difference between a nova and a Type 1a supernova

November 11, 2025 Comments off

This is Bob Moler with Ephemeris for Veterans Day, Tuesday, November 11th. Today the Sun will be up for 9 hours and 43 minutes, setting at 5:18, and it will rise tomorrow at 7:36. The Moon, 1 day before last quarter, will rise at 11:37 this evening.

I’ve always wondered what the difference is between a nova like T Coronae Borealis, sometimes called the Blaze Star, and a Type 1a supernova. Both involve a white dwarf star and a larger star and having the mass of the larger star being drawn off onto the surface of the white dwarf until an explosion happens. If the detonation, which is a thermonuclear detonation of the hydrogen drawn off the larger star, is on the surface only, involving the outer layers of the white dwarf, the star becomes thousands of times brighter for a short period of time. The star survives. In the Type 1a supernova, the accretion of the hydrogen onto the white dwarf causes a more massive explosion involving the core of the white dwarf because its mass approaches or will surpass 1.4 times the Sun’s mass. At that point the star explodes.

The astronomical event times given in this blog are for the Traverse City/Interlochen area of Michigan (Lat 44.7° N, Long 85.7° W; EDT, UT – 4 hours) unless stated otherwise. Times will be different for other locations.

Addendum

This image has an empty alt attribute; its file name is recurrent-nova_nasa-gsfc.jpg
NASA artist's depiction of a recurrent nova.
NASA artist’s depiction of a recurrent nova. In this case the white dwarf is buried in the disc of gas surrounding a red giant star. This is a generic representation and may not depict the state of affairs of T CrB.
If T CrB goes nova around November 10, 2025, this would be the location of the nova in the sky at 7 PM for the Grand Traverse area of Michigan.
If T CrB goes nova around November 10, 2025, this would be the location of the nova in the sky at 7 PM for the Grand Traverse area of Michigan. This is about an hour and 20 minutes after sunset for most northern mid-latitude locations. Created using Stellarium,, labeled in LibreOffice Draw and exported in GIMP.

Categories: Nova, Supernova Tags: ,

Ephemeris: 11/10/2025 – Waiting on a stellar explosion

November 10, 2025 Comments off

This is Ephemeris for Monday, November 10th. Today the Sun will be up for 9 hours and 46 minutes, setting at 5:19, and it will rise tomorrow at 7:34. The Moon, 2 days before last quarter, will rise at 10:22 this evening.

According to one astronomer, that I mentioned last Thursday, today is about the day he expects a star to erupt as a nova in the constellation Corona Borealis, the Northern Crown. In the early evening, it will appear low in the west northwest. The star is designated T Coronae Borealis (T CrB). Its appearance should make the normal news outlets, because it will be the brightest stellar outburst in a very long time. It will appear just left of the constellation Corona Borealis and be about as bright as its brightest normal star. However, it will soon fade and to be less the naked eye brightness in about a week. So we’re hoping for clear skies, if it happens. If it’s not this time, the next predicted time is June 25th, next year. Or he could be wrong, and it could go off at any time. Spaceweather.com has more information.

The astronomical event times given in this blog are for the Traverse City/Interlochen area of Michigan (Lat 44.7° N, Long 85.7° W; EDT, UT – 4 hours) unless stated otherwise. Times will be different for other locations.

Addendum

If T CrB goes nova around November 10, 2025, this would be the location of the nova in the sky at 7 PM for the Grand Traverse area of Michigan.
If T CrB goes nova around November 10, 2025, this would be the location of the nova in the sky at 7 PM for the Grand Traverse area of Michigan. This is about an hour and 20 minutes after sunset for most northern mid-latitude locations. Created using Stellarium, labeled in LibreOffice Draw and exported in GIMP.

According to a paper in the Research Notes of the American Astronomical Society, Jean Schneider with the Paris Observatory predicted that the next eruption of T Coronae Borealis would be somewhere around November 10th 2025, or June 25th 2026. The first prediction of the 27th of March earlier this year turned out to not have occurred. These were tentative predictions based on the orbit around each other, of the two stars involved. The period of 80 years between eruptions is an approximation. There is an additional periodicity due to the fact that the two stars involved, a red giant and a white dwarf, have an orbital period of about 228 days which is why the predictions are 228 days apart. There have been four previous eruptions of the star observed. The first was in 1217, the next in 1787, then in 1866 and then finally in 1946. The reason for the big gap between 1217 and 1787 is unknown. Either the star didn’t erupt, or more likely, nobody observed and recorded it. The times of the first two eruptions weren’t accurately reports, but fell within what the 228-day periodicity would explain.

T Coronae Borealis is far enough north in the sky so that it is visible sometime during the night, year round. Currently, it would be best seen at the end of twilight in the west northwest. This will shift over to the morning sky, before morning twilight, after about the 25th of November, only 15 days from now in the east northeast. This star like any other star that rises and sets does so approximately 4 minutes earlier each night, or 28 minutes per week. So after the 25th the best observing opportunity will be before dawn in the morning until much later in the late winter, when it will be available also in the evening sky again.

Ephemeris: 11/06/2025 – An astronomer thinks a nova will appear soon

November 6, 2025 Comments off

This is Ephemeris for Thursday, November 6th. Today the Sun will be up for 9 hours and 56 minutes, setting at 5:24, and it will rise tomorrow at 7:29. The Moon, 1 day past full, will rise at 5:50 this evening.

We’ve been waiting for the past year or so for the eruption of a nova in the constellation Corona Borealis the Northern Crown. It last erupted in 1946. Eruptions are about 80 years apart. Astronomer Jean Schneider of the Paris Observatory has made a study of this particular nova. It occurs in a binary star system with a white dwarf and a much larger star that orbit each other every 228 days. So it is possible that the Nova occurs at one point in that orbit. And based on the last eruption in 1946, November 10th, give or take, is one of the days we might look to see the eruption. If it doesn’t happen that day its next likely occurrence is around June 25th next year. It will appear just left of Corona Borealis low in the west northwest around 7 PM, and as bright as the normally brightest star in that constellation.

The astronomical event times given in this blog are for the Traverse City/Interlochen area of Michigan (Lat 44.7° N, Long 85.7° W; EDT, UT – 4 hours) unless stated otherwise. Times will be different for other locations.

Addendum

If T CrB goes nova around November 10, 2025, this would be the location of the nova in the sky at 7 PM for the Grand Traverse area if Michigan.
If T CrB goes nova around November 10, 2025, this would be the location of the nova in the sky at 7 PM for the Grand Traverse area if Michigan. This is about an hour and 20 minutes after sunset for most northern mid-latitude locations. Created using Stellarium, labeled in LibreOffice Draw and exported in GIMP.

The website Spaceweather.com monitors reports of the brightness of the star on the right side of its page under the heading of T CrB NOVA WATCH. It is currently around 10th magnitude, invisible to the naked eye and barely visible in binoculars. It is expected to grow to 2nd magnitude or 1,600 times it’s normal brightness, about as bright as a Big Dipper star or Alphecca, near it, in Corona Borealis. The nova will fade rapidly, and will be visible to the naked eye for only about a week.

Ephemeris: 05/20/2025 – Corona Borealis, Ariadne’s Crown

May 20, 2025 Comments off

This is Ephemeris for Tuesday, May 20th. Today the Sun will be up for 15 hours and 1 minute, setting at 9:10, and it will rise tomorrow at 6:08. The Moon, at last quarter today, will rise at 3:12 tomorrow morning.

There are two bright stars in the eastern part of the sky. High in the southeast at 11 PM is Arcturus, and in the east northeast, lower down is the star Vega. A third of the way between Arcturus and Vega is a small arc of stars called Corona Borealis, the northern crown. It is a small constellation. The brightest star in it is called Alphecca. According to Greek mythology it is the crown given to Princess Ariadne, daughter of King Minos of Crete. Of interest in the next year or so is a possibility of a nova or bright star appearing just south of that arc of stars for about a week. It is a recurrent nova, which explodes about every 80 years. The last time was in 1946, so the next time would be within the next year or so. And astronomers are breathlessly waiting for that to happen.

The astronomical event times given in this blog are for the Traverse City/Interlochen area of Michigan (Lat 44.7° N, Long 85.7° W; EDT, UT – 4 hours) unless stated otherwise. Times will be different for other locations.

Addendum

Looking in the east southeastern sky for Corona Borealis. The view is from the horizon to just pass the zenith. Corona Borealis is about 1/3 of the way from Arcturus which is high in the southeast to Vega lower in the east-northeast.. It’s a small semicircle of stars. Created using Stellarium, LibreOffice Draw, and GIMP.
T Coronae Borealis (T CrB) nova finder.
T Coronae Borealis (T CrB) nova finder, when it occurs. This is the orientation of its position in the sky if it occurs in the spring. Created using Stellarium, LibreOffice Draw, and GIMP.

Ephemeris: 11/11/2024 – Still waiting for the promised nova

November 11, 2024 Comments off

This is Ephemeris for Veterans Day, Monday, November 11th. Today the Sun will be up for 9 hours and 43 minutes, setting at 5:18, and it will rise tomorrow at 7:36. The Moon, 2 days past first quarter, will set at 3:19 tomorrow morning.

We’ve been waiting all year so far for the appearance of a nova or Blaze Star, as they called it, in the constellation of Corona Borealis. The astronomical name For it is T Coronae Borealis or T CrB for short. It last erupted in 1946 and the time before that it was 1866 an interval of 80 years. This year would be 78 years since 1946 so we could be waiting another two years. Observations of the star, which is still visible, though faint, between eruptions, were not as comprehensive in the prior 80 years, as they are today. It’s possible that observations of pre-nova activity were missed during war years preceding the 1946 outburst.

The astronomical event times given are for the Traverse City/Interlochen area of Michigan (EST, UT – 5 hours). Times will be different for other locations.

Addendum

A Finder for the location of the nova, or Blaze Star, T Coronae Borealis or T CrB (when it happens), for the early evening now
A Finder for the location of the nova, or Blaze Star, T Coronae Borealis or T CrB (when it happens), for the early evening now. Corona Borealis is a small horseshoe shaped constellation whose brightest star Alphecca is just above the “n” in Corona. It is a second magnitude star about the same brightness as the nova will get at its peak. After late November the best time to see the nova, if it occurs then, will be in the morning sky just before sunrise. Though the nova is not circumpolar, meaning it rises and sets, it is up in the sky for 16 of the 24 hours of the day, so we will never completely lose it to daylight. When the Nova explosion occurs it will be visible to the naked eye for about a week so it’s easy to miss in time and also, in Northern Michigan due to the winter weather, we could miss it because of clouds. But as I mentioned in the program script above we are currently about two years away from the nominal time between between explosions, so we still have a couple of years to go before 80 years are up. Created using Stellarium, and LibreOffice Draw.

Ephemeris: 08/12/2024 – Expect a stellar explosion soon

August 12, 2024 Comments off

This is Ephemeris for Monday, August 12th. Today the Sun will be up for 14 hours and 9 minutes, setting at 8:52, and it will rise tomorrow at 6:43. The Moon, at first quarter today, will set at 12:07 tomorrow morning.

This is a reminder that we are expecting a once in a lifetime nova or exploding star in our skies fairly soon, maybe in a month or two. At least we’re hoping. Unlike many reoccurring events in astronomy this one cannot be predicted exactly since we’re not really sure what is happening. We have a general idea. The star is T Coronae Borealis which is in the Northern Crown constellation, which is a small semicircular stellar group near the star Arcturus which is a bright star found off the end of the handle of the Big Dipper. It is to the upper left of that star and the kite shaped constellation of Boötes of which Arcturus is at the base. The nova will appear as bright as Corona’s brightest star, but will fade in about 8 days below naked eye visibility. So it will be easy to miss.

The astronomical event times given are for the Traverse City/Interlochen area of Michigan (EDT, UT–4 hours). Times will be different for other locations.

Addendum

A Finder chart for the expected nova
A Finder chart for the expected nova. It should occur shortly in the constellation of Corona Borealis or the Northern Crown. It is designated T Coronae Borealis (T CrB) and it is in the West above the bright star Arcturus which can be found by following the curve of the handle of the Big Dipper. Created using Stellarium, LibreOffice Draw and GIMP.

Ephemeris Extra: 07/02/2024 – A closer look at Corona Borealis

July 2, 2024 Comments off

Adapted from an article that ran in the Stellar Sentinel, the July 2024 newsletter of the Grand Traverse Astronomical Society.

Corona Borealis in relation to some of its neighboring constellations and bright stars. Created using Stellarium.

A small constellation is getting a lot of attention this year because we expect a bright nova to appear in it sometime in the next few months. The constellation is Corona Borealis, the Northern Crown. It is a small constellation between the Boötes and the bright star Arcturus and Hercules, and farther off to the east the bright star Vega. Corona Borealis contains seven stars in the 2/3 circle of stars. Its brightest star is the third star from the right. It’s the second magnitude star called Alphecca. In Arabic, it means The Bright Star of the Broken Ring of Stars, which is a pretty good description of it. It is also known as Gemma though it sounds like a gem in a crown, it actually means blossom which would appear in a floral crown.

In Greek mythology the crown was given to the Princess Ariadne. The story goes like this. During the time of the Minoan civilization on Crete, It was ruled by King Minos, whose daughter was Ariadne. The Minoans apparently had defeated Athens in battle and had extracted tribute from them. That yearly tribute being the sacrifice of the young man or maiden to enter the Labyrinth which was home to a monster called the Minotaur. In this story a fellow by the name of Theseus from Athens was sent to Crete to face the Minotaur. He fell in love with Ariadne, but he had to enter the Labyrinth, so she provided him with a spool of thread so he could find his way back out again after he had slain the Minotaur, if he was able to. He entered the Labyrinth and found the Minotaur. Theseus was able to slay the beast, and was able to follow the thread back out. Theseus and Ariadne fled to the Island of Naxos where he married her. However, he soon abandoned her. As consolation, the god Dionysus gave her a crown. She kept the crown until she remarried, and it was placed in the sky where we see it today.

For the Anishinaabe native peoples of our area Corona Borealis becomes the Sweat Lodge. Other indigenous peoples of North America see these stars as circles of maidens, or other circles. To the Aborigines of Australia who see Corona Borealis very low in the north, it’s Woomera, the boomerang.

The location and expected brightness of T Coronae Borealis (T CrB) when it goes nova later this year.


The constellation has two famous variable stars. The one we’re expecting to flare up this year, up to second magnitude as a nova, is T Coronae Borealis (T CrB), sometimes called the Blaze Star. It was recorded in 1866 and at even earlier times, and was naked eye for eight days, dropping a half magnitude per day. It also blazed forth in 1946, making it one of the few known recurrent novas. In 1946 the star, normally 10th magnitude, barely visible in binoculars, underwent a slight dimming about 11 months before it blazed forth as a nova. This has already happened last year, so we are expecting it soon to blaze forth again. It will appear to the lower left, just outside the circle of stars in the crown, and will grow as bright as Alphecca.

Novas, also in the case of T CrB, are close binary stars containing a large star and a white dwarf. A white dwarf is a star at the end of its life, and has run out of hydrogen or other light elements in its core to keep it sustained. So it shrinks down to about the size of the Earth, even though it has the mass of the Sun or a little more. It orbits with the larger star and is basically siphoning off gas from that large star onto its surface, enough gases accumulate on the star for a thermonuclear reaction to occur, and it becomes a nova, brightening thousands of times for a few days. The white dwarf survives to do it all over again in some cases.

Corona Borealis, pointing out the location of variable stars R CrB and T CrB. Created using Stellarium.

Corona Borealis’ other famous variable star is R Coronae Borealis, a star that’s normally about 6th magnitude that irregularly dips down to 10th or even dimmer. The mechanism for this appears to be that the star is surrounded by clouds of dust that periodically block it from our view.

If you’re interested in observing variable stars, check out the American Association of Variable Star Observers: https://www.aavso.org/

Corona Australis finder
Corona Australis finder chart, for around midnight August 2nd.

If there’s a Northern Crown, there should be a Southern Crown, and there is. It is Corona Australis made of dim stars, and it is located just below the constellation of Sagittarius, right below the Teapot asterism, which is very low on our southern horizon after midnight this month, but better seen in August.

Ephemeris: 06/27/2024 – Why do astronomers think a nova will appear this year?

June 27, 2024 Comments off

This is Ephemeris for Thursday, June 27th. Today the Sun will be up for 15 hours and 33 minutes, setting at 9:32, and it will rise tomorrow at 5:59. The Moon, 1 day before last quarter, will rise at 1:18 tomorrow morning.

Our expected nova this year, T Coronae Borealis, is expected by some astronomers to erupt sometime in September give or take, but nobody knows for sure. The last eruption was seen in 1946. And if the average time between outbursts is 80 years, it seems to be two years early this time. In 1946 there were observations showing that there were some precursor effects going on before the eruption, and those have been noticed this time too, which is which why we assume that the nova will occur this year. Stars that vary in brightness are denoted in a constellation by a letter starting with R through Z, then RR, RS, etcetera through ZZ. After that it’s V and a number plus the constellation name or abbreviation.

The astronomical event times given are for the Traverse City/Interlochen area of Michigan (EDT, UT–4 hours). They may be different for your location.

Addendum

T Coronae Borealis Finder Chart
This animated GIF shows the constellations of Hercules, Corona Borealis and Boötes from left to right. Flashing on and off is T Coronae Borealis (T CrB). It is shown at its approximate maximum brightness, about the same as Alphecca (spelled Alphekka here). Created using Stellarium and GIMP.

Ephemeris: 06/25/2024 – Three kinds of novas

June 25, 2024 Comments off

This is Ephemeris for Tuesday, June 25th. Today the Sun will be up for 15 hours and 33 minutes, setting at 9:32, and it will rise tomorrow at 5:58. The Moon, 3 days before last quarter, will rise at 12:35 tomorrow morning.

As I mentioned yesterday we’re expecting a nova or bright star that we expect to appear sometime this year, maybe in September according to some astronomers. A nova is a rapid brightening of a star due to some cataclysmic event happening to it. There are three kinds that we actually know of. A nova, which is what we’re expecting; a supernova, an explosion maybe a million times greater; and the recently discovered kilonova when two neutron stars collide, which is a thousand or so times brighter than an ordinary nova. A nova and one kind of supernova (Type 1) involve a binary star system which contains a white dwarf star near the end of its life close enough to a larger star to siphon off material. At some point enough has built up and an explosion occurs.

The astronomical event times given are for the Traverse City/Interlochen area of Michigan (EDT, UT–4 hours). They may be different for your location.

Addendum

The second type of Supernova is caused when a supermassive star’s core collapses when it’s made of iron and tries to fuse it into heaver elements. That process takes energy rather than producing it. Oops! The star collapses on itself, and… Kablooey!

Nova in a binary system


A red giant star and white dwarf orbit each other in this animation of a nova similar to T Coronae Borealis. The red giant is a large sphere in shades of red, orange, and white, with the side facing the white dwarf the lightest shades. The white dwarf is hidden in a bright glow of white and yellows, which represent an accretion disk around the star. A stream of material, shown as a diffuse cloud of red, flows from the red giant to the white dwarf. When the red giant moves behind the white dwarf, a nova explosion on the white dwarf ignites, creating a ball of ejected nova material shown in pale orange. After the fog of material clears, a small white spot remains, indicating that the white dwarf has survived the explosion. NASA/Goddard Space Flight Center
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Ephemeris: 06/24/2024 – Waiting for a bright nova*

June 24, 2024 Comments off

This is Ephemeris for Monday, June 24th. Today the Sun will be up for 15 hours and 34 minutes, setting at 9:32, and it will rise tomorrow at 5:58. The Moon, 3 days past full, will rise at 12:09 tomorrow morning.

The small constellation of Corona Borealis, or Northern Crown appears about a third of the way between the bright star Arcturus, high in the south and the star Vega in the east. It is a small semicircle of stars with the brighter star called Alphecca near the center of the arc of stars. Sometime this year, we hope, another bright star will appear there. A nova of a dim star brightening about 1,600 times normal near that circle of stars. It has done it before. It has the designation of T Coronae Borealis (T CrB for short), and is a recurrent nova of a white dwarf star that suffers an explosion about once every 80 years. So this year we need to be looking out for that stellar explosion, which will be bright for only a few days, so one must be vigilant to spot it.

The astronomical event times given are for the Traverse City/Interlochen area of Michigan (EDT, UT–4 hours). They may be different for your location.

* The word ‘nova’ comes from the Latin Nova Stella, meaning New Star.

Addendum

Finding Corona Borealis
Putting Corona Borealis in context with the Big Dipper, to the upper right, looking overhead while facing south, at 11 pm in late June. Created using Stellarium and GIMP.
Showing the location of T Coronae Borealis
This animated GIF shows the constellations of Hercules, Corona Borealis and Boötes from left to right. Flashing on and off is T Coronae Borealis (T CrB). It is shown at its approximate maximum brightness, about the same as Alphecca (spelled Alphekka here). Created using Stellarium and GIMP.
Light curve for Nova Cygni 1975 (V1500 Cyg) which burst forth in the constellation of Cygnus the Swan in August of 1975, just two months after the beginning of the Ephemeris program. There hasn’t been a brighter one since. Notice the initial sharp rise and initial decline. Magnitudes (Mag on the vertical axis) work like golf scores or prizes, the brighter the star the lower the magnitude number. The dimmest star visible to the naked eye is about 6th magnitude. You can blame Hipparchus for that numbering scheme.

NASA has post about T CrB here: https://www.nasa.gov/centers-and-facilities/marshall/nasa-global-astronomers-await-rare-nova-explosion/