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Archive for April, 2026

Ephemeris: 04/30/2026 – GTAS meeting tomorrow, The Space Race.

April 30, 2026 Comments off

This is Ephemeris for Thursday, April 30th. Today the Sun will be up for 14 hours and 12 minutes, setting at 8:46, and it will rise tomorrow at 6:32. The Moon, 1 day before full, will set at 6:03 tomorrow morning.

The Grand Traverse Astronomical Society will host its May meeting tomorrow, May 1st at 9 PM at Northwestern Michigan College’s Joseph H Rogers Observatory. The later meeting time through July allows us to have viewing after the meeting start in darker skies. The program is a video called the Space Race. I’m not sure if it was the one 6 decades ago in the 1960s or the current one, which is in doubt. It will be informative either way. Afterward, about 10 PM if it’s clear, there will be viewing of the heavens through the observatory’s telescopes, featuring Jupiter, its cloud bands and moons. The observatory is located on Birmley Rd. South of Traverse City. Also, available on ZOOM, see gtastro.org.

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

Maybe we can contrast the 1960s space race with the 2020s. There are differences on many levels.
Maybe we can contrast the 1960s space race with the 2020s. There are differences on many levels.

Ephemeris: 04/29/2026 – Taking our weekly look at the whereabouts of the naked-eye planets

April 29, 2026 Comments off

This is Ephemeris for Wednesday, April 29th. Today the Sun will be up for 14 hours and 9 minutes, setting at 8:45, and it will rise tomorrow at 6:34. The Moon, 2 days before full, will set at 5:42 tomorrow morning.

Let’s take our weekly look at the whereabouts of the naked-eye planets. By 9:30 PM tonight or about 45 minutes or so after sunset, Venus may be seen very low in the West. A telescope will show a very tiny disc on Venus, because it is still pretty much beyond the Sun, 136 million miles (217 million kilometers) away from us. Over the next 6 months it will be moving closer to us and becoming much larger. Jupiter is the brilliant star-like object in the western before 10 PM. It is above and left of the brighter Venus. Venus will set at 11:11 PM, while Jupiter will hold out until 2:12 AM. Meanwhile, Mercury, Mars and Saturn are breaking up just west of the Sun, but are still overwhelmed by bright morning twilight.

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 west to Jupiter, and Venus with fading winter stars at 9:30 PM tonight, April 29, 2026. Jupiter and Venus are appearing to approach each other. They will be in conjunction on the evening of June 8th.
Jupiter, and Venus with fading winter stars at 9:30 PM tonight, April 29, 2026. Jupiter and Venus are appearing to approach each other. They will be in conjunction on the evening of June 8th. Created using Stellarium.
The Moon, 2 days before full, as seen at 10 PM tonight, April 29, 2026. A view visible in small telescopes showing an image with and without selected features labeled. Created using Stellarium, LibreOffice Draw, and GIMP.
Telescopic Jupiter and Venus as they would be seen in a small telescope with the same magnification.
Telescopic Jupiter and Venus (north up) as they would be seen in a small telescope with the same magnification. Venus will be visible for a short time near the western horizon, while Jupiter will be visible until after midnight. Venus’ apparent diameter will be 11.6″, and be 88.2% illuminated. It’s on the far side of the Sun. Jupiter will be 35.7″ in diameter, with its moons shown here for 10 PM, tonight April 29, 2026. The moons can shift noticably over an hour, especially Io and Europa. The (”) symbol means seconds of arc, or 1/3600th of a degree. Created using Cartes du Ciel (Sky Charts), LibreOffice Draw and GIMP.
The naked-eye planets at sunset and sunrise on a single night.
The naked-eye planets at sunset and sunrise on a single night, starting with sunset on the right on April 29, 2026. The night ends on the left with sunrise on the 30th. Click or tap on the image to enlarge it. Created using my LookingUp app and GIMP.
A low precision ephemeris of the Sun Moon and naked eye planet positions for today and tomorrow, April 29 and 30th, 2026.
This is a low precision ephemeris of the Sun Moon and naked eye planet positions for today and tomorrow, April 29 and 30th, 2026. Some of the columns are self-explanatory, others are not. The transit column is the time that the body crosses the meridian and is due south. Elong, for elongation, is the angle between the Sun and that body. RA is right ascension, which is the object’s east-west position on the celestial sphere in hours and minutes. Dec is declination which is the north-south position of the object on the celestial sphere in degrees and minutes. R is the distance of that object from the Sun in astronomical units. An astronomical unit is about 93 million miles or 150 million kilometers. And Delta is the distance of that object from the Earth, also in astronomical units. I omit the ‘m’ in am and pm for compactness. The data was generated using my LookingUp for DOS app and displayed as a table by my Ephemeris Helper app.

Ephemeris: 04/28/2026 – Stars spend most of their lives fueled by hydrogen

April 28, 2026 Comments off

This is Ephemeris for Tuesday, April 28th. Today the Sun will be up for 14 hours and 7 minutes, setting at 8:44, and it will rise tomorrow at 6:35. The Moon, 3 days before full, will set at 5:24 tomorrow morning.

A star is a gaseous ball made mostly of hydrogen, which due to its mass crushes down in its core to create heat in the millions of degrees. Under those temperatures and pressures hydrogen nuclei, stripped of their electrons can collide to convert into helium and in doing so lose a tiny bit of mass that turns into energy which is used to sustain the star’s light and keep it stable. This hydrogen burning, so to speak, takes place during the longest period of a star’s life. And stars have a characteristic color based on their mass. Stars with little mass are cooler and appear a dim red. We call them red dwarfs. The nearest star to our solar system is a red dwarf called Proxima Centauri. It’s so dim that it’d be difficult to find with a pair of binoculars. And it’s only four light years away.

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

H-R diagram
The Hertzsprung-Russell (H-R) diagram of star luminosity vs. surface temperature. Credit: European Southern Observatory (ESO).

The HR diagram above shows the various types and brightness of stars. The relatively thin line of stars from upper left to lower right, called the main sequence, are stars that are running primarily on hydrogen as a fuel. At the bottom end of the main sequence small stars with a fraction of the sun’s mass. All these stars are near the sun. It doesn’t mean that we live in a bad neighborhood, but that the most numerous stars are red dwarfs, and we just can’t see them when they’re farther away. All the other stars are not using as hydrogen as their main fuel source. Stars the upper right are using heavier elements to produce energy from the fusion products of lighter elements, after having run out of hydrogen in their cores. The white dwarf stars in the lower part of the diagram no longer have active thermonuclear reactions in their cores and are cooling down and collapsing. A star with the mass of the sun, when it becomes a white dwarf, will shrink down to about the size of the earth.

Ephemeris: 04/27/2026 – Mare Orientale made a splash!

April 27, 2026 Comments off

This is Ephemeris for Monday, April 27th. Today the Sun will be up for 14 hours and 4 minutes, setting at 8:42, and it will rise tomorrow at 6:37. The Moon, halfway from first quarter to full, will set at 5:06 tomorrow morning.

One of the pictures that the astronauts of Artemis 2 took of the far side of the moon was one that revealed chains of craters which appear to be emanating from the Sea on the edge of what we can see on the moon from the Earth, called Mare Orientale or the Eastern Sea. It was created by the impact of an asteroid onto the Moon’s surface, maybe 4 billion years ago, kicking out debris in all directions. Apparently the ejecta thrown out created chains of craters that appear to trace back to Orientale. They are most easily seen to the north and west of Orientale towards the terminator, the sunrise line, where the shadows are deeper. There’s probably chains of craters going in other directions, but they have no shadows.

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

Crater chains that can be traced back to Mare Orientale. Credit: NASA/CSA/Artemis II Crew

Ephemeris: 04/24/2026 – Where did the lunar “seas” come from?

April 24, 2026 Comments off

This is Bob Moler with Ephemeris for Arbor Day, Friday, April 24th. Today the Sun will be up for 13 hours and 55 minutes, setting at 8:39, and it will rise tomorrow at 6:41. The Moon, 1 day past first quarter, will set at 4:08 tomorrow morning.

The face of the Moon is a bit more than half uncovered from our point of view, with first quarter occurring yesterday. It shows the string of lunar seas, those gray areas on the Moon which lead to the terminator, the Moon’s sunrise line. There is a larger sea called the Ocean of Storms on the eastern side of the Moon, as we see it. Most were created about 3.8 to 3.9 billion years ago by asteroid strikes. The same collisions happened to the Earth, but plate tectonics destroyed the evidence. Not so on the Moon. Many planetary scientists think it was the result of the Late Heavy Bombardment, caused by the changing orbits of mainly Saturn, Uranus and Neptune disrupting the asteroids, and sending them careening through the solar system.

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

Lunar seas
Lunar seas and their ages. (b.y. = billion years ago) Credit NASA.
Nice model of solar system evolution infographic
Nice model infographic: Evolution of the solar system. Step 6, with the exchange of Neptune’s and Uranus’ orbits, cause the Late Heavy Bombardment. The Nice model isn’t that nice. It’s named for Nice, France, the city where the model was first developed. Click or tap on the image to enlarge it. Credit: Nora Eisner

Ephemeris: 04/23/2026 – Where did the Moon come from?

April 23, 2026 Comments off

This is Ephemeris for Thursday, April 23rd. Today the Sun will be up for 13 hours and 52 minutes, setting at 8:37, and it will rise tomorrow at 6:43. The Moon, at first quarter today, will set at 3:42 tomorrow morning.

When one gazes upon the moon tonight the thought of where the moon came from might come to mind. Did it form with the Earth? Was it captured by the Earth? The latest thinking on the origin of the moon centers around a grazing collision with the Earth of a Mars sized body that has been given the name Theia, the mother of Selene, the goddess of the Moon, shortly after the Earth was formed. This is based on Apollo mission discoveries that the composition of the rocks on the moon are approximately the same as those of Earth’s crust. It’s been known for a while that there are two dense masses within the Earth about halfway to the center. One geologist has put forth that these masses could have been the core of Theia that sank into the Earth.

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

Collision spawning the Moon
The hypothetical collision of a Mars sized body with the young Earth. Credit: Joe Tucciarone via NASA
New moon formation
A new simulation on how the Moon formed. Credit: PBS.
Categories: Ephemeris Program, Origins Tags: , ,

Ephemeris: 04/22/2026 – Taking our weekly look at the whereabouts of the naked-eye planets

April 22, 2026 Comments off

This is Ephemeris for Earth Day, Wednesday, April 22nd. Today the Sun will be up for 13 hours and 50 minutes, setting at 8:36, and it will rise tomorrow at 6:45. The Moon, 1 day before first quarter, will set at 3:07 tomorrow morning.

Let’s take our weekly look at the whereabouts of the naked-eye planets. By 9 PM tonight or about 30 minutes or so after sunset, Venus may be seen very low in the West. A telescope will show a very tiny disc on Venus, because it is still pretty much beyond the Sun, 138 million miles (222 million kilometers) away from us. Over the next 6 months it will be moving closer to us and becoming much larger. Jupiter is the brilliant star-like object high in the west-southwestern sky before 10 PM. It will appear just below the crescent Moon tonight. Venus will set at 10:54, while Jupiter will hold out until 2:30 AM. Meanwhile, Mercury, Mars and Saturn are still bunched up just west of the Sun, but are overwhelmed by bright morning twilight.

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

Jupiter, and Venus with the Moon and Sirius at 9 PM tonight.
Jupiter, and Venus with the Moon and Sirius at 9 PM tonight, April 22, 2026. Created using Stellarium.
A closer look at Jupiter and the Moon at 9 PM tonight.
A closer look at Jupiter and the Moon at 9 PM tonight, April 22, 2026. Created using Stellarium.
The Moon, a day before first quarter, as seen at 9:30 PM tonight, April 22, 2026. A view visible in small telescopes showing an image with and without selected features labeled. Created using Stellarium, LibreOffice Draw, and GIMP.
Telescopic Jupiter and Venus (north up) as they would be seen in a small telescope with the same magnification.
Telescopic Jupiter and Venus (north up) as they would be seen in a small telescope with the same magnification. Venus will be visible for a short time near the western horizon, while Jupiter is visible most of the night. Venus’ apparent diameter will be 11.3″, and be 89.7% illuminated. It’s on the far side of the Sun, 1.5 times the Sun’s distance from us. Jupiter will be 36.4″ in diameter, with its moons shown here for 9:30 PM, tonight April 22, 2026. The moons can shift noticably over an hour, especially Io and Europa. The (”) symbol means seconds of arc, or 1/3600th of a degree. Created using Cartes du Ciel (Sky Charts), LibreOffice Draw and GIMP.
The naked-eye planets at sunset and sunrise on a single night, starting with sunset on the right on April 22, 2026. The night ends on the left with sunrise on the 22nd.
The naked-eye planets at sunset and sunrise on a single night, starting with sunset on the right on April 22, 2026. The night ends on the left with sunrise on the 22nd. Click or tap on the image to enlarge it. Created using my LookingUp app and GIMP.
A low precision ephemeris of the Sun Moon and naked eye planet positions for today and tomorrow.
This is a low precision ephemeris of the Sun Moon and naked eye planet positions for today and tomorrow, April 22 and 23rd, 2026. Some of the columns are self-explanatory, others are not. The transit column is the time that the body crosses the meridian and is due south. Elong, for elongation, is the angle between the Sun and that body. RA is right ascension, which is the object’s east-west position on the celestial sphere in hours and minutes. Dec is declination which is the north-south position of the object on the celestial sphere in degrees and minutes. R is the distance of that object from the Sun in astronomical units. An astronomical unit is about 93 million miles or 150 million kilometers. And Delta is the distance of that object from the Earth, also in astronomical units. I omit the ‘m’ in am and pm for compactness. The data was generated using my LookingUp for DOS app and displayed as a table by my Ephemeris Helper app.

Ephemeris: 04/21/2026 – The Lyrid meteor shower reaches its peak tomorrow

April 21, 2026 Comments off

This is Ephemeris for Tuesday, April 21st. Today the Sun will be up for 13 hours and 47 minutes, setting at 8:35, and it will rise tomorrow at 6:46. The Moon, 2 days before first quarter, will set at 2:21 tomorrow morning.

The second major meteor shower this year will reach its peak tomorrow afternoon around 3 PM (~19h UT). The best time to see it will be tomorrow morning after moonset at 2:21 AM. Astronomical twilight will begin to interfere after 5 AM. The other is tomorrow night starting 45 minutes later. The meteor shower is called the Lyrids, because they seem to come from near the constellation Lyra the harp and the bright star Vega. By 3 AM Vega will be high in the east. The radiant of the meteors is to the west of Vega, between Lyra and the dim constellation of Hercules. Though a major shower, the peak hourly rate is expected to be about 20 meteors an hour.

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

Lyrid meteor radiant.
Lyrid meteor radiant (LyrR) is near Lyra and the bright star Vega. The bright star by “Lyr” is Vega. Create by my LookingUp app.

Ephemeris: 04/20/2026 – A seeming convergence of planets too close to the Sun to be seen from Michigan

April 20, 2026 Comments off

This is Ephemeris for Monday, April 20th. Today the Sun will be up for 13 hours and 44 minutes, setting at 8:34, and it will rise tomorrow at 6:48. The Moon, halfway from new to first quarter, will set at 1:20 tomorrow morning.

There’s a close planetary alignment this happening and today in the morning sky that we can’t see, of Mercury Mars and Saturn which are too close to the sun, and the time of year is not the best for seeing them. So they’re invisible to us but visible for folks in the Southern Hemisphere. Even the Artemis 2 astronauts talked about them when they went into solar eclipse on their trip around the moon. But the action is all happening yesterday and today. As of last Friday they were, from left to right, Saturn Mars and Mercury. As of today it’s almost a vertical arrangement with Mars on top Saturn in the middle and Mercury on the bottom and by tomorrow it will be Mercury on the bottom Venus on the top and Saturn off to the right.

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

The apparent convergence of three naked eye planets.
The apparent convergence of three naked eye planets which are invisible from our location in Northern Michigan, as being too close to the Sun and lost in morning twilight. Folks in the Southern Hemisphere may get a better view of it. This animation steps from April 16th through the 22nd at one day intervals, centered on Mars, as the planets Saturn and Mercury slowly switch places with respect to it. This image has an equatorial orientation with north directly up and west to the right. The orientation in the sky will be tilted about 45° to the left. Created using Stellarium and GIMP.

Ephemeris: 04/17/2026 – The Moon’s Far Side isn’t dark!

April 17, 2026 Comments off

This is Bob Moler with Ephemeris for Friday, April 17th. Today the Sun will be up for 13 hours and 35 minutes, setting at 8:30, and it will rise tomorrow at 6:53. The Moon is new today, and won’t be visible.

When I hear discussions about the Artemis 2 missions, some people who ought to know better still refer to the far side of the moon as the dark side. Officially we have the two faces of the moon: the near side and the far side. I’ll even accept front side and back side. Until 1959 no one had ever seen the far side of the moon so it was dark, in the sense that we could not see it. Not dark because of the lack of light. I’ve been thinking about it. The far side sees more light from the sun, so maybe we should call it the bright side. It certainly has fewer maria or seas, those dark patches that we see on the near side of the Moon. There’s only one on the far side, it’s called the Moscow Sea since the Russian spotted first. Mare Orientale, subject of much study by the Artemis 2 crew, straddles the near side-far side line. It’s closer to the sun when it’s fully illuminated than the near side by about half a million miles, and it doesn’t suffer solar eclipses to darken it like the near side, being already in night, like it always is, at full moon.

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

Photograph of the crescent Earth setting behind the limb of the Moon by the Artemis 2 crew.
The far side may seem to be the dark side in this photograph of earthset by the Artemis 2 crew. It is as bright as the brightest parts of the near side. These are the crater filled highlands, so it is the exact same brightness as the highlands on the near side. And indeed in traveling to the Moon, when it was seen half near side and half far side, there was no difference in the brightness of the highlands between the two. So the moon is really dark gray in brightness, on average. It reflects something like 12% of the sunlight it receives, while the earth is more than twice that reflectance. Astronomers call that quantity albedo. So the Moon has an albedo of 12% while the Earth has an albedo of something like 29% on average. So the reason the full moon is so bright at night is due to lack of competition from something that’s actually much whiter. Credit: NASA/ESA/CSA -The Artemis 2 crew.