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Ephemeris: 08/03/2026 – The Milky Way, a spiral galaxy with a bar

August 3, 2026 Comments off
A somewhat dipalidated drinking establishment with the neon sign stating "Galaxy Bar".
Not this kind of bar. See below. Generated by Google Gemini AI.

This is Ephemeris for Monday, August 3rd. Today the Sun will be up for 14 hours and 34 minutes, setting at 9:05, and it will rise tomorrow at 6:32. The Moon, 2 days before last quarter, will rise at 11:07 this evening.

The Milky Way is classed as a barred spiral galaxy. It has an apparent spiral structure in its disk illuminated by bright massive short lived stars that don’t stray far from the nebulae they were born from. Nebulae, mostly dark, form the backbone of the spiral structure. The Andromeda Galaxy is also a spiral, a little larger than our Milky Way Galaxy. Dwarf galaxies like the Magellanic clouds which are seen from the southern hemisphere of the earth that happen to be satellites of the Milky Way, and are irregular in shape. A third type of galaxy is the elliptical galaxy, many of which are extremely large and contain pretty much nothing but old stars, and no nebulosity to make new ones.

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

Artist's conception of the Milky Way. From NASA/JPL/Spitzer/Cal Tech
Artist’s conception of the Milky Way. From NASA/JPL/Spitzer/Cal Tech
The Magellanic Clouds
The Small and Large Magellanic Clouds, these dwarf galaxies are seen best from the southern hemisphere. Credit: ESO S. Brunier.
Different types of galaxies.
Different types of galaxies. The lenticular type are thought to be intermediate between elliptical and spiral.
Categories: Concepts, Galaxies

Ephemeris: 07/30/2026 – The types and distribution of galaxies

July 30, 2026 Comments off

This is Ephemeris for Thursday, July 30th. Today the Sun will be up for 14 hours and 44 minutes, setting at 9:10, and it will rise tomorrow at 6:27. The Moon, 1 day past full, will rise at 9:52 this evening.

Until a little over 100 years ago the Milky Way was thought to be the whole universe. Then with photography the great Andromeda nebula turned out to be not a cloud of gas but a great group of stars outside. Since then we have found billions upon billions of these galaxies. Galaxy simply is a derivation from “Milky Way” in Latin. Galaxies are not sprinkled through the universe uniformly. They appear in great clusters and in small groups. The Milky Way and the Andromeda Galaxy belong to a relatively small group of galaxies called the Local Group, which contains 130 or more, mostly dwarf galaxies of which Andromeda and our Milky Way are the largest. The Great Andromeda Galaxy will come in view into the evening sky this autumn.

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

Different types of galaxies.
Different types of galaxies. The lenticular type, not mentioned in the program, are thought to be intermediate between elliptical and spiral.
A panchromatic view of galaxy cluster MACS0416
This panchromatic view of galaxy cluster MACS0416 was created by combining infrared observations from the NASA/ESA/CSA James Webb Space Telescope with visible-light data from the NASA/ESA Hubble Space Telescope. The larger, yellowish galaxies belong to the galaxy cluster in the foreground. The reddish galaxies are more distant. The thin arcs are also distant galaxies, whose images ares deformed by gravitationsl lensing caused by the foreground cluster.

Ephemeris: 07/28/2026 – The size and shape of the Milky Way

July 28, 2026 Comments off

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This is Ephemeris for Tuesday, July 28th. Today the Sun will be up for 14 hours and 48 minutes, setting at 9:13, and it will rise tomorrow at 6:25. The Moon, 1 day before full, will set at 6:11 tomorrow morning.

August and September are the two months in which the Milky Way dominates the evening sky. It also dominates the sky in the winter, six months from now but we’re looking out away from the center of the Milky Way. It is dimmer, an almost invisible as a band, but we have a great number of really bright stars, including those of Orion. The Milky Way is a galaxy, a large conglomeration of stars that are arranged in a disk, with the central bulge, whose diameter is about 87,400 light years. The thickness of the disk runs from 8,500 light years near the center to 1,000 light years farther out. The sun’s location is 25 to 26,000 light years from the center. From our location within the disk it appears to be a glowing band that surrounds the sky.

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

Artist's conception of the Milky Way. From NASA/JPL/Spitzer/Cal Tech
Artist’s conception of the Milky Way. Credit: NASA/JPL/Spitzer/Cal Tech
The summer and winter Milky Way viewing directions.
The summer and winter Milky Way viewing directions. During Spring and Autumn, we look out the sides to the universe beyond. Credit Credit: NASA with annotations by Bob King at Universe Today.
The span of the Milky Way across the summer sky
The span of the Milky Way across the summer sky as seen in the free Stellarium app. Specifically August 15th at 10 pm from Northern Michigan. The Milky Way has been set to its maximum brightness to show as much detail as possible. It really isn’t that bright. The horizon is only delineated by the compass points. The dark clouds of the Great Rift are also visible. The Milky Way, in Stellarium, is photo-realistic. The triangle of three bright stars above center is the Summer Triangle, Specifically, clockwise from the top star: Vega, Altair and Deneb. Large images can be truncated on the right. Click or tap on the image to enlarge and display the complete image.

Ephemeris: 07/24/2026 – AI, a paradigm shift in computing

July 24, 2026 Comments off

This is Ephemeris for Friday, July 24th. Today the Sun will be up for 14 hours and 57 minutes, setting at 9:17, and it will rise tomorrow at 6:21. The Moon, 3 days past first quarter, will set at 2:15 tomorrow morning.

Astronomy is my hobby. Back in my working days I was a computer systems analyst designing computer software systems for particular tasks, mainly for banks. However I was always interested in the idea of artificial intelligence. The computers I worked with were dumb. They did exactly what you told it to do, whether it was correct or not. So computer errors were really human errors. The current AI, based on neural networks, which are an approximation of what happens in the human brain, are different. Their errors are their own, because they are taught rather than programmed. And to my mind are more than the sum of their inputs. Even the people who design these systems admit they don’t really know what goes on inside. Scary.

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.

A visualization of a neural network, capturing the complex flow of information as it travels through interconnected layers and nodes to process data. Currently, neural networks are simulated by software. Hardware implimenations are currently being perfected, which could lower the power consumption of AI models.  Created by Google's Gemini AI.
A visualization of a neural network, capturing the complex flow of information as it travels through interconnected layers and nodes to process data. Currently, neural networks are simulated by software. Hardware implimenations are currently being perfected, which could lower the power consumption of AI models. Created by Google’s Gemini AI.

Ephemeris: 07/23/2026 – Our location in the Eastern Time zone

July 23, 2026 Comments off

This is Ephemeris for Thursday, July 23rd. Today the Sun will be up for 14 hours and 59 minutes, setting at 9:18, and it will rise tomorrow at 6:20. The Moon, 2 days past first quarter, will set at 1:36 tomorrow morning.

Continuing my discussion about daylight savings time: In theory time zones are supposed to be centered on longitude meridians 15º apart, starting at 0° through Greenwich Observatory in England and proceed eastward and westward. our time meridian for Standard Time (75º west longitude) runs through Philadelphia, Pennsylvania, far to the east. The central standard time meridian runs down just east of Ironwood, Michigan. Most of us in the western lower peninsula are between 85 and 86° west longitude, meaning that we are already from 40 to 45 minutes behind our time meridian in Philadelphia and Eastern Daylight Time we are an hour and 40 to 45 minutes behind our daylight time meridian which is out in the Atlantic Ocean at 60° west longitude.

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

US time zone map for daylight saving time.
US time zone map for daylight saving time. I’ve added the approximate locations of the time meridians where, under standard time, the sun averages being due south at noon. there was not room for the EDT/AST meridian. It does touch the eastern end of Nova Scotia. Map credit: nist.gov.

Ephemeris: 07/06/2026 – The Sun is farthest away from Earth today!

July 6, 2026 Comments off

This is Bob Moler with Ephemeris for Monday, July 6th. Today the sun will be up for 15 hours and 26 minutes, setting at 9:30, and it will rise tomorrow at 6:05. The Moon, 1 day before last quarter, will rise at 12:42 tomorrow morning.

Today at 10:59 AM the Earth reaches aphelion from the Sun, the farthest it gets from it during the year. Earth will be 94 and a half million miles away from the Sun, a bit farther than our normal 93 million. In a planet’s orbit of the Sun, the Earth is no exception; it moves slowest when farthest from the Sun than when it’s closer, and fastest when at perihelion, its closest. It doesn’t make much difference in the amount of heat we get from the Sun being only 1½% farther than average. But it makes summer the longest season at 94 days, versus winter’s 89 days. OK, I know it doesn’t feel like it here in Northern Michigan, but count the days between each solstice and the next equinox.

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

A highly exaggerated look at the orbit of the Earth showing perihelion and aphelion, also the equinoxes and solstices and the relation thereof.
A highly exaggerated look at the orbit of the Earth showing perihelion and aphelion, also the equinoxes and solstices and the relation thereof. Periapsis and apoapsis are general terms, for any orbit. For a satellite orbiting the Earth the terms would be perigee and apogee. Source unknown.
This is a diagram of the true shape of the Earth’s orbit
This is a diagram of the true shape of the Earth’s orbit and position of the Sun showing aphelion and perihelion for the year 2024. The dates do vary by up to a couple of days each year as do the distances a little bit. The date range is a bit more than the date range of the solstices and equinoxes year to year. Created using my LookingUp app, LibreOffice Draw for captions, and GIMP.
Categories: Concepts, Ephemeris Program Tags:

Ephemeris: 06/29/2026 – Red stars large and small

June 29, 2026 Comments off

This is Ephemeris for Monday, June 29th. Today the Sun will be up for 15 hours and 32 minutes, setting at 9:32, and it will rise tomorrow at 6:00. The Moon, at full today, will rise at 9:53 this evening.

There are two kinds of red stars very bright ones and very dim ones. The bright red ones are very few. One of them in the evening sky now is Antares in the heart of Scorpius the scorpion. Another one is in the winter sky and the most famous red giant of all, Betelgeuse in the shoulder of Orion the hunter. These are giant stars have exhausted the hydrogen in their cores to produce helium and are working on helium or even heavier elements fusing them to still heavier elements at even higher temperatures to keep them alive, but since they are working on the ash of the previous reaction, they won’t last very long, and the star dies, possibly cataclysmically. The higher internal heat bloats the star to be, huge, making its outer layers are actually cooler.

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

Size comparison between the Sun and two famous red giant stars.
Size comparison between the Sun and two famous red giant stars. However, believe the numbers, not the image size comparisons, which are not to scale and actually too small.
Graphic of the Sun and Barnard's Star.
Graphic of the Sun and Barnard’s Star. Until we found a planet in the habitable zone of Proxima Centauri, the nearest star to the Sun, Barnard’s Star was the most famous red dwarf star. Bernard’s star’s claim to fame that is it has the fastest proper motion of any known star, mainly because it’s only 6 light years away. Proper motion is the apparent star’s motion against more distant stars. In 1916 E. E. Barnard discovered it above the right shoulder of the constellation Ophiuchus the serpent bearer. It moves at a rate of 10.3 arcseconds per year that is 10.3/3600ths of a degree. It can only be seen in a telescope.

Ephemeris: 06/26/2026 – How do we know so much about those points of lights in the sky?

June 26, 2026 Comments off

This is Ephemeris for Friday, June 26th. 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, 3 days before full, will set at 3:37 tomorrow morning.

All but a handful of stars are mere points in even our largest telescopes. How do we know so much about them then? The reason is the science of spectroscopy, breaking down light into its constituent colors where color equals frequency or the energy of the light. Isaac Newton was the first to discover that by passing white light through a prism it turned into a rainbow of colors that the colors were actually combined within the white light. Passing sunlight through a vertical slit and smearing the light horizontally with the prism into its constituent colors, many dark vertical lines within that spectrum of colors appear. They turned out to be the fingerprints of the elements within the atmospheres of the stars, and that is just the beginning.

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 visible solar spectrum. In 1814 Joseph von Fraunhofer observed the spectrum and labeled the dark lines on it.
This is the visible solar spectrum. In 1814 Joseph von Fraunhofer observed the spectrum and labeled these lines with the letters that you see on top . These lines are the most prominent lines of the solar spectrum. There are many more for all the elements in the sun’s atmosphere. These elements absorb light of specific wavelengths coming to us and remit it in all directions, so we have a net loss. The lines are actually the images of the slit that the light went through, or in this case didn’t go through so they imprint on the spectrum as a line. The bottom scale is the wavelength in nanometers (billionths of a meter).

Ephemeris: 06/25/2026 – The color of stars

June 25, 2026 Comments off

This is Ephemeris for Thursday, June 25th. 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, halfway from first quarter to full, will set at 3:03 tomorrow morning.

Looking out at the night sky casually, the first impression is that the stars all appear to be white. Closer inspection shows that some appear with tinges of red or orange or maybe yellow while other stars have a bluish cast to them. The color of stars is due to their surface temperature which physicists call black body radiation. A rainbow is a spectrum of colors from red through orange yellow green blue and violet. These colors represent the different wavelengths of light. The peak wavelength determines the star’s surface temperature. The Sun’s in the green in the middle of our visual field. Cooler stars have their peak in the red, while hotter stars have their peak output to the blue end of the spectrum.

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 curved lines are the black body emission curves of these three particular stars the blue one the yellow one and the red one. The peak of each moves farther into the blue as the surface temperature of the star increases.
The curved lines are the black body emission curves of these three particular stars the blue one the yellow one and the red one. The peak of each moves farther into the blue as the surface temperature of the star increases. The temperature is in Kelvins. Think Celsius. Multiply by 2 (1.9 if you’re picky) to get the approximate temperature in Fahrenheit.
The spectral class of the star is determined by its surface temperature which is shown by its color.
The spectral class of the star is determined by its surface temperature which is shown by its color. The alphabetical classes used to be in alphabetical order by the strength of the hydrogen absorption lines in their spectrum. This turned out to be not useful. So about to turn it the last century Annie Jump Cannon, a Harvard College Observatory human “computer”, and an expert in determining spectral classes of stars, had them rearranged in this particular order by color. She even made-up a mnemonic to remember the order. It was “Oh Be A Fine Girl, Kiss Me”. Of course nowadays you could substitute guy for girl.
Annie Jump Cannon (1863-1941)
Annie Jump Cannon (1863-1941)

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.