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Ephemeris: 09/28/2026 – What happens to the Earth during Autumn

September 28, 2026 Leave a comment

This is Ephemeris for Monday, September 28th. Today the Sun will be up for 11 hours and 51 minutes, setting at 7:28, and it will rise tomorrow at 7:38. The Moon, 2 days past full, will rise at 8:04 this evening.

Autumn is a season of change. The Sun, at noon each day, will not rise as high as the previous day. Sunrises will occur progressively later each day, while the Sun sets progressively earlier. This is not occuring by the earth moving away from the sun giving us colder temporatures. In fact throughout autumn we’re moving slowly closer to the Sun. But the entire yearly range in the sun’s distance change is only 3 million miles out of 93 million. The reason for the change of season is the tilt of the axis of the Earth to its orbital plane around the sun. The axis of the Earth points in a single direction, currently towards the star Polaris, so as the Earth moves around the Sun the Earth’s axis appears to change its orientation with the Sun.

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 diagram of the true shape of the Earth’s orbit and position of the Sun showing aphelion and perihelion, equixoxes and solstices for the year 2026.
A diagram of the true shape of the Earth’s orbit and position of the Sun showing aphelion and perihelion, equixoxes and solstices for the year 2026. The dates do vary by up to a couple of days each year as do the distances a little bit. The date differences for perihelion and aphelion are a bit more than the date change of the solstices and equinoxes from year to year. Created using my LookingUp app, LibreOffice Draw for captions, and GIMP.

Ephemeris: 09/24/2026 – The Harvest Moon Effect

September 24, 2026 Comments off

This is Ephemeris for Thursday, September 24th. Today the Sun will be up for 12 hours and 3 minutes, setting at 7:36, and it will rise tomorrow at 7:33. The Moon, 2 days before full, will set at 6:18 tomorrow morning.

The full, or nearly full moon, just rising, looks like a large orange pumpkin. The color, like the red of the sunset is caused by the scattering out of blue light by the atmosphere. It can happen at any full moon, not just the Harvest Moon, which will occur on Saturday. What the Moon around the Harvest Moon does do is rise only a little later each evening. This helped the farmers in earlier times effectively extend twilight to bring in the crops. On average the moon rises or sets 50 minutes later each night. However when the Moon is in the part of the sky where it is moving northward as well as eastward, then it rises only a little later each night. Tomorrow’s Moon will rise only 19 minutes later than it will this evening.

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 Harvest Moon effect is a phenomenon where the Moon's nightly advance in rising times become much shorter than the average of 50 minutes.
The Harvest Moon effect is a phenomenon where the Moon’s nightly advance in rising times become much shorter than the average of 50 minutes. This has the effect of extending the bright part of twilight for up to a week near the Full Moon. Created using Cartes du Ciel (Sky Charts).

Ephemeris: 09/14/2026 – The young September Moon slowly enters the evening sky

September 14, 2026 Comments off

This is Ephemeris for Monday, September 14th. Today the Sun will be up for 12 hours and 34 minutes, setting at 7:55, and it will rise tomorrow at 7:21. The Moon, half way from new to first quarter, will set at 9:07 this evening.

Something interesting is happening to the moon in late summer and early autumn. The moon, when either near new or near full, tends to hang low near the horizon for a long time. We are now about 4 days past new moon, and it is hanging low in the southwestern sky, and will set only about an hour and 12 minutes after the sun. Later this month we’ll have the Harvest Moon when the moon rises at short daily intervals later each night around full moon. I call it the Harvest Moon effect and that allowed farmers of old together in their crops by extending twilight. What the young moon does right now is keeping it really low in the sky so as a crescent it’s not easy to observe low on the southwestern horizon.

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 diagram that shows why the moon is slow in taking over the evening sky in September after new moon.
This is a diagram that shows why the moon is slow in taking over the evening sky in September after new moon, because its path away from the sun run low near the horizon. What September giveth, September will taketh away. Come near full moon, it will be slow to leave the evening sky. The reason is the ecliptic, at sunset, runs low in the south. At first quarter at or near sunset, the moon is in the south 90 degrees from, and three months later that where the sun is now, which takes us into December which is why the sun is so low in December bringing our winter season. Created using Cartes du Ciel (Sky Charts), with added annotations.

Ephemeris: 09/08/2026 – Where is the Sun heading to?

September 8, 2026 Comments off

This is Ephemeris for Tuesday, September 8th. Today the Sun will be up for 12 hours and 52 minutes, setting at 8:06, and it will rise tomorrow at 7:14. The Moon, 2 days before new, will rise at 5:18 tomorrow morning.

We know that the Earth orbits the sun, but where is the sun going? The sun orbits the center of the Milky Way moving something like 137 miles (220 kilometers) per second in the direction of Cygnus the Swan. It takes about 200 to 250 million years to orbit the center of the galaxy. However, the sun has a motion with respect to the general flow of stars in our neighborhood orbiting the center of the galaxy. Where the sun is heading is it called the solar apex. That point is it just a little bit south of the star Vega which is high in the south in the evening. Vega is the brightest star of this Summer Triangle, which includes Altair to the southeast and Deneb to the east. The sun’s motioned towards the apex that is about 8 miles (13 kilometers) per second.

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 Solar Apex, where the sun is headed.
The Solar Apex, where the sun is headed compared to the cicular orbit around the center of the galaxy. The general circular orbit would point the sun at a point just north of Deneb in our sky at 10 PM on September 8th. The deviation of the apex point shows the sun has a slightly elliptical orbit that bobs above and below the galactic plane. Star field from Stellarium, apex point position from Wikipedia.

Ephemeris: 08/25/2026 – Thursday’s lunar eclipse – and when eclipses can occur

August 25, 2026 Comments off

This is Ephemeris for Tuesday, August 25th. Today the Sun will be up for 13 hours and 34 minutes, setting at 8:31, and it will rise tomorrow at 6:58. The Moon, 3 days before full, will set at 5:06 tomorrow morning.

This Thursday’s partial lunar eclipse will occur only 15 days after the last eclipse, a nibble of a solar eclipse for us, and a total eclipse for others on August 12th. Eclipses occur in seasons of about a month long that occur at a bit less than six month intervals, so eclipses will occur a little earlier next year to this. That’s because the crossing points of the Moon’s and the Earth’s orbital planes regress slowly westward. In an eclipse season two eclipses will occur: a solar and a lunar eclipse. On rare occasions when a lunar eclipse occurs in the center of a season a partial solar eclipse can occur two weeks before and again after the lunar eclipse, but they will affect the opposite polar regions of the Earth. For Thursday night, the partial eclipse will start at 10:34 PM. Maximum eclipse occurs at 12:13 AM, and will end at 1:52 AM.

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

Why there are eclipse seasons, and why they move progressively earlier each year.
Why there are eclipse seasons, and why they move progressively earlier each year. Since the sun has to be within 17 º of a node to be within an eclipse season, and the sun travels about 1º a day, an eclipse season lasts about 34 days, a bit longer than a lunar month of 29½ days. So two eclipses will occur, and possibly three. Whether any are visible depends on one’s location.
Preview of the partial lunar eclipse on the night of August 27-28 2026.
Preview of the partial lunar eclipse on the night of August 27-28 2026. The orientation of the moon and earth’s shadow is that for the naked-eye or binoculars. The motion of the moon in the sky during the eclipse is east to west (left to right) due to the earth’s rotation. However, the moon’s motion against the stars and with the earth’s shadow is west to east (right to left). The times are for the beginning maximum and end of the partial phase. EDT is 4 hours brhind Universal Time. Created using Stellarium.

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.