Monday, July 29, 2024

Nova Explosion Seen w/out Telescope Due by End of Year

 A 'new' star will light up the sky soon and you can see it for yourself ...

                Artist's concept of a Red Giant Star and a White Dwarf Star, that causes a Nova.

                                (Image Source: Goddard Space Flight Center, NASA)

By Glenn A. Walsh

Reporting for SpaceWatchtower

The year 2024 continues to be a great year for citizen stargazers. On April 8, millions of people saw a Solar Eclipse, many of them viewing the Total Solar Eclipse. And, just a month later, the Sun, again, assisted in allowing many people to see, for the first time, the Northern Lights or Aurora Borealis in southern latitudes where this atmospheric phenomenon is rarely seen. Near the end of this blog-post are Internet links to blog-posts specifically on these two events, including many photographs of the events.

Now NASA has announced that a rare Nova, a star which explodes in brightness on a recurring basis, should be visible without the need of a telescope or binoculars later this year --- perhaps as early as September.

A White Dwarf Star, the collapsed and dead remnant of a star that is now about the size of the Earth but the mass of our Sun, in a star system known as T Coronae Borealis (nicknamed the 'Blaze Star'; astronomical designation: T CrB) is presently too dim to see with the unaided eye (Apparent Visual Magnitude of +10), but should be visible without the need of a telescope or binoculars (one-power) when it becomes a Nova.

This White Dwarf Star is located in the constellation Corona Borealis, the Northern Crown of our Milky Way Galaxy. This constellation can be seen in a distinctive “C” shape, primarily in the Spring and Summer months (best viewed in July), about half-way between the stars Arcturus and Vega, two of the brightest stars in the night sky of the Northern Hemisphere.

If you find the stars Arcturus and Vega, the constellation Corona Borealis is located almost exactly in the middle between the two bright stars. Sky-gazing apps on your smart-phone could help to find this constellation.

While you will need a dark sky to see this constellation, the Nova should be visible in the night sky without the need of a telescope or binoculars. When the Nova does occur, the brightness will jump to approximately a similar Apparent Visual Magnitude as that of the star Polaris, currently our North Star or Pole Star (Apparent Visual Magnitude of Polaris: +1.86 to +2.13).

Once the Nova does occur, it should be visible without the need of a telescope or binoculars for a few days, as well as being visible in binoculars and a telescope for a little more than one week. So, there should be one or more good-weather days to see this Nova.

The T Coronae Borealis binary star system of a White Dwarf Star and an ancient Red Giant Star is located about 3,000 light-years away from the Earth, one of the closest Nova stars to our planet. This means that when the Nova explosion is visible here on Earth, that Nova explosion would have actually occurred 3,000 years ago!

Due to the great distance to this star system, do not expect to see an explosion like you might see on television or in motion pictures. Once the Nova occurs, it will start as a dim star and over the next day or so will slowly brighten.

Many people may have heard of a Supernova, the massive explosion of a dying star, which destroys the star and violently ejects many elements, particularly the heavy elements that will help build future stars and planets. A Supernova is the largest explosion ever seen by human beings. In the year A.D. 1054, Chinese astronomers witnessed a Supernova, which they called a “Guest Star”. Today, the debris from SN 1054 can be viewed in the night sky as the Crab Nebula.

In the case of a Nova, when the star explodes it does not destroy itself. A Nova consists of a White Dwarf Star which uses its massive gravitational pull to take a stream of material from a dying, companion, Red Giant Star. As the White Dwarf Star accumulates material from the Red Giant Star, the massive heat and pressure creates a run-away thermonuclear reaction resulting in the White Dwarf Star having a Nova explosion.

However, this explosion does not destroy the White Dwarf Star. In fact, such a Nova explosion comes in cycles. This is how NASA and astronomers can predict approximately when each Nova explosion will occur.

However, unlike a Solar Eclipse, scientists cannot predict the exact date or time of a Nova. So, you need to pay attention to the news media (newspapers, radio, television, and the Internet) over the next several months, particularly astronomy and science media and web-sites, to be alert to when the Nova occurs. When the Nova does occur, SpaceWatchtower will announce the Nova occurrence on the SpaceWatchtower 'X' / Twitter News-Feed (Internet link to this 'X' / Twitter News-Feed near the end of this blog-post).

It was in February of 2016 that astronomers announced that T Coronae Borealis had entered a “phase of unprecedented high activity” that would lead to a Nova. The star began to dim in March of last year, a precursor to going Nova. Hence, scientists predicted that the Nova would probably occur between June and September of this year, but it could occur later in the year.

Recurrent novae are unpredictable and contrarian,” said Dr. Koji Mukai, a fellow astrophysics researcher at NASA's Goddard Space Flight Center in Greenbelt, Maryland, a suburb of Washington DC. “When you think there can’t possibly be a reason they follow a certain set pattern, they do – and as soon as you start to rely on them repeating the same pattern, they deviate from it completely. We’ll see how T CrB behaves.”

The T Coronae Borealis White Dwarf Star recurrent Nova (recurring approximately once every 80 years) last had a Nova explosion in 1946. This Nova was discovered in 1866, but has been observed as early as 1217 (when it was recorded as a star by a German monk named Abbott Burchard, according to NASA) and 1787 simply as a star with a brightness of 10th magnitude.

In Latin, Nova simply translates as 'new'. Hence, when the ancient peoples saw a bright new star in a location where no star had previously been observed (as Galileo Galilei did not invent the astronomical telescope until 1609), they called it a Nova.

Novae (plural of Nova) are rare. In fact, there are only ten located within our Milky Way Galaxy, according to William J. Cooke from NASA's Meteoroid Environments Office.

Internet Links to Additional Information ---

Nova: Link >>> https://en.wikipedia.org/wiki/Nova

T Coronae Borealis (Blaze Star): Link >>> https://en.wikipedia.org/wiki/T_Coronae_Borealis

Science Experiments Children & Teens Can Do At Home During Summer Break !

Relsted Blog-Posts ---

"Photos: Total Solar Eclipse Viewed in Cleveland." Sat., 2024 June 8.


"Northern Lights Seen in Pittsburgh." Wed., 2024 May 15.

Source: Glenn A. Walsh Reporting for SpaceWatchtower, a project of Friends of the Zeiss     

               "Once-in-Lifetime Bright Nova Star Visible W/Out Telescope by End of Year"

                  Monday, 2024 July 22.

            Artificial Intelligence not used in the writing or production of this article.

            © Copyright 2024 Glenn A. Walsh, All Rights Reserved

                             Like This Post? Please Share!

More Astronomy & Science News - SpaceWatchtower 'X' / Twitter News-Feed:
Link >>> https://twitter.com/spacewatchtower

Astronomy & Science Links: Link >>> http://buhlplanetarium.tripod.com/#sciencelinks

Want to receive SpaceWatchtower blog posts in your in-box ?
Send request to < spacewatchtower@planetarium.cc >.

gaw

Glenn A. Walsh, Informal Science Educator & Communicator                                                             (For more than 50 years! - Since Monday Morning, 1972 June 12):
Link >>> http://buhlplanetarium2.tripod.com/weblog/spacewatchtower/gaw/
Electronic Mail: < gawalsh@planetarium.cc >
Project Director, Friends of the Zeiss: Link >>> http://buhlplanetarium.tripod.com/fotz/
SpaceWatchtower Editor / Author: Link >>> http://spacewatchtower.blogspot.com/
Formerly Astronomical Observatory Coordinator & Planetarium Lecturer, original Buhl Planetarium & Institute of Popular Science (a.k.a. Buhl Science Center), America's fifth major planetarium and Pittsburgh's science & technology museum from 1939 to 1991.
Formerly Trustee, Andrew Carnegie Free Library and Music Hall, Pittsburgh suburb of Carnegie, Pennsylvania, the fourth of only five libraries where both construction and endowment funded by famous industrialist & philanthropist Andrew Carnegie.
Author of History Web Sites on the Internet --
* Buhl Planetarium, Pittsburgh: Link >>> http://www.planetarium.cc Buhl Observatory: Link >>> http://spacewatchtower.blogspot.com/2016/11/75th-anniversary-americas-5th-public.html
* Adler Planetarium, Chicago: Link >>> http://adlerplanetarium.tripod.com
* Astronomer, Educator, Optician John A. Brashear: Link >>> http://johnbrashear.tripod.com
* Andrew Carnegie & Carnegie Libraries: Link >>> http://www.andrewcarnegie.cc

 * Other Walsh-Authored Blog & Web-Sites: Link >>> https://buhlplanetarium.tripod.com/gawweb.html

Monday, July 22, 2024

Once-in-Lifetime Bright Nova Star Visible W/Out Telescope by End of Year

             A 'new' star will light up the sky soon and you can see it for yourself ...

                Artist's concept of a Red Giant Star and a White Dwarf Star, that causes a Nova.

                                (Image Source: Goddard Space Flight Center, NASA)

By Glenn A. Walsh

Reporting for SpaceWatchtower

The year 2024 continues to be a great year for citizen stargazers. On April 8, millions of people saw a Solar Eclipse, many of them viewing the Total Solar Eclipse. And, just a month later, the Sun, again, assisted in allowing many people to see, for the first time, the Northern Lights or Aurora Borealis in southern latitudes where this atmospheric phenomenon is rarely seen. Near the end of this blog-post are Internet links to blog-posts specifically on these two events, including many photographs of the events.

Now NASA has announced that a rare Nova, a star which explodes in brightness on a recurring basis, should be visible without the need of a telescope or binoculars later this year --- perhaps as early as September.

A White Dwarf Star, the collapsed and dead remnant of a star that is now about the size of the Earth but the mass of our Sun, in a star system known as T Coronae Borealis (nicknamed the 'Blaze Star'; astronomical designation: T CrB) is presently too dim to see with the unaided eye (Apparent Visual Magnitude of +10), but should be visible without the need of a telescope or binoculars (one-power) when it becomes a Nova.

This White Dwarf Star is located in the constellation Corona Borealis, the Northern Crown of our Milky Way Galaxy. This constellation can be seen in a distinctive “C” shape, primarily in the Spring and Summer months (best viewed in July), about half-way between the stars Arcturus and Vega, two of the brightest stars in the night sky of the Northern Hemisphere.

If you find the stars Arcturus and Vega, the constellation Corona Borealis is located almost exactly in the middle between the two bright stars. Sky-gazing apps on your smart-phone could help to find this constellation.

While you will need a dark sky to see this constellation, the Nova should be visible in the night sky without the need of a telescope or binoculars. When the Nova does occur, the brightness will jump to approximately a similar Apparent Visual Magnitude as that of the star Polaris, currently our North Star or Pole Star (Apparent Visual Magnitude of Polaris: +1.86 to +2.13).

Once the Nova does occur, it should be visible without the need of a telescope or binoculars for a few days, as well as being visible in binoculars and a telescope for a little more than one week. So, there should be one or more good-weather days to see this Nova.

The T Coronae Borealis binary star system of a White Dwarf Star and an ancient Red Giant Star is located about 3,000 light-years away from the Earth, one of the closest Nova stars to our planet. This means that when the Nova explosion is visible here on Earth, that Nova explosion would have actually occurred 3,000 years ago!

Due to the great distance to this star system, do not expect to see an explosion like you might see on television or in motion pictures. Once the Nova occurs, it will start as a dim star and over the next day or so will slowly brighten.

Many people may have heard of a Supernova, the massive explosion of a dying star, which destroys the star and violently ejects many elements, particularly the heavy elements that will help build future stars and planets. A Supernova is the largest explosion ever seen by human beings. In the year A.D. 1054, Chinese astronomers witnessed a Supernova, which they called a “Guest Star”. Today, the debris from SN 1054 can be viewed in the night sky as the Crab Nebula.

In the case of a Nova, when the star explodes it does not destroy itself. A Nova consists of a White Dwarf Star which uses its massive gravitational pull to take a stream of material from a dying, companion, Red Giant Star. As the White Dwarf Star accumulates material from the Red Giant Star, the massive heat and pressure creates a run-away thermonuclear reaction resulting in the White Dwarf Star having a Nova explosion.

However, this explosion does not destroy the White Dwarf Star. In fact, such a Nova explosion comes in cycles. This is how NASA and astronomers can predict approximately when each Nova explosion will occur.

However, unlike a Solar Eclipse, scientists cannot predict the exact date or time of a Nova. So, you need to pay attention to the news media (newspapers, radio, television, and the Internet) over the next several months, particularly astronomy and science media and web-sites, to be alert to when the Nova occurs. When the Nova does occur, SpaceWatchtower will announce the Nova occurrence on the SpaceWatchtower 'X' / Twitter News-Feed (Internet link to this 'X' / Twitter News-Feed near the end of this blog-post).

It was in February of 2016 that astronomers announced that T Coronae Borealis had entered a “phase of unprecedented high activity” that would lead to a Nova. The star began to dim in March of last year, a precursor to going Nova. Hence, scientists predicted that the Nova would probably occur between June and September of this year, but it could occur later in the year.

Recurrent novae are unpredictable and contrarian,” said Dr. Koji Mukai, a fellow astrophysics researcher at NASA's Goddard Space Flight Center in Greenbelt, Maryland, a suburb of Washington DC. “When you think there can’t possibly be a reason they follow a certain set pattern, they do – and as soon as you start to rely on them repeating the same pattern, they deviate from it completely. We’ll see how T CrB behaves.”

The T Coronae Borealis White Dwarf Star recurrent Nova (recurring approximately once every 80 years) last had a Nova explosion in 1946. This Nova was discovered in 1866, but has been observed as early as 1217 (when it was recorded as a star by a German monk named Abbott Burchard, according to NASA) and 1787 simply as a star with a brightness of 10th magnitude.

In Latin, Nova simply translates as 'new'. Hence, when the ancient peoples saw a bright new star in a location where no star had previously been observed (as Galileo Galilei did not invent the astronomical telescope until 1609), they called it a Nova.

Novae (plural of Nova) are rare. In fact, there are only ten located within our Milky Way Galaxy, according to William J. Cooke from NASA's Meteoroid Environments Office.

Internet Links to Additional Information ---

Nova: Link >>> https://en.wikipedia.org/wiki/Nova

T Coronae Borealis (Blaze Star): Link >>> https://en.wikipedia.org/wiki/T_Coronae_Borealis

Science Experiments Children & Teens Can Do At Home During Summer Break !

Relsted Blog-Posts ---

"Photos: Total Solar Eclipse Viewed in Cleveland." Sat., 2024 June 8.


"Northern Lights Seen in Pittsburgh." Wed., 2024 May 15.

Source: Glenn A. Walsh Reporting for SpaceWatchtower, a project of Friends of the Zeiss     

               "Once-in-Lifetime Bright Nova Star Visible W/Out Telescope by End of Year"

                  Monday, 2024 July 22.

            Artificial Intelligence not used in the writing or production of this article.

            © Copyright 2024 Glenn A. Walsh, All Rights Reserved

                             Like This Post? Please Share!

More Astronomy & Science News - SpaceWatchtower 'X' / Twitter News-Feed:
Link >>> https://twitter.com/spacewatchtower

Astronomy & Science Links: Link >>> http://buhlplanetarium.tripod.com/#sciencelinks

Want to receive SpaceWatchtower blog posts in your in-box ?
Send request to < spacewatchtower@planetarium.cc >.

gaw

Glenn A. Walsh, Informal Science Educator & Communicator                                                             (For more than 50 years! - Since Monday Morning, 1972 June 12):
Link >>> http://buhlplanetarium2.tripod.com/weblog/spacewatchtower/gaw/
Electronic Mail: < gawalsh@planetarium.cc >
Project Director, Friends of the Zeiss: Link >>> http://buhlplanetarium.tripod.com/fotz/
SpaceWatchtower Editor / Author: Link >>> http://spacewatchtower.blogspot.com/
Formerly Astronomical Observatory Coordinator & Planetarium Lecturer, original Buhl Planetarium & Institute of Popular Science (a.k.a. Buhl Science Center), America's fifth major planetarium and Pittsburgh's science & technology museum from 1939 to 1991.
Formerly Trustee, Andrew Carnegie Free Library and Music Hall, Pittsburgh suburb of Carnegie, Pennsylvania, the fourth of only five libraries where both construction and endowment funded by famous industrialist & philanthropist Andrew Carnegie.
Author of History Web Sites on the Internet --
* Buhl Planetarium, Pittsburgh: Link >>> http://www.planetarium.cc Buhl Observatory: Link >>> http://spacewatchtower.blogspot.com/2016/11/75th-anniversary-americas-5th-public.html
* Adler Planetarium, Chicago: Link >>> http://adlerplanetarium.tripod.com
* Astronomer, Educator, Optician John A. Brashear: Link >>> http://johnbrashear.tripod.com
* Andrew Carnegie & Carnegie Libraries: Link >>> http://www.andrewcarnegie.cc

 * Other Walsh-Authored Blog & Web-Sites: Link >>> https://buhlplanetarium.tripod.com/gawweb.html

Wednesday, July 3, 2024

Dog Days of Summer Begin, As Earth Farthest from Sun!

  


While the Orion constellation can be seen to the right, the bright star Sirius, the "Dog Star", can be seen at the bottom of this image. (Image Sources: European Space Agency, NASA, Wikipedia.org, By Hubble European Space AgencyCredit: Akira Fujii - http://www.spacetelescope.org/images/heic0206j/ (watermark was cropped), Public Domain, https://commons.wikimedia.org/w/index.php?curid=5246351)

By Glenn A. Walsh

Reporting for SpaceWatchtower

We are now entering the “Dog Days of Summer” in Earth's Northern Hemisphere. However, this is also the time of year, shortly after the Northern Hemisphere's Summer Solstice, when the Earth is actually farthest from the Sun (known as Earth Aphelion) !

Today, the Dog Days of Summer are considered the days between July 3 and August 11 each year. These Dog Days begin just a little less than two weeks after the Summer Solstice, the official beginning of Summer in the Northern Hemisphere.

For A.D. 2024, the season of Summer began at Earth's Northern Hemisphere's Summer Solstice (and the season of Winter begins at the Southern Hemisphere's Winter Solstice) at the moment of the June Solstice: Thursday Afternoon, 2024 June 20 at 4:51 p.m. Eastern Daylight Saving Time (EDT) / 20:51 Coordinated Universal Time [UTC – International time used by scientists; previously referred to as Greenwich Mean Time (GMT) or Greenwich Civil Time (GCT)]. Summer will continue in the Northern Hemisphere (and Winter will continue in the Southern Hemisphere) until the Autumnal Equinox when the season of Autumn / Fall commences in the Northern Hemisphere (and Spring begins in the Southern Hemisphere): Sunday Morning, 2024 September 22 at 8:44 a.m. EDT / 12:44 UTC.

In Meteorology (Weather Science), the convention is to start a season on the first day of a calendar month. So, Meteorological Summer runs from June 1 to August 31.

Also within the Dog Days of Summer come the traditional Cross-Quarter (XQ) Day known as Lammas (Anglo-Saxon) or Lughnasadh (Irish / Scottish) on August 1. Located approximately half-way between the Summer Solstice and the Autumnal Equinox, this day has long been considered the beginning of harvesting crops.

Lammas / Lughnasadh Day, in ancient times,was a festival day which marked the start of the harvest season, particularly the wheat harvest. On Lammas Day, it was customary to bring a loaf of bread, from the new crop, to church to be blessed.

August 1 also marks the anniversary of the birth of America's first professional, female astronomer. Maria Mitchell, Professor of Astronomy at Vassar College and discoverer of Miss Mitchell's Comet in 1847, was born on 1818 August 1 in Nantucket, Massachusetts.

While August 1 is the traditional Cross-Quarter Day, due to calendar changes over the years, in modern times the actual Cross-Quarter Day differs by as much as a week. For 2024, Lammas / Lughnasadh Day actually occurs on Tuesday, 2024 August 6 at 8:10 p.m. EDT / August 7 at 0:10 UTC.

Dog Days of Summer

So, how did these days become known as the Dog Days of Summer?

First, we need to look at the pictures in the sky that ancient peoples saw in the stars, now known as constellations. One of the most recognized constellations is that of Orion the Hunter (Ori).

And, many hunters have one or more hunting dogs to assist them. This was also true in Greek mythology for Orion. Orion's two dogs, Canis Majoris or Canis Major (CMa: Greater Dog) and Canis Minoris Canis Minor (CMi: Lesser Dog), were each given their own constellation.

The brightest star in Canis Major also happens to be the brightest star in Earth's night sky, the star Sirius (Alpha CMa or a CMa). And, being the brightest star in Canis Major, Sirius is known as the “Dog Star”. Sirius is located 8.611 light-years from the Earth and has an astronomical, Apparent Visual Magnitude of brightness of -1.45.

Being the brightest star in the night sky, ancient Romans assumed that Sirius provided heat to the Earth, as did our Solar System's Sun. During the Summer months, Sirius rises and sets at generally the same time as our Sun. Even in ancient times, astronomers were able to use mathematics to determine the rising and setting times of a star in the daytime sky.

The Romans believed that heat from Sirius, added to the heat from the Sun, caused the Summer months to be so much hotter than the rest of the year. Hence, the middle of the Summer season in Earth's Northern Hemisphere, now during July 3 to August 11 (the actual dates varied, somewhat, in ancient times), has become known as the Dog Days of Summer.

Today, we realize that a star 8.611 light-years away, no matter how bright, can never provide enough heat to affect life on Earth. Further, even the annual, variable distance between Earth and our own Sun is not the reason for the additional heat in the Northern Hemisphere during the Summer months.

Earth Aphelion

Although the Summer months in the Northern Hemisphere are known for the year's warmest weather, the Earth is actually at the point in its orbit farthest from the Sun (astronomically known as the point of Aphelion) around July 5. This Friday morning, just one day after the day we celebrate the 248th year of American Independence on July 4 and a couple weeks after the Summer Solstice on June 20, will mark Aphelion for 2024, the location in Earth's annual orbit around the Sun where our planet is farthest from the Sun for the entire year!

This year, Earth Aphelion will occur early on Friday Morning, 2024 July 5 at 1:06 a.m. Eastern Daylight Saving Time (EDT) / 5:06 Coordinated Universal Time [UTC – International time used by scientists; previously referred to as Greenwich Mean Time (GMT) or Greenwich Civil Time (GCT)]. At that moment, Earth will be the farthest from the Sun for the whole year: 94,510,539 statute miles / 152,099,968 kilometers.

Earth's closest approach to the Sun this year (known astronomically as Perihelion) occurred on 2024 January 2 at 7:38 p.m. Eastern Standard Time (EST) / January 3 at 0:38 UTC, at a distance of 91,404,095 statute miles / 147100631.86 kilometers. Next year, Perihelion occurs on 2025 January 4 at 8:28 a.m. EST / 13:28 UTC, at a distance of 91,405,993 statute miles / 147103686.4 kilometers.

In general, the distance from the Earth to the Sun is not the major factor determining the heat of Summer or the cold of Winter. This is true, despite the fact that Earth receives about 7 per-cent more solar radiation from the Sun during the time of Earth Perihelion in January, than at the time of Earth Aphelion in July.

Solar radiation, and hence the heat from the Sun, depends on the length of daylight and the angle of the Sun above the horizon. The tilt of the planet's axis, about 23.44 degrees toward the Sun, determines the additional and more direct solar radiation received by a planet's Northern or Southern Hemisphere, and hence, the warmer season of the respective hemisphere.

While the Sun does have motions (the Sun rotates on its own axis about once every 27 Earth days; our Solar System revolves around the center of the Milky Way Galaxy once every 225 million-to-250 million Earth years), it is actually the motion of the Earth tilted on its axis, away from the plane of the ecliptic (Earth's orbital plane around the Sun), while revolving around the Sun, that causes the Earth's seasons.

The Earth's Perihelion in January, and Aphelion in July, are due to the elliptical nature of the Earth's orbit around the Sun. Perihelion and Aphelion would not occur if the Earth's orbit was a true circle.

The dates of Earth Perihelion and Earth Aphelion are not fixed. Due to the Earth's Precession of the Equinoxes, these days shift forward approximately one day every 58 years. About 800 years ago, the Earth Perihelion was on the date of the Winter Solstice, around December 21; Earth Perihelion will be on the Vernal Equinox, the beginning of Spring around March 20, about 4,300 years from now. Earth's Axial Precession (often described as a "wobble" in the Earth's orientation, like a spinning top or a gyroscope) gradually changes the orientation of the Earth's Rotational Axis, which completes one rotational cycle once every 25,772 years.

However, because Earth is farther from the Sun during our Spring and Summer seasons, people in Earth's Northern Hemisphere actually benefit from a few extra days of warmth (on average), than the number of days in the Autumn and Winter seasons of the year. When Earth is closer to the Sun, the Earth travels faster in its elliptical orbit around the Sun (during the Autumn and Winter months); and, when Earth is farther than average from the Sun (during the Spring and Summer seasons) the Earth travels a little more slowly (Kepler's Second Law of Planetary Motion) --- again, this refers to the Northern Hemisphere. Hence, the Spring and Summer seasons, in the Northern Hemisphere, have a few more days than the Autumn and Winter seasons.

In fact, the late Jay Pasachoff, who was Field Memorial Professor of Astronomy at Williams College in Williamstown, Massachusetts and author of widely-used, college astronomy text-books, precisely calculated the duration of each season in the Northern Hemisphere:

* Summer: 93 days, 15 hours

* Spring: 92 days, 19 hours

* Autumn / Fall: 89 days, 20 hours

* Winter: 89 days, 0 hours

Internet Links to Additional Information ---

Dog Days of Summer -

Link 1 >>> https://wilstar.com/dogdays/

Link 2 >>> https://en.wikipedia.org/wiki/Dog_days

Star Sirius: Link >>> https://en.wikipedia.org/wiki/Sirius

Constellation Canis Major: Link >>> https://en.wikipedia.org/wiki/Canis_Major

Science Experiments Children & Teens Can Do At Home During Summer Break !


Related Blog-Posts ---

"Summer Begins Thursday Afternoon at Solstice." Mon., 2024 June 17.


"Earth Farthest from Sun for Year: Thursday." Mon., 2023 July 3.


1st U.S. Female Professional Astronomer: Leading Women's Suffragist." Wed., 2020 Aug. 26.


"Astronomical Mid-Point of Summer." Tue., 2013 July 30.

Source: Glenn A. Walsh Reporting for SpaceWatchtower, a project of Friends of the Zeiss     

               "Dog Days of Summer Begin, As Earth Farthest from Sun!"

                  Wednesday, 2024 July 3.

            Artificial Intelligence not used in the writing or production of this article.

            © Copyright 2024 Glenn A. Walsh, All Rights Reserved

                             Like This Post? Please Share!

More Astronomy & Science News - SpaceWatchtower 'X' / Twitter Feed:
Link >>> https://twitter.com/spacewatchtower

Astronomy & Science Links: Link >>> http://buhlplanetarium.tripod.com/#sciencelinks

Want to receive SpaceWatchtower blog posts in your in-box ?
Send request to < spacewatchtower@planetarium.cc >.

gaw

Glenn A. Walsh, Informal Science Educator & Communicator                                                             (For more than 50 years! - Since Monday Morning, 1972 June 12):
Link >>> http://buhlplanetarium2.tripod.com/weblog/spacewatchtower/gaw/
Electronic Mail: < gawalsh@planetarium.cc >
Project Director, Friends of the Zeiss: Link >>> http://buhlplanetarium.tripod.com/fotz/
SpaceWatchtower Editor / Author: Link >>> http://spacewatchtower.blogspot.com/
Formerly Astronomical Observatory Coordinator & Planetarium Lecturer, original Buhl Planetarium & Institute of Popular Science (a.k.a. Buhl Science Center), America's fifth major planetarium and Pittsburgh's science & technology museum from 1939 to 1991.
Formerly Trustee, Andrew Carnegie Free Library and Music Hall, Pittsburgh suburb of Carnegie, Pennsylvania, the fourth of only five libraries where both construction and endowment funded by famous industrialist & philanthropist Andrew Carnegie.
Author of History Web Sites on the Internet --
* Buhl Planetarium, Pittsburgh: Link >>> http://www.planetarium.cc Buhl Observatory: Link >>> http://spacewatchtower.blogspot.com/2016/11/75th-anniversary-americas-5th-public.html
* Adler Planetarium, Chicago: Link >>> http://adlerplanetarium.tripod.com
* Astronomer, Educator, Optician John A. Brashear: Link >>> http://johnbrashear.tripod.com
* Andrew Carnegie & Carnegie Libraries: Link >>> http://www.andrewcarnegie.cc

 * Other Walsh-Authored Blog & Web-Sites: Link >>> https://buhlplanetarium.tripod.com/gawweb.html