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03.14/2017 – Ephemeris – It’s Pi Day!

March 14, 2017 Comments off

Ephemeris for Pi Day 3.14, Tuesday, March 14th.  The Sun will rise at 7:56.  It’ll be up for 11 hours and 51 minutes, setting at 7:47.  The Moon, 2 days past full, will rise at 10:04 this evening.

Welcome to Pi Day.  I had some NASA inspired links posted on this blog this past Sunday for your enjoyment.  Also simply do an Internet search for Pi Day and lots of fun information and activities will be listed.  I remember an exercise in high school calculating pi with an inscribed polygon in a circle of ever increasing numbers of sides.  Somewhere in there I messed up and came out with an answer that didn’t quite get there.  This was in the years B.C. that is Before Calculators.  Speaking of round things, Jupiter will rise this evening followed by the Moon and the star Spica in the east.  They will all be up by 10:30.  Jupiter is not yet an evening planet, since it is not up by sunset.  It’s still seen in the morning sky.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addenda

Had I known in the tenth grade this strategy to calculate pi, I could have saved myself a lot of grief.  Simply google calculate pi with toothpicks.  One of the hits was this from Science Friday:  https://sciencefriday.com/articles/estimate-pi-by-dropping-sticks/*.  Basically it’s by dropping lots of toothpicks on a piece of paper with parallel lines spaced the length of the toothpicks apart.  The total number of toothpicks dropped times two divided by the number of toothpicks that cross a line will approximate pi.  The more drops, the closer to pi one gets.

  • In the formula in the link, if the length of the toothpicks equals the distance between the lines, those terms drop out of the formula.

Grouping of Jupiter, the Moon and the star Spica

Jupiter, the Moon and the star Spica

Jupiter, the Moon and the star Spica at 11 p.m. March 14, 2016. Since the Moon moves eastward about its diameter an hour. So observers east or west of here will see the Moon in a different position in relation to these other two bodies. Created using Stellarium.

03/13/2017 – Ephemeris – More thoughts about yesterday’s time change

March 13, 2017 Comments off

Ephemeris for Monday, March 13th.  The Sun will rise at 7:58.  It’ll be up for 11 hours and 48 minutes, setting at 7:46.  The Moon, 1 day past full, will rise at 9:03 this evening.

We are now plunged back into dark mornings like we were two month’s ago thanks to the start of Daylight Saving Time.  However we are only a week from the vernal equinox, the first day of spring here in the northern hemisphere.  However some of my blog followers down under will experience the start of autumn on that day.  For us in the next three months the sunrise time will back down 2 hours, and will rise around 6 a.m.  Our sunset times will advance a bit less than that, an hour and 45 minutes.  The lopsidedness is a consequence of both the Earth’s axial tilt and its slightly elliptical orbit.  We are moving somewhat away from the Sun now and are slowing down a bit.  It’s all kind of hard to explain, but makes perfect sense… eventually.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addendum

Well, I’m going to try to explain it now.

If one visits most observatories, there will be a clock, usually in the dome that doesn’t seem to read the correct time. We have one in Northwestern Michigan College’s Rogers Observatory’s dome. It only agrees with the time on your watch for an instant on October 16th. It’s called a sidereal clock and it measures Earth’s rotation with respect to the stars, and it gains approximately 4 minutes a day compared to our normal clocks which are geared to the Sun.

The Earth and all the planets orbit the Sun in a counterclockwise direction when seen from the north. Also the Earth and most of the planets spin also in a counterclockwise direction. The exceptions are Venus and Uranus. Most large satellites like our Moon also orbit their planets in a counterclockwise direction. From the surface of the Earth these bodies appear to generally move eastward, while the celestial sphere mirror reflects our eastward rotation by appearing to move east to west.

The Sun appears to move about one degree a day eastward. (360° / 365 days = 1° approximately). The Earth rotates through 15° an hour (360°/24 hours = 15° and 60 minutes in an hour / 15 = 4 minutes to rotate a degree). So on average and approximately after the Earth rotates back to the same point with regard to the stars, it has to rotate and extra degree to catch up to the Sun, which takes 4 more minutes, which is why the solar day is 4 minutes longer than a sidereal day. (Well, 3 minutes 55.9084 seconds if you want to get picky about it!)

Of course it’s not that simple. It never is that simple. This would all work out if the Earth orbited the Sun in a uniform circle and the Earth had no axial tilt. The Earth’s tilt is also called obliquity. The Sun would appear to move uniformly over the Earth’s equator. That Sun, called the mean Sun is what we base our solar time on, not the real Sun. However the Earth’s orbit is elliptical, with the Earth moving fastest at its perihelion or closest point to the Sun, around January 3rd, and slowest at aphelion or farthest point around July 4th. Also the Earth’s axial tilt is 23 ½ °, and is only on the equator two days a year March 20th and September 23rd.

Ever see this funny figure 8 in the Pacific Ocean on old globes?

The Analemma

Illustration 1. An Analemma graphically demonstrating the actual Sun’s relation to the mean Sun during the year.

Both eccentricity and obliquity work together to produce the analemma as seen in the diagram below. This figure 8 can actually be photographed in the sky by exposing the same frame of film at regular intervals, or stacking images of the same area of the sky over a year at the same time of day. There are plenty of examples using an Internet search engine to search for analemma images. It is one way to illustrate the equation of time, which is the correction one must make to a sundial reading to get to the correct local mean solar time. To that one must add or subtract one’s offset from the time zone’s time meridian. See Friday’s post.

Cause of the analemma

Illustration 2. How eccentricity of the Earth’s orbit and obliquity combine to affect the analemma. The effects add at the bottom near the winter solstice and subtract near the summer solstice.


The above diagram was taken from Ethan Siegel’s Starts with a Bang blog: http://scienceblogs.com/startswithabang/2010/12/17/celebrate-this-winter-solstice/ which also explains it.

The equation of time can be found in tabular form for easy sundial correction, or in a linear graphical form as seen below.

Equation of Time

Illustration 3. Linear representation of the equation of time

Actually the biggest effect on the equation of time, is especially near the solstices is the Earth’s obliquity (axial tilt). Below we see how the Sun’s declination affects how fast it appears time wise.

Sun crossing time lines

Illustration 4. How the Sun’s declination affects how rapidly it appears to cross time lines (meridians).

Declination of celestial objects is the same as latitude on the Earth. A star whose declination is the same value as one’s latitude will cross at the zenith once a day. In illustration 4 note that the near the solstices the time lines (meridians) are closer together, so the Sun will pass them faster than when near the equinoxes where the time lines are farther apart and the Sun is moving somewhat diagonally, taking longer to cross the time lines. In time only east-west motion counts.

Looking at Illustration 2, I’ve added arrows at the top (northern) and bottom (southern) extremities of each analemma source to give some idea of the Sun’s apparent speed at the solstices. At the bottom, near the December solstice the eccentricity speed of the Sun adds to the obliquity speed increasing the effects at that part of the analemma lobe, making it bigger. At the June solstice end of things eccentricity speed is in the opposite direction, slowing the Sun down.

So what? This affects the dates of the earliest and latest sunrises and sunsets. Here are those dates and time values for us here in northern Michigan (specifically the Interlochen/Traverse City area):

Earliest and Latest Sunrises and Sunsets

Table of Earliest and Latest Sunrises and Sunsets during the year for Interlochen/Traverse City area of Michigan.

All this may make little difference to our modern lives, governed by the atomic clocks in Paris and Fort Collins, Colorado, divorced as they are from the Earth’s actual rotation and the Sun except for the inclusion of the occasional leap second, like we had last December 31st. To folks like me who are amateur astronomers and have (or had in my case)  a day job, it would’ve been nice to have, on the summer solstice, astronomical evening twilight end before midnight.

I hope this helped rather than confused you.  What do you think?  drop me a comment.

03/10/2017 – Ephemeris – Daylight Saving Time starts Sunday

March 10, 2017 1 comment

Ephemeris for Friday, March 10th.  The Sun will rise at 7:03.  It’ll be up for 11 hours and 39 minutes, setting at 6:42.  The Moon, 2 days before full, will set at 6:38 tomorrow morning.

Daylight saving time will begin this Sunday at 2 a.m.  That means “spring forward”, setting our clocks ahead an hour.  Did you know that we spend more time under daylight time than standard time.  Standard time only lasts about 4 months and one week.  The rest of the time, nearly 8 months is spent under daylight time.  According to theory, anyway, one’s time meridian should run in the middle of its time zone. Right now our standard time meridian of 75 degrees west longitude runs through Philadelphia, 5 hours west of the prime meridian of Greenwich.  Come Sunday our time meridian will be 60 degrees west longitude, in the Atlantic at our latitude, and further to the north just touches the eastern tip of Nova Scotia.  In relation to the actual Sun we will be an hour and 43 minutes behind it, which is why sundials don’t tell the correct time around here.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addendum

Time Zones

Time zones with their meridians for North America.

11/24/2016 – Ephemeris – The little constellation that used to start the seasonal year

November 24, 2016 Comments off

Ephemeris for Thanksgiving Day, Thursday, November 24th.  The Sun will rise at 7:52.  It’ll be up for 9 hours and 14 minutes, setting at 5:06.  The Moon, 3 days past last quarter, will rise at 3:54 tomorrow morning.

From antiquity, the first constellation of the Zodiac has been Aries the ram.  That’s the constellation the Sun entered on the first day of spring, or the vernal equinox.  Well that was a couple of thousand years ago.  Currently the vernal equinox point is in western Pisces.  This is due to the wobbling of the Earth’s axis called precession.  The spinning Earth like and top or gyroscope wobbles when force is applied to it.  In this case the Sun and Moon.  One wobble takes 26,000 years to complete.  Anyway, Aries is a small constellation of four stars in a bent line, below the triangular constellation of Triangulum, which is itself below Andromeda.  It’s a bit west or right of the Pleiades or Seven Sisters star cluster.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addendum

Aries the ram

Aries the ram animated finder chart for 9 p.m. November 24, 2016. Created using Stellarium and GIMP.

The vernal equinox today

The vernal equinox today, where the blue line, the celestial equator and the orange line, the ecliptic or path of the Sun cross. The Sun is where these lines cross on the first day of spring (March 20th around here). Note that the vernal equinox is now in western Pisces. Created using Stellarium.

The vernal equinox in AD 100

The vernal equinox back in AD 100, where the blue line, the celestial equator and the orange line, the ecliptic or path of the Sun cross. The Sun is where these lines cross on the first day of spring. Note that the vernal equinox was at the east edge of Pisces. Created using Stellarium.

09/12/2016 – Ephemeris – Mercury passes inferior conjunction with the Sun today

September 12, 2016 Comments off

Ephemeris for Monday, September 12th. The Sun will rise at 7:18. It’ll be up for 12 hours and 39 minutes, setting at 7:58. The Moon, 3 days past first quarter, will set at 3:34 tomorrow morning.

Today the Planet Mercury will pass inferior conjunction, that is move between the Earth and the Sun. Unlike last inferior conjunction, when it passed directly in front of the Sun on May 9th. This time it will pass below the Sun. The term inferior means it is between the Earth and the Sun. A superior conjunction is when Mercury passes the back side of the Sun. Mercury will be moving into the morning side of the sky, and toward the end of the month it will be much easier to spot than it was last month when it was low in the west. On autumn mornings the ecliptic, the path of the Sun and planets, sticks up, close to vertical, while in the evenings it lies close to the horizon, which is also why Venus sets so soon after the Sun now.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addendum

Greatest Eastern Elongation of Mercury

Mercury last August 16 at greatest eastern elongation. Note how low Mercury is to the horizon at sunset. Created using Cartes du Ciel (Sky Charts).

Note in the charts above and below the line passing through the Sun, and the one the planets hang around is the ecliptic, the projection of the Earth’s orbit on the celestial sphere.  The grid line running through the west compass point at the horizon is the celestial equator.  I’m allowing us to see below the horizon.  As planets rise, move across the sky and set they will appear to move parallel to the celestial equator.

Greatest Western Elongation of Mercury

Mercury this coming September 28 at greatest western elongation. Note how high Mercury is to the horizon at sunrise. Created using Cartes du Ciel (Sky Charts).

Note too that Mercury appears farther from the Sun on August 16th than at September 28th.  And it is.  On August 16th Mercury appears 27.4 degrees from the Sun.  On September 28th, it’s only 17.8 degrees.  That’s a big advantage for observers in the southern hemisphere.  The best times to see an eastern elongation of Mercury is on winter and spring evenings, and the best times to see a western elongation of Mercury is on summer and autumn mornings.  Since the seasons are reversed from the northern hemisphere to the southern hemisphere.  Our not so good August 16th elongation of Mercury was a really good one for folks south of the equator.  We’ll return the favor September 28th.  But the best southern hemisphere greatest elongations are always greater in the separation of Mercury from the Sun  than northern ones because Mercury has a markedly elliptical orbit.

 

 

06/27/2016 – Ephemeris – Astronomical twilight lasts till after midnight… Bummer!

June 27, 2016 Comments off

Ephemeris for Monday, June 27th.  Today the Sun will be up for 15 hours and 33 minutes, setting at 9:32, and it will rise tomorrow at 5:59.  The Moon, at last quarter today, will rise at 1:57 tomorrow morning.

Here we are a week into summer and we find that the latest sunset was already last night.  That means that the last vestiges of twilight* don’t end until just after midnight.  It wouldn’t be so bad if the Sun was in the south at noon instead of 1:43 in the afternoon, due to being in the extreme western part of the eastern time zone and the imposition of daylight time.  For latitudes north of 48 ½ degrees, twilight currently doesn’t end.  That latitude will move northward as the Sun heads south.  As it is now we in the Grand Traverse region are currently getting only 4 ½ hours of darkness Moon willing.  And it won’t for the next few days at least.  Our darkness situation will start to get better in about a month from now.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

*Astronomical twilight begins and ends when the Sun is 18° below the horizon.

05/19/2016 – Ephemeris – Daylight Saving Time in West Michigan

May 19, 2016 Comments off

Ephemeris for Thursday, May 19th.  Today the Sun will be up for 14 hours and 59 minutes, setting at 9:09.   The Moon, 2 days before full, will set at 5:49 tomorrow morning.  Tomorrow the Sun will rise at 6:08.

It is nearing summer and the powers that be have bequeathed on us daylight saving time, even starting it before the end of winter since 2007.  It is a thing that amateur astronomers hate.  This time of year through the end of July the Sun just sets too late, and if one has a day job, it’s nearly impossible to stay up long enough to start observing at 11 p.m. or midnight, and be bright-eyed and bushy-tailed the next morning.  Nautical twilight, when the sea horizon is no longer discernible ends at 10:28 p.m. tonight, and astronomical twilight, when it’s pitch dark, ends at 11:19.  It gets worse the farther north and west you go in the Eastern time zone.   At least this year we have three planets to entertain us in the evening twilight.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addendum

Time Zone Map

Our place in the Eastern Time Zone. Source http://www.nationsonline.com.  If you are using Firefox right-click on the map and select View Image to enlarge.

We are near longitude W 86°.  Our Eastern Standard time meridian is W 75°, which runs through Philadelphia, which I’ve added to the map, southwest of New York.  With 15° per hour that makes that 44 minutes behind Philadelphia.  Theoretically time zones should extend 30 minutes on either side of a standard time meridian.

During daylight time our time meridian is W 60°, which is off the map.  That meridian just ticks the eastern end of Nova Scotia in Canada.  For us near 45° north latitude astronomical twilight ends shortly after midnight.

02/28/2016 – Ephemeris Extra – The years of our lives

February 28, 2016 1 comment

The continuing story of a small planet revolving around its star

Updated from the originally published in the January 1997 Stellar Sentinel, the monthly newsletter of the Grand Traverse Astronomical Society and republished in the February 2016 edition.

This year, 2016, is a leap year.  In leap years we have the US presidential elections, the Summer Olympic Games, and February has 29 days.  So what exactly is a leap year, and why am I writing about this earthly phenomenon in an astronomical society newsletter?  Well it’s astronomical of course. And if you think a year is a year is a year, well think again.
The calendar we use today is based on the Sun.  In ancient times the calendars of the Babylonians, Jews and many other ancient civilizations were based on the Moon, using the lunation, the period of about 29.5 days between new moons, as the basis for the calendar.  Lunar calendars tended to have months alternating 29 and 30 days, and years of 12 or 13 months to keep the whole scheme roughly in sync with the seasonal year.  There are vestiges of this system today in the various folklore of planting by the Moon.

The ancient Egyptians actually used two calendars.  The first was one based close to the sun and had 365 days.  It had 12 months of 30 days, each containing three 10 day decans.  There were 5 days at the end of the year that were holidays, and belonged to no month.  This civil calendar was used for state and accounting purposes.  The agricultural calendar was based on the Moon.  These two calendars were reconciled every 25 civil years which equaled 209 lunations, divided into 16 ordinary 12 month years, and 9 ‘great’ years of 13 months.  Still, since the Egyptian civil year is nearly a quarter of a day a year short, the civil calendar shifted slowly in relation to the seasons.  The Egyptian agricultural year started with the flooding of the Nile, which in those days was coincident with the heliacal rising of the brightest night time star Sirius, which they called Sothis.  A heliacal rising is when a star or planet is first visible in the morning twilight.  This heliacal rising occurs at a mean interval of 365.2507 days.  Thus the Egyptian civil calendar would be in sync with the agricultural year every 1460 years, a period called the Sothic Cycle.

The ancient Greek calendars were lunar ones.  Early on, each locality had their own calendar.  Starting in the 6th century BC the calendar situation got better when a cycle synchronizing lunar calendars with the sun was discovered.  It is the Metonic Cycle, probably discovered in Babylon.  Here 19 years of 365.25 days equal almost exactly 235 lunations.  That’s 12 ordinary 12 month years and 7 ‘great’ years of 13 months.  We find remnants of the Metonic Cycle with the Golden Number for the year given in almanacs, a number ranging from 1 to 19.  This year’s Golden Number is 3.  The year 1 BC was 1.  Under the old Julian calendar it was use to help determine the date of Easter.

The Julian Calendar is named for Julius Caesar who instituted it as a part of calendar reform he instituted in 46 BC.  The old Roman calendar was a lunar one, but in the earlier years of Julius Caesar’s reign the adjustments, called intercalations, such as 13th months in some years to keep the calendar roughly attuned to the sun, were neglected.  To straighten all this our, the year 46 BC was made 445 days long.  Starting in 45 BC the new calendar was instituted using the year of length 365.25 days.  Each 4 years an intercalary day was added.  This was February 29th, giving a 366 day year.  This we call a leap year.  Year 45 BC was a leap year, but due to some misunderstanding about the calendar reform, the one leap year in every four, was not kept.  In fact too many leap years were added, so in Caesar Augustus’ reign leap years from 8 BC to AD 8 were omitted to get back on track.

The western world ended up adopting the Julian calendar, and it was humming along just fine with leap years every 4 years.  However the Catholic Church and Pope Gregory XIII became alarmed that Easter was in danger of no longer being a spring feast.  The early church, adopted the Julian calendar rather than the Jewish lunar calendar.  But the most important feasts, the Crucifixion and Easter were tied to the Jewish feast of Passover, a spring feast starting in the middle of the month at full moon time.  Part of the problem was that the Vernal Equinox for ecclesiastical purposes was assumed to fall on March 21st, whether it actually did or not.  The first Sunday after the first full moon was Easter.

The problem is that the seasonal or tropical year is 11 minutes and 14 seconds shorter than the Julian year of 365.25 days.  In 400 years this amounts to about 3 days error.  So the easy correction is to eliminate 3 leap years out of 400 years.  The formula is simple.  All years divisible by 4 are leap years except century years which are not also divisible by 400.  Thus the year 1900 was not a leap year, but 2000 was, and 2100 will not be.

The other part of the reform was harder to swallow.  It was the elimination of 10 days because the real Vernal Equinox was by the 16th century falling on March 11th.  The Church was able to have this adopted in Catholic countries right away, so in the calendar of 1582 ten days were omitted between October 4th and 15th.  Protestant countries generally followed suit later.  England and the American Colonies converted to this new Gregorian Calendar in 1752 when by then 11 days were omitted between September 2nd and 14th.  The last to convert to the Gregorian Calendar was Greece and Orthodox Christianity who also made further improvements for the future.

I had once investigated how Microsoft Excel spreadsheets store dates.  It’s stored as a consecutive date starting with date 1 on January 1, 1900.  I had to convert dates downloaded from an IBM AS400 computer into a format compatible with Excel.  The dates came one day off.  It turns out that Microsoft or whoever devised the Excel dating scheme forgot that the year 1900 was not a leap year in the Gregorian calendar.  For my astronomical research I use dates both far in the past I use dating algorithms that use the Julian and Gregorian calendars where appropriate and takes into account the Gregorian discontinuity of 1582 into account.  These algorithms convert calendar dates to another type of consecutive day scheme called Julian Day Numbers of Julian dates for short, and back again.  In astronomy we see cycles of planetary orbits, variable star periods, etc.  They don’t fit into our hodgepodge of different month and year lengths.  We just want to know how many days between event A and event B.  Julian dates work for us.  The Julian dates start on January 1, 4713 of the Julian calendar, which predates any known historical date.  Oh by the way:  Julian dates start at noon Universal Time (UT) or Greenwich Mean Time (GMT), and fractional days are decimal.
I didn’t even touch when the year begins.  In Great Britain when the 1752 reforms took place they also changed the start of the year from March 25th to January 1st.

Bibliography

  • The Exact Sciences in Antiquity by O.  Neugbauer. Dover Publications
  • Explanatory Supplement to the Ephemeris H.M. Nautical Almanac Office

12/21/2015 – Ephemeris – Except for 12 minutes today is the last day of autumn.

December 21, 2015 Comments off

Ephemeris for Monday, December 21st.  The Sun will rise at 8:16.  It’ll be up for 8 hours and 48 minutes, setting at 5:04.   The Moon, 3 days past first quarter, will set at 4:50 tomorrow morning.

Here we are at the mostly last day of autumn.  The last 12 minutes will be the start of winter.   The winter solstice will occur at 11:48 this evening, here in the Eastern Standard Time Zone.  Next year winter will start 18 hours earlier.  The reason is that next year is a leap year and the addition of an extra day will push all the solstices and equinoxes back by about 18 hours.  Why only 18 hours?  18 hours is three-quarters of a day, and by this time next year we will have used up a quarter of that adjustment already.  The Earth takes approximately 365 and a quarter days to orbit the Sun, so a day is added every 4th year, except century years not divisible by 400.  I’ll discuss more about the implications of the solstice tomorrow.

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.

Addendum

The Earth near December solstice

Not quite the solstice, this is the Earth on December 16th, 2015 taken by the EPIC camera on the DISCOVR spacecraft at the Sun-Earth L1 point, some 1.5 million miles (1 million km) from the Earth.  Credit:  NOAA.

 

12/04/2015 – Ephemeris – Yours truly will survey ancient and pre-scientific cosmologies tonight

December 4, 2015 Comments off

Ephemeris for Friday, December 4th.  The Sun will rise at 8:02.  It’ll be up for 8 hours and 59 minutes, setting at 5:02.   The Moon, 1 day past last quarter, will rise at 2:09 tomorrow morning.

This evening’s meeting of the Grand Traverse Astronomical Society starting at 8 p.m. at Northwestern Michigan College’s Rogers Observatory will be a traditional December program.  This program alternates with a program on the Star of Bethlehem which will be revamped for next year.  This year I’m presenting Ancient Cosmologies, a look at the cosmologies or world views of many mostly pre-scientific cultures, including how the Biblical world view was influenced by one of them.  Then we’ll see the beginnings of Greek scientific thought that codified by Ptolemy in the second century AD, held sway for 1,500 years.   Also I’ll look at Monday’s occultation of Venus and Comet Catalina.  At 9 p.m. there will be a star party at the observatory with another program.  All are welcome.
I’ll post more on the Occultation of Venus on the blog tomorrow and Monday

Times are for the Traverse City/Interlochen area of Michigan. They may be different for your location.