[image: Atena-e-Aracne-mito-e-storia-della-tessitura-a-Venezia.jpg]
*Arachne:*  Weaving the Sordid Tale
Had the Olympian gods condescended to sit for a psychiatric evaluation, the
examiner would have quickly concluded that they suffered from an incurable
narcissistic personality disorder. Such an affliction is understandable
when one considers that they were powerful beyond all mortal comprehension
and they all enjoyed an ageless beauty, save Hephaestus, the deformed god
of fire, forges and stonecraft.   Narcissists tend to be quite insecure
when in the presence of someone possessed of comparable or even superior
abilities. Olympians even more so, especially when their rival is a mere
mortal, as the following tale about a weaver named Arachne will illustrate.
Arachne was born in Lydia to Idmon of Colophon, a revered dyer in purple.
Even from an early age, Arachne exhibited extraordinary skills as a
weaver.   Her tapestries were not only vibrantly colorful, but
astonishingly lifelike.   It was once said that she wove a tapestry
depicting the quest of the Argonauts so brilliantly one could actually see
the waves moving along the threads.   Athena, the goddess of war, wisdom,
and handicraft, came to hear about this precocious girl.   On occasion she
watched Arachne working at her craft and to her distress realized that the
mortal was,indeed, profoundly gifted. Athena's distress devolved into rage
when she heard Arachne once proclaim that her tapestries were superior to
all others, even those of Athena herself.   Athena promptly disguised
herself as an old woman and came upon Arachne working at her loom.
"Your boasts have displeased the mighty Athena," the crone warned her.  "Be
humble before the goddess.  Acknowledge her as a superior weaver and she
might spare your soul."   Arachne scoffed.  "If Athena is displeased, have
her tell me herself.  If she believes herself to be the better weaver, let
her prove it in a contest."     At this, the old crone transformed back
into the imposing goddess resplendent in her helmet and chiton.   Apart
from being daunted, Arachne held her in a steadfast gaze and said, "Shall
we begin our contest now?"   Athena conjured her own loom and set
immediately to work.   Both Athena and Arachne worked furiously on their
tapestries.   Athena's depicted the Olympians punishing mortals for their
hubris and winning great battles, such as those against the Titans and
Giants.    Arachne's tapestry showed the gods engaged in less noble
actions, such as Zeus' many pursuits of mortal women.    Her aim was to
depict the Olympians as not only flawed, but frivolous.      At the
contest's end, Athena was incensed to observe that Arachne's tapestry was
not only insulting to the gods, but of superior quality to her own.
 Athena furiously ripped Arachne's tapestry into shreds and then struck her
three times.      The humiliated Arachne then hanged herself.    However,
as she was dying, the suddenly contrite Athena dabbled her head with one of
Hecate's potions.  Arachne changed from a woman into a spider and in this
new form was able to weave with eight arms instead of one.    Hence, the
term "Arachnid."
[Note for the nitpickers:   Yes, Ovid is the principal source for this
story.   As Ovid was a Roman poet, he would have referred to Athena as
"Minerva."  We thought we'd point that out because when it comes to facts,
mythology people tend to even be less forgiving than Trekkies.]


THE SOUTHWORTH PLANETARIUM
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Founded January 1970
Julian Date: 245954.16
2019-2020:  CXXVI

THE DAILY ASTRONOMER
Tuesday, April 14, 2020
Remote Planetarium 12: Anatomy of an Orbit

Before we begin, let's review what we already know about planetary orbits


   - Every planet's orbit is an ellipse with the Sun at one focus
   - All planet orbits, save Pluto, are aligned closely with Earth's
   orbit.  For this reason we will only see the planets around the ecliptic,
   the undulating curve that passes through thirteen constellations
   - The closer a planet is to the Sun, the greater its orbital velocity
   will be.
   - The planet's distance is related to its orbital period
   - A planet's distance from the Sun isn't constant


We also know that we're watching moving planets from a moving platform.
Moreover, the speeds of those planets, and their distances from Earth and
the Sun are always changing.  All this motion can make for a great deal of
complexity.   However, we will discover that we can still track these
planets quite easily just by remembering a few nifty tricks.    Now we
should review some terms:


[image: vt2004-if11-fig4.jpg]

   - *Inferior conjunction:  * when an inferior planet moves between the
   Sun and Earth
   - *Opposition:* when a planet is on the far side of Earth relative to
   the Sun
   - *Superior conjunction:*  when a planet is on the far side of the Sun
   relative to Earth

Now, for some new terms:

   - *Greatest elongation:   *the greatest angular distance separating an
   inferior planet from the Sun in our sky.  When at* greatest western
   elongation,* the planet will be visible in the eastern pre-dawn sky.
   When at *greatest eastern elongation*, the planet will be visible in the
   western evening sky.
   - *Quadrature: *  the position of a superior planet at right angles from
   the line connecting Earth and the Sun.


Our aim today is to determine how we can use our knowledge of planetary
orbits to predict when we will be able to see planets and where they will
be located.

We know:

   - when a planet is in *inferior conjunction*, it isn't visible, unless
   it is moving directly in front of the Sun (a topic for another day.)
   - when a planet is at *opposition,* it will rise around sunset and set
   around sunrise.
   - when a planet is in* superior conjunction*, it isn't visible at all.


To understand how all this information can aid us in tracking the planets,
let's follow an* inferior planet *from one inferior conjunction to another
to see how its orbital position affects its location from our perspective.


   1. At inferior conjunction, the planet isn't visible.   Yes, you're
   right, we already said that.
   2. After inferior conjunction, the planet will move into the pre-dawn
   eastern sky until reaching greatest western elongation.
   3. The planet will appear to move back toward the Sun in our sky as it
   moves toward superior conjunction when it will no longer be visible again.
   4. After superior conjunction, the planet will then move into the
   western evening sky until it reaches greatest eastern elongation.   It then
   appears to move back toward the Sun and then vanishes before reaching
   inferior conjunction again.

A *superior planet*'s orbit is somewhat simpler because it will never be in
inferior conjunction.

   1. A superior planet will move into* superior conjunction, *meaning that
   it will be at the far side of the Sun relative to Earth.
   2. Then, the planet will appear in the early morning sky.  Eventually
   the planet will move from morning sky into the late evening sky.
   3. The planet will then be at* opposition, *on the far side of Earth
   relative to the Sun.   It will rise at sunset and set at sunrise
   4. After opposition, the planet will appear to approach the Sun in the
   evening sky until it vanishes with the Sun at dusk.    It will then pass
   back through superior conjunction.



That is all very well. However, in order to predict when the planet will
move through those various stages, one needs to know how much time each
cycle requires.       We'll now proceed to the concepts of sidereal periods
and synodic periods.

A *sidereal period* is the time a planet requires to complete an orbit
around the Sun with respect to the distant stars.

A *synodic period* is the time a planet requires to reappear at the same
point relative to Earth.  For instance, the time period separating
successive oppositions or inferior conjunctions.

These periods are not the same because Earth is always on the move.    To
explain the synodic period, we'll use Jupiter as an example.

[image: synjup.png]
At a certain time, Jupiter is at opposition (point A), meaning that it is
on the far side of Earth relative to the Sun.     After this opposition,
Earth and Jupiter continue moving.  As Earth is much closer to the Sun, it
will be revolving around it much faster.  A year later, Earth returns to
the same point it occupied when Jupiter was last at opposition.  However,
during that year Jupiter also moved along its orbit.  Because Jupiter's
year is almost equal to 12 Earth years, Jupiter progressed only through
1/12th of its orbit.   Earth then has to "catch up" to Jupiter in order for
it to be as opposition again (point B.)   The amount of time separating
these two oppositions is, on average, 399 days.     (This varies somewhat
because the distances and therefore the speeds of the planets are not
constant.)

Let's look at some of Jupiter's past opposition dates

2005  April  3

2006  May 4

2007 June 5

2008  July 9

2009 August 14

2010  September 21

Notice the pattern?    Even though each date is not separated by exactly
399 days, it is a close approximation.  Expect Jovian opposition to occur
about 1 year and 1 month apart with a few extra days here and there.
Would you guess that the following opposition occurred around Halloween
2011?  If so, your guess is correct.  The 2011 Jupiter opposition date was
October 29th.

The following chart lists the sidereal and synodic periods of the planets:

PlanetSynodic Period (days)Sidereal Period
Mercury 116 88 days
Venus 584 225 days
Earth - 1.0 year
Mars 780 1.9 years
Jupiter 399 11.9 years
Saturn 378 29.5 years
Uranus 370 84.0 years
Neptune 368 164.8 years
Pluto 367 248.5 years

This year Saturn is in opposition on July 20.   Based on the chart above,
when you would expect Saturn to be at opposition in 2021?
Answer: * August 2*
You can plan to see Saturn all night long in early August 2021.
When will you see Saturn all night long in 2022?
Saturn opposition 2022:*  August 14*

About one year and two weeks separate successive Saturian oppositions.


Let's finally use Venus as an example.  One can currently see Venus in the
western evening sky. (And, it is brilliant, of course.)

We know that Venus will next be in inferior conjunction on June 3, 2020.
At what time will it next pass through  inferior conjunction?   *Jan 9,
2022 *
And the time after that?  *August 1, 2023 *
Venus' successive inferior conjunctions will be separated by about 1 year
and seven months.

During the quiz on Friday, we'll devote a section to using this information
to find the planets in their current positions.

Tomorrow, we turn to physics with Newton's Weighty Laws.




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