| DIFFERENCES
OBSERVED ON THE SKY ON THE TWO HEMISPHERES |
This paper is submitted
by Fernando Martín Asín and Rosa Chueca Castedo,
faculty members of the College of Technical Topographical
Engineering of the Polytechnic University of Madrid
It highlights the main differences observed on the two hemispheres.
We will point out the differences observed as regards to seasons
(see details in the Annex), constellations, the moon, planets,
comets, and other starts of our sky.
************
First, let’s remember
the geographic coordinates of both Universities:
MADRID: Longitude
= 0 h 14 m 45 s (W to Greenwich) - Latitude = +40º 24’
ROSARIO:
Longitude = 3 h 53 m (W to Greenwich) - Latitude = -34º
36’
As regards to latitudes, please notice
that both cities, though having opposite signs, share almost
a symmetrical position as to Equator.
************
Probably, the most significant difference
between hemispheres lays on seasons since they are exactly
reversed. When we are in summer in our country, you are in
winter in Argentina. When we are in spring, you are in autumn.
Many times people take advantage of this fact and just in
a few hours by plane, they are able to leave the hot summer
of their place for the cold winter of the other hemisphere
or the opposite. Enclosed in the Annex, please find how to
calculate season’s duration. In fact, if our winter
is the shortest season in the year; your winter, on the other
hemisphere, will be the longest season.
************
Let us continue with our satellite,
the moon. Whenever we explain its movements, we focus on the
special language we use in our hemisphere, e.g. “the
moon lies”. We use this expression because when the
moon shows us a “D” shape (in Spanish, initial
letter of the word “decrease”), in fact, it is
a waxing moon. On the contrary, when we see a “C”
shape (in Spanish initial letter of “crescent”),
it is a waning moon. In Argentina, the situation is exactly
the opposite, then we say that the moon does not lie in the
southern hemisphere.
The moon is the satellite of the
Earth. It has been said that “it is man’s faithful
mate” and the poet’s inspiration source. There
is so much to say about our beloved moon!
************
Another interesting topic is the
observation of planets. We are here giving only a few details
about them because the only difference found is that they
are always observed—as with the moon— very near
to the Ecliptic. We know that ecliptic latitudes of planets
are always small, except with Mercury, first planet in our
solar system and even more so in the case of Pluto, the last
one. These planets together with the stars orbit the sky with
different slants from the horizontal depending on the hemisphere
on which we are standing as observers.
************
And now let’s search for comets
and asteroids. Certainly, it is their slant which determine
whether it results easier to observe them from Argentina or
from Spain. We took advantage of this topic in our classes
and we usually tell our students that we, Spanish observers,
find it rather difficult to spot comets since some hours before
we see a part of the sky, many other countries, e.g. Japan,
have already seen and searched it. The reason is the position
of that country in the terrestrial sphere; in other words,
the geographic longitude the inhabitants enjoy.
Likewise, we could also say that
we observe a part of the sky four hours before Argentine people
do. Therefore, since the sky moves counter clockwise, it is
always easier to spot comets in Spain rather than in Argentina.
We would like to develop this topic and we will do it when
our paper is accepted. Another point to take into account
is the comet’s particular position on the sky which
would favour a better view from negative latitude.
************
To finish our presentation, we will
speak about constellations. About how it is that some which
are hard to spot on the northern hemisphere due to their stars
slants, are so spectacularly seen on the other hemisphere.
Short time ago, a working mate commented us about how marvellous
it was for her to spot Scorpious constellation while travelling
along a latitude quite near to Rosario. She was amazed when
she spotted it in its full grandeur, especially because it
is so difficult to see it from our country.
Now let’s move to the Southern
Cross. Some time ago, I told my mates about my experience
with this constellation when I spotted it while on a trip
to Brazil. I commented on the difficulties I had to detect
it and how great I felt when I managed to see it.
It is also interesting to remark
the great feelings of surprise one experiences when the nearest
to the sun star—Centaurus or Rigil Kent—is spotted
from the southern hemisphere. This star is 4,3 light years
and takes position 4 as regards to brightness.
Then, we are going to speak about
a number of constellations that we can appreciate on this
hemisphere and that are forbidden on our latitudes. We thank
the opportunity to speak to the population of this marvellous
country of Argentina. We would like to comment about constellations
which, for us, are circumpolar and difficult to see from there.
For example, Ursa Major, Ursa Minor, Cassiopeia, Draco (Dragon)
and many others.
************
Another exciting topic is to observe
the differences on the sky during day movement by passing
from a positive latitude site to a negative one. I have always
been curious at observing how stars orbit without going past
the zenith when we are observers on northern latitudes. Instead,
stars crossing the sky approach the North Pole, i.e. they
cross the “first vertical”, but to the north.
We are not seeking a full understanding
on the part of the reader, we are only trying to get some
awareness about how different it may be to be an observer
on one place or another.
************
We are also making commentaries on
some expressions taken from Argentine books:
For example, when these books giving
a definition of the Vernal Point, they speak about the “Autumnal
Equinox” and our books speak about “Spring Equinox”.
It sounds
rather odd to our ears when you speak about your summer hours
running from September 1st to March 1st.
We also
read that you observe the stars Alpha Crux and Beta Crux at
maximal digressing position to determine the meridian.
In short, we are so enthusiastic
about observing the sky that we are always encouraging others
to join us. Argentina has a privileged position regarding
sky observation—as compared to Spain—since Argentineans
are able to watch constellations that are rather difficult
to see from our country.
************
Let’s profit from this opportunity
and talk a little about the 89 constellations the sky superbly
displays in front of our eyes. These constellations help us
to understand our own position and to locate planets. We know
that these planets—according to the time of the year
we are observing them— are constantly changing their
position against the background of the stars.
In Spain, in summer—winter,
in your country—if we raise our eyes to the sky, we
can easily detect the “Summer Triangle” on our
zenith. Even in autumn, we are able to marvel at this triangle.
It is built up by three stars: Vega, Deneb and Altair from
the constellations of the Lyre, the Swan and the Eagle respectively.
In my opinion, this triangle invites us to search for the
most beautiful double star in the sky: Albireo.
In the gravity centre of the Summer
Triangle, we find the beta star of the Swan. Let me tell you
an anecdote I really enjoy narrating. At my college time,
I had the honour of having a great professor who loved music.
He frequently spoke about Mussorgsky plays.
Once, our professor told us the story
of a play composed by this musician. In this story, the most
terrible storm struck and frightened the population of a little
village in the Alps. At dawn, when the storm was over, the
peaceful landscape emerged with Mussorgsky descriptive music
and a moment later, a bell from a tiny church rang far in
the distance and a flute of a shepherd sounded in the mountain.
And our professor used to say that “only for the sound
of that bell and the tunes of that flute life was worth living!”
I would like to paraphrase his expression
and speak about Albireo from the Swan. The sole pleasure of
splitting that start makes life worth living!. I have witnessed
such feeling in those who spot this double star for the first
time. It is a wonderful experience.
With the help of an ordinary telescope,
we can split that star and the weak spot of light of 3,1 magnitude
breaks in two within the range of the instrument. I invite
my readers to try this experience.
Two stars build up Albireo. They
are located 500 light years away, 34” distant one from
the other, their magnitudes are 3,1 and 5,4.
I often add that on splitting Albireo,
we can appreciate two dewdrops, one tinted in red and the
other in blue—one a ruby, the other a turquoise.
************
The Milky Way run through Cygnus
constellation. It is rather easy to picture the swan formed
by the stars of the constellation.
Another important detail is the star
M 27 from Messier Catalogue. It is also known as Dumb-Bell,
the name given to the brightest and largest nebula on the
sky. It was spotted by Carlos Messier in 1764.
We turn our eyes to the north and
we find Ursa Major, Ursa Minor with the north star Polaris,
Draco and Andromeda with the surprising M 31, and finally
Corona Borealis and so many others that we are not mentioning
here.
Another detail. In the old times,
the collection of stars received the name of “asterism”.
>From the very beginning, they have been compared to animals,
divinities, heroes and ordinary objects. In the old times,
the Greeks named many of the constellations with this kind
of words.
Ptolemy (100-178 B.C.)recorded 48
constellations in his Almagest. In the following centuries,
J.Bayer (1572-1625) and others identified 12 constellations
on the northern hemisphere and around 50 on the southern one.
Astronomers identified some others and today we have 89 constellations.
To the north of the Zodiac, there
are:
Andromeda, Aquila (Eagle),
Bootes (Herdsman), Camelopardalis (Giraffe), Canis Minor (Little
Dog), Cassiopeia (Queen Cassiopeia), Cepheus (King Cepheus
), Coma Berenices (Berenice´s Hair), Corona Borealis
(Northern Crown), Cygnus (Swan), Delphinus (Dophin), Draco
(Dragon), Equuleus (Colt), Hercules, Lacerta (Lizard), Lynix
(Lynx), Lyra (Lyre), Pegasus (Pegasus), Perseus (Perseus),
Sagitta (Arrow), Triangulum (Triangle), Ursa Major (Great
Bear), Ursa Minor (Little Bear), Vulpecula (Little Fox)
Then, the 13 well know from the Zodiac.
We are going to speak about them later.
And to the south of the Zodiac:
Antlia (Air Pump), Apus
(Bird of Paradise), Ara (Altar), Auriga (Charioteer), Caelum
(Chisel), Canes Venatici (Hunting Dogs), Canis Major (Larger
Dog), Carina (Keel), Centaurus (Centaur), Cetus (Whale), Chamaeleon
(Cameleon), Circinus (Compasses), Columba (Dove), Corona Australis
(Southern Crown), Corvus (Crow), Crater (Cup), Crux (Southern
Crux), Dorado (Goldfish), Eridanus (River), Fornax (Furnace),
Grus (Crane, Bird), Horologium (Clock), Hydra (Female Water
Snake), Hydrus (Male Water Snake), Indus (Indian), Leo Minor
(Smaller Lion), Lepus (Hare), Lupus (Wolf), Mensa, (Table
Mountain), Microscopium (Microscope), Monoceros (Unicorn),
Musca, (Fly), Norma (Square), Octans (Octant), Orion (Hunter),
Pavo (Peacock), Phoenix (Phoenix), Pictor (Painter’s
easel), Pisces (Fishes), Pisces Austrinus (Southern Fish),
Puppis (Stern), Pyxis (Compass), Reticulum (Reticle), Sculptor
(Sculptor´s Workshop), Scutum (Shield), Serpens Caputi
(Serpent´s Head), Serpens Cauda (Serpent´s Tail),
Sextans (Sextant), Telescopium (Telescope), Triangulum Australe
(Southern Triangle), Tucana (Toucan), Vela (Sails), Volans
(Flying Fish).
************
This presentation will be incomplete
unless we include some words about the Zodiac, the area where
the sun moves in its apparent movement around the Earth in
a year.
I am making reference to those 12
constellations we learnt in our childhood. In fact, they are
13 with Ophiuchus between Scorpious and Sagittarius.
Every Zodiac constellation has changed
its position with the passing of time. This is due to the
phenomenon called “Precession of the equinoxes”
or “Retrogradation of Aries point” discovered
by Hipparch, in the II century B.C.
Every constellation gradually changed
its position as compared to the original ones dated from 2000
years ago—when the correspondence with the 12 months
of the year was established.
Probably, those who have read some
of my books (Professor Martin Asin speaking), particular “Atlas
of the Sky” or a more recent one named “Constellations
of the Sky”, may recall my advise as regards to
cartographic representations; for the sky a stereographical
projection, for areas near to the poles a polar design and
for wedge-like divisions of the celestial sphere a meridian
scheme.
Although we have cited the 88 constellations
present in the sky, I always sustain that they are 89 since
Serpens, in my opinion, should be counted as two.
************
Finally, I would like to remind everybody,
especially those who follow horoscope advices, that we all
have our Zodiac sign changed. Horoscopes from magazines and
newspapers does not resemble in the least the rigorous position
of the Sun as it enters and leaves each constellation.
Actually, the first of the 13 signs
must be Pisces and not Aries. Currently, when the Sun is on
the Vernal Equinox, the constellation over which it is projected
is Pisces, although 2000 years ago it was Aries. Besides,
to make matters worse, there is Ophiuchus—the thirteenth
sign—located between Scorpious and Sagittarius.
ANNEX
HOW TO CALCULATE SEASON'S
DURATION
We feel it useful to make the calculus
in reference to the year 2000. We know that season’s
duration is gradually changing and will continue so until
the year 6500 in which two seasons will coincide:
Spring = Summer and Winter = Autumn
Nowadays, seasons are organised according
to their length—being the shortest the first and so
on:
Winter – Autumn – Spring
- Summer
This order corresponds to an observer
on the northern hemisphere. For observers on the southern
hemisphere, the order is reversed:
Summer – Spring – Autumn
- Winter
Let’s calculate the four season’s
length taking into account the “Ecliptic Longitude of
Perigee”. This datum changes every year and this year
2000 is 282º 56‘ 18”. I invite our readers
to revise some Astronomy concepts which will be useful to
follow our explanations.
First, let us remember that in Astronomy,
apart from the True Sun—the only one that exists and
gives light— we speak about two other Suns: the Fictitious
and the Mean one. The Fictitious is an ideal Sun moving along
the Ecliptic at a steady speed and it coincides with the True
one at Perigee and Apogee points. The Mean Sun is another
ideal Sun moving along the Equator at a steady speed and it
coincides with the Fictitious one at Aries and Libra points.
We relate the three Suns using the
Equation of Time. We define this equation as the difference
in right ascension between the True and the Mean Sun.
We use this Mean Sun to measure time
in our ordinary life. We relate mean, civil, official and
legal hours to the period of time called mean day and we get
the hour of our watches. The mean day is defined as the period
of time the Mean Sun takes to pass twice through the meridian
of a place. Then, dividing that value by 24 hours we get the
mean hour, and dividing the latter by 60, the mean minute
and likewise the mean second.
When we study the “Equation
of Time”, we said that it is the resultant of the two
functions named “Equation of the Centre” and “Reduction
to the Equator” (Readers may study these concepts in
the Astronomy book written by one of the speakers of this
presentation) The “Equation of the Centre” is
fundamental to understand how to calculate season’s
duration.
We are going to use some diagrams
with the three Suns we have already defined. You can clearly
appreciate what Function Q (“Equation of the Centre”)
represents on this diagram—the difference in the ecliptic
longitude of the True Sun and the Fictitious one.
We remind that the True Sun moves
at variable speed throughout a year. It is so because it obeys
Kepler´s Laws, especially the 2nd, which relates the
areas swept by the Earth-Sun Vector. The Fictitious Sun, instead,
moves at steady speed along the same plane of the Ecliptic.
This Fictitious Sun will describe
360º angle in a Tropical Year of 365.2422 mean days In
fact, to be more accurate, this Fictitious Sun describes a
bit smaller angle because the Aries Point retrogrades 50.2”
every year. This phenomenon is called “Precession of
the Equinoxes” or “Retrogradation of Aries Point”.
Now, we are going to calculate spring
duration with the help of these concepts and the other three
season’s can be estimated likewise.
In the diagram, we can see both the
Ecliptic and the Equator planes, and the Perigee Point of
the Earth Orbit located between the “Tropic of Capricorn”
or “Winter Solstice” and Aries Point. In other
words, around January 2nd or 3rd , the Sun is on the furthest
end of the apsis line—the point where the Sun is nearer
to the Earth speaking about the apparent movement of the Sun
around the Earth, instead of the real movement of the Earth
around the Sun. All these concepts are the same considering
one or other movement.
The Sun at crossing the Perigee Point
on January 3rd, poses us a paradox because it makes us think
that when the Sun is nearer to the Earth, we are in winter
in our hemisphere. We clearly realise that this paradox does
not apply to Argentina. When the Sun is nearer to the Earth,
you are in summer.
Now then, following this reasoning,
we are representing the True and Fictitious Sun with the letters
T and F and it becomes clear that the difference from the
Perigee Point to both Suns is Q (“Equation of the Centre”).
In the Astronomy book mentioned before, it is:
Q = v – nt = 2.e.sin nt + 5/4
e2.sin 2.nt
where v
and nt are true and mean anomalies respectively.
The value of nt represents the daily mean
movement of the Sun, i.e. the angular speed of the Fictitious
Sun. The value of e in the formula represents
the eccentricity of the Earth orbit. e = 0.0168.
For our calculus, we are going to
use the expression that relates true and mean anomalies. We
move nt, and we have
nt = v – 2.e.sin nt - 5/4 e2.sin
2.nt
We calculate the value of nt
with this expression and successive reiterations. Then, we
will have the point when the True Sun is in Aries and the
same when it is in the Tropic of Cancer. These are the points
where spring begins and ends. Our calculus starts by assuming
that nt = v. The value of v is
360º - 282º 56´18”
= 77º 03´42”
Please remember that
282º 5618” is Perigee longitude.
In this way, we obtain a
first value for nt. Then we substitute it
in the previous equation and we calculate again nt.
And we continue like that until we get a value which is not
very different from the previous one. This value corresponds
to the position of the Fictitious Sun when the Spring begins.
It tells us the nt value at the beginning
of the season.
With the help of a calculator,
we solve the problem and we get successively the following
angles for the value of x in the diagram:
77º
03’ 42”
75º
11’ 29.81”
75º
12’ 19.47”
75º
12’ 19.08”
75º 12’ 19.09”
When the True Sun has advanced
other 90º, the spring will finish. Following the same
method as before, we get the following successive values for
y :
167º
03’ 42”
166º
38’ 33.82”
166º
37’ 45.80”
166º
37’ 44.28”
166º
37’ 44.23”
Then, spring will last:
y – x = 91º 25’ 25.14"
This value is equivalent
to 92 days, 18 hours 12 minutes and 16 seconds.
We consider the year
is 365.2422 days long, the time the Fictitious Sun describes
360º, and we take this reference value to convert degrees
into hours and the like.
Following analogue reasoning,
we could get m and n values
which give us the Fictitious Sun positions at the beginning
of autumn and winter.
m
= 258º 55’ 42.53”
n
= 347º 29’ 02.31”
Taking the diagram as a
guide, it is easy to see the length of the four seasons:
Spring:
y – x = 91º 25’
25.14” = 92 days 18 hours 07 minutes and 06 seconds
Summer:
m – y = 92º 17’ 58.30” = 93
days 15 hours 26 minutes and 44 seconds
Autumn:
n – m = 88º 33’ 19,78” = 89
days 20 hours 16 minutes and 49 seconds
Winter:
p + x = 87º 43’ 16.78” =
88 days 23 hours 58 minutes and 07 seconds
We could check these times
using the data of a yearbook that contains the dates the seasons
begin. We would be able to see that they coincidence with
the ones we have calculated.
Adding up the four results
corresponding to season's duration, we get 365 days 4 hours
48 minutes and 46 seconds: This value equals the 365.2422
days that represent the Tropical Year length. It is rather
curious to see that the difference between winter and summer
is almost four days.
Evidently, it is not necessary
to insist that seasons are reversed in the southern hemisphere.
However, please remember that when we speak about spring it
corresponds to autumn in the southern hemisphere. Likewise,
when we refer to summer, autumn and winter on our hemisphere,
it corresponds to winter, spring and summer respectively on
the other hemisphere.
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