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Southern Constellations
To the right hand I turned, and fixed my mind
Upon the other pole, and saw four stars
Ne'er seen before save by the primal people.
Rejoicing in their flamelets seemed the heaven.
O thou septentrional and widowed site,
Because thou art deprived of seeing these!
--Dante
Purgatorio: Canto I
Overview
●
Understand visibility of the constellations from different latitudes on Earth.
●
Become familiar with constellations and features of the southern sky.
Introduction
Origin of the Southern Constellations
There are 88
constellations
officially recognized by the International Astronomical Union, each of which has official
boundary lines to divide up the sky. Fifty-two of the constellations have origins in Ptolemy's
Almagest
catalog (ca. AD
150). The remainder, including the constellations of the deep south, were invented by Europeans of the 17th and 18th
centuries. Star catalogs and constellations created by the Dutch explorers, Frederick de Houtman and Pieter Keyser, were
mapped by their countryman, Petrus Plancius in 1598. These Dutch constellations represented flora and fauna of the East
Indies and Madagascar. Johannes Hevelius, the Polish astronomer and cartographer, invented 7 northern and equatorial
constellations that received IAU endorsement. These were published in his famous atlas,
Firmamentum Sobiescanum
in
1690. The prolific French astronomer Nicolas Louis de Lacaille catalogued and created the remaining 14 of the standard
constellations in 1754, which represent tools of science and art.
A prominent southern Ptolemaic constellation was
Argo Navis,
the ship
Argo
of the Greek hero Jason, and the Argonauts.
This constellation was so huge that it was divided into three smaller constellations, Puppis, the Stern; Carina, the Keel;
and Vela, the Sails.
The most distinctive southern constellation is Crux, the Cross, which is also known as the Southern Cross. This
constellation was visible to the ancient Greeks before 1000 BC, and considered part of the constellation Centaurus, the
Centaur. However, due to precession (see the Precession Activity), Crux slipped below the horizon in the ancient world,
and was not included in Ptolemy's list. Crux was later known anecdotally by 16th century European sailors, and was
officially included as a constellation by Plancius.
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Another noteworthy Plancius constellation is Indus, the "Indian". Since the Dutch explorers went to Madagascar and the
East Indies, Indus by his name clearly represents a native of the East Indies, today's Indonesia. Plancius originally
represented Indus with only a loincloth and spears. Later cartographers represented him with feathers, the attribute of
Native Americans.
Many people consider the southern sky to be more splendid to the naked eye than the north. Among the treasures to be
seen are the two largest satellites of our Milky Way Galaxy, the Large and Small Magellanic Clouds. They are clearly
visible to the naked eye, indeed appearing like small clouds. Another interesting object is the largest globular cluster in the
Galaxy, ω Cen, which is so huge that it may represent the core of a dwarf galaxy whose stars have been tidally stripped
off. Also in Centaurus is the nearest Sun-like star, α Cen. The center of our Galaxy transits at a much higher altitude in the
southern hemisphere, enhancing the visibility of the many nebulae and clusters in that direction. In this activity, you will
explore constellations and features of the southern sky.
Constellation Visibility
Recall that
circumpolar
constellations are those that are close enough to the celestial pole that they remain mostly above
the horizon all the time as the sky turns (See Figure 1, for the northern hemisphere). The other visible constellations are
seasonal constellations that rise and set (see the Out of Seasons Constellations activity). You know that the seasons in the
southern hemisphere are reversed from those in the northern hemisphere. (This is explored in detail in the Seasons
Activity.) So how does your latitude affect which parts of the sky, and which constellations, you can see, and when?
Figure 1: Equatorial grid for the northern hemisphere.
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Figure 2: Relation between latitude, declination, and visibility.
The observer is standing at latitude l on the Earth, in the
northern hemisphere.
Figure 2 shows how the visible range of declination on
the sky is related to your latitude. The northern-most
declination visible for the northern hemisphere is dec =
90º, the north celestial pole. The figure shows how your
zenith always has a declination equal to your latitude
(
l
).
Your horizon is 90° from your zenith, and so the
southern-most declination visible, set by your horizon, is
dec =
l
-90º. (For the southern hemisphere, the
northern-most declination visible is
l
+90, for negative
l
.)
Now consider the circumpolar constellations. As seen in
Figure 2, the altitude of the north celestial pole is also equal to your latitude
l
(recalling from the Coordinate Systems
activity that altitude is measured up, from the horizon). This means that circumpolar stars must have an angular distance
from the pole less than
l
. It may be helpful to refer to Figure 1 as well.
Additional Resources
●
Star Charts
(print out Southern Chart)
●
Ian Ridpath's
Star Tales
.
●
Do-it-yourself southern hemisphere planisphere at
http://www.handsonuniverse.org/activities/uncleal/
.
Original MSO, updated 10/8/20
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Southern Constellations: Worksheet
Part 1: Constellation Visibility
1.
Your GSI will show the sky in Ann Arbor (lat 42º N) at midnight on March 21, which is the northern spring
equinox. Determine whether you see each of the constellations in Table 1. Fill in the row for Ann Arbor. If a
constellation is visible
and
it is also circumpolar, write "C". Otherwise, write "Y" or "N" for the visibility. If the
constellation is visible, also write its declination in the first row.
2.
Your GSI will adjust the sky to show how it appears
on the same date
, at the other two locations, the equator and
Santiago, Chile. At each location, the GSI will turn the sky through one night, so you can observe the rotation of
the sky at each location. Continue completing Table 1.
Table 1: Constellation Visibility
Location
Ursa Major
Leo
Corvus
Crux
Declination of
Constellation
Ann Arbor
latitude 42º N
Equator
latitude 0º
Santiago
latitude 33º S
3.
Does your latitude affect a constellation's visibility?
4.
Can people in Ann Arbor and Santiago see any of these same constellations on the same night? If so, which
one(s)?
5.
The GSI will point out the position of the South Celestial Pole. Is there a pole star analogous to Polaris?
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Part 2: Identifying Constellations on the Sky
The GSI will set the sky for Santiago, Chile (latitude 33º S) on the following dates at 10pm: April 1 and Oct 1.
1.
Identify which constellations are visible in the shown season. Note that the constellations are listed in order of
RA. Find the general direction in which to look for each constellation visible in this season. Include both altitude
and azimuthal direction. For example, you might say high in the south, or low in the west-northwest (WNW).
Enter this in Table 2. In each group, each person should be responsible for identifying at least one object in each
season for the next part of the activity. In the "Origin" column, specify whether the constellation is due to Ptolemy
and the ancient Greeks (G), Plancius and the Dutch explorers (D), or Lacaille (L).
2.
Your GSI will identify additional objects from the list below. Note the type of object for each one.
a.
Small Magellanic Cloud: __________________________
b.
Large Magellanic Cloud: __________________________
c.
ω Centauri: _______________________________
d.
The False Cross: __________________________
e.
Argo (Puppis, the Stern; Carina, the Keel; and Vela the Sails) ____________________________
3.
The GSI will move the planetarium to the next season. Repeat the above steps to find your next object. Look out
for any constellations that may appear in both seasons. Make two entries for these constellations.
Table 2: Some Southern Constellations
Name
Represents
Origin
Season
Direction
1
Eridanus
The River
Eridanus
2
Grus
The Crane or
Hornbill
3
Indus
The Indian
Man
4
Octans
The Octant
6
Centaurus
The Centaur
7
Crux
The Cross
8
Vela
Sails of Argo
9
Carina
The Keel of
Argo
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Concluding Questions:
1.
Can you see southern constellations (having negative declinations) from the northern hemisphere? Explain. How
far south in declination can we see from Ann Arbor? Show your work, using Figure 2.
2.
In the northern hemisphere, Polaris can be used to identify the north celestial pole. Review your answer to
Part 1, Question 5. Why don't both poles have a pole star?
3.
From which location on Earth can you see more constellations throughout the year: the equator, the south pole, or
do you see the same number from both places? Explain.
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4.
Is Orion visible at night in the southern hemisphere during the same months of the year as in the northern
hemisphere? The same seasons as in the northern hemisphere? Explain.
5.
What range of declination is seen as circumpolar from Santiago? Explain and show your work. You may want to
make a figure analogous to Figure 2. Which constellations from Table 2 are circumpolar from Santiago?
Original MSO, updated 03/14/22
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