Astronomy Report
Southern Cross Constellation
PDF version of this report (prints in 10 or less pages).
Authors
Felipe Garrido Goicovic
Matias Marchant Taborga
Juan Soto Rosales
Mario Campos Duque (teacher)
School
Colegio Cristóbal Colón
Santiago de Chile
Pasaje Berna 1658, Conchalí
colcrico@ctcreuna.cl
Acknowledgements
The authors acknowledge the support provided by the Chilean Astronomy Network (RChA, Red Chilena de Astronomía, http://www.rcha.cl) during the production of this work. The Spanish version of this report has been freed to the public domain under the terms of the License RChA.
2003
The Southern Cross
One of the constellations more easily seen during the whole year in the South Hemisphere is the Southern Cross (in Spanish “Cruz del Sur”). This is a group of stars readily observable (due to its simple shape) which has been object of veneration in diverse cultures, providing guidance and inspiration for a long time. One of the telescopes at Cerro Paranal [1] has been named after the Southern Cross using the mapudungún name for it, Melipal [2], which means “four tips” (as in the tips of arrows). (N.B.: Mapudungún is the language of the Mapuche, the native people living in central and southern Chile).
Our report includes the following aspects:
· The Southern Cross as lighthouse of literary inspiration.
· Knowing the Southern Cross astronomically.
· The Southern Cross in comparison to the Northern Cross.
· The Southern Cross and the mythology of the original cultures of the Andes.
· Classroom activity.
I. The Southern Cross as lighthouse of literary inspiration
Diverse authors have mentioned the Southern Cross in their works. Dante is one of them. In the Divine Comedy he writes in the first canto of the second part: “I turned right and, directing my attention to the other pole, I distinguished four stars only seen by the first humans. The sky seemed to rejoice in their shine...”. [3]
A Chilean author, the Literature Nobel Prize winner Pablo Neruda, wrote in his book “One hundred love sonets” (poem LXXXVI): “Oh Southern Cross, oh threefold of fragrant phosphorum / with four kisses today it penetrated your beauty / and went through the shadow and my hat: / the moon was round because of the chill. / Then with my love, oh diamonds / of blue frost, serenity of the sky, / mirror, you appeared and all was full of night / with your four depots trembling of wine.” [4]
These two examples make us think on how this constellation has inspired different poets which, from different latitudes and from different ways of viewing it, have found themselves captivated by this stellar cross; Dante, in the XIII c., observing from far away, and Neruda, in the XX c., from the austral Temuco [5], observing its whole grandeur.
II. Knowing the Southern Cross astronomically
This constellation is one of the 88 classified by the International Astronomical Union in 1930. Formerly it was part of Centaur after a classification by Ptolemy. Due to the precession of the Earth the Southern Cross became invisible from the North Hemisphere. It was split from Centaur by A. Royer in 1679. [6]
The shape of this constellation is that of a cross. It is formed by 4 outstanding stars and a dark nebula. It can be distinguished from other cross found in the same hemisphere (the False Cross) because it has a fifth star near its centre.
Its coordinates are A. R. 12.45 h and Dec. -59.97 degrees, visible between parallels 20 degrees N to 90 degrees S. Its area is 68 square degrees.
Image by astrophotographer Pedro Aguirre V. (http://astrosurf.com/pedro)
In Table 1 we show data for the 11 brightest stars of this constellation. We present data for position, magnitude and spectral class of each star.
Table 1 - Source: Catálogo de Brillos de Estrellas [7].
HR |
Common Name |
Bayer |
VarID |
RA |
DEC |
mag |
MK Spectral Class |
Multiple |
|
4853 |
Becrux (Mimosa) |
Beta |
Bet Cru |
12h 47m 43.2s |
-59° 41' 19" |
1.25 |
B0.5III |
3 |
|
4730 |
Acrux |
Alpha [7] |
|
12h 26m 35.9s |
-63° 5' 57" |
1.33 |
B0.5IV |
3 |
|
4763 |
Gacrux |
Gamma |
5672 |
12h 31m 9.9s |
-57° 6' 48" |
1.63 |
M3.5III |
3 |
|
4731 |
|
Alpha [8] |
|
12h 26m 36.5s |
-63° 5' 58" |
1.73 |
B1V |
3 |
|
4656 |
|
Delta |
Del Cru |
12h 15m 8.7s |
-58° 44' 56" |
2.8 |
B2IV |
|
|
4700 |
|
Epsilon |
5568 |
12h 21m 21.6s |
-60° 24' 4" |
3.59 |
K3-4III |
|
|
4898 |
|
Mu [7] |
|
12h 54m 35.6s |
-57° 10' 40" |
4.03 |
B2IV-V |
|
|
4679 |
|
Zeta |
|
12h 18m 26.1s |
-64° 0' 11" |
4.04 |
B2.5V |
|
|
4616 |
|
Nu |
|
12h 6m 52.9s |
-64° 36' 49" |
4.15 |
F2III |
|
|
4599 |
|
Theta [7] |
|
12h 3m 1.5s |
-63° 18' 46" |
4.33 |
Am |
|
|
4897 |
|
Lambda |
Lam Cru |
12h 54m 39.2s |
-59° 8' 48" |
4.62 |
B4Vne |
|
Acrux is one of the brightest stars in the sky, being the twelfth in bright. Other interesting Southern Cross data are the distances, temperatures, solar radii and absolute magnitudes, as obtained from the software Starry Night. [7]
Table 2 - Source: Software Starry Night, version 3.1.
HR |
Bayer |
Distance |
Temperature |
Solar Radius |
Absolute Magnitude |
|
4853 |
Beta |
353 |
20.695 |
6,4 |
-3.92 |
|
4730 |
Alpha [7] |
321 |
21.259 |
7,1 |
-4.22 |
|
4763 |
Gamma |
88 |
3.276 |
269 |
-0.6 |
|
4731 |
Alpha [8] |
|
|
|
|
|
4656 |
Delta |
364 |
16.569 |
4,7 |
-2.46 |
|
4700 |
Epsilon |
226 |
3.738 |
129 |
-0.66 |
|
4898 |
Mu [7] |
379 |
15.620 |
3 |
-1.33 |
|
4679 |
Zeta |
362 |
14.819 |
3,1 |
|
|
4616 |
Nu |
64,3 |
7.144 |
2,3 |
|
|
4599 |
Theta [7] |
231 |
7.477 |
6,8 |
|
|
4897 |
Lambda |
360 |
13.904 |
2,7 |
|
The following images were obtained from Simbad (astronomical database). [9]
Acrux |
Becrux |
Gacrux |
Delta crux |
Epsilon crux |
|
Comparing the images with the spectral class of the stars (see Table 2), and using as a reference the classification by Morgan and Keenan, we see that:
Table 3
HR |
Bayer |
Absolute Magnitude |
Class of star |
|
4853 |
Beta |
-3.92 |
Giant, white-blue, cepheid |
|
4730 |
Alpha [7] |
-4.22 |
Subgiant, white-blue |
|
4763 |
Gamma |
-0.6 |
Red giant |
|
4731 |
Alpha [8] |
|
Dwarf or from the main sequence |
|
4656 |
Delta |
-2.46 |
Subgiant |
|
4700 |
Epsilon |
-0.66 |
Giant |
|
4898 |
Mu [7] |
-1.33 |
Subgiant |
|
4679 |
Zeta |
|
Dwarf or from the main sequence |
|
|
Nu |
|
|
|
|
Theta [7] |
|
|
|
|
Lambda |
|
|
Another interesting information we are able to show about this constellation is the location of the stars in relation to the Milky Way.
Table 4 - Source: Catálogo de Brillos de Estrellas [7].
|
Acrux |
Member of the Scorpio Centaur cluster. |
|
Betacrux |
Probably a member of the cluster Sco-Cen; member of the association Sco-Cen; member of the Pleiades group. |
|
Delta Cru |
Probably a member of the Scorpio Centaur cluster. |
|
Epsilon Cru |
Hyades group. |
Other objects we can distinguish in the Southern Cross are the following:
Table 5 - Source: Catálogo de Brillos de Estrellas [7].
|
Name |
HR |
Object |
Magnitude |
|
NGC |
4755 |
Open cluster |
4,2 |
|
NGC |
4609 |
Open cluster |
6,9 |
|
Ru |
98 |
Open cluster |
7 |
|
Harvard 5 |
|
Open cluster |
7,1 |
|
NGC |
4103 |
Open cluster |
7,4 |
|
NGC |
4349 |
Open cluster |
7,4 |
|
NGC |
4439 |
Open cluster |
8,4 |
|
NGC |
4052 |
Open cluster |
8,8 |
|
NGC |
4337 |
Open cluster |
8,9 |
|
Ru |
97 |
Open cluster |
9,1 |
|
Hogg |
14 |
Open cluster |
9,5 |
|
Tr |
20 |
Open cluster |
10,1 |
|
Hogg |
15 |
Open cluster |
10,3 |
|
PK |
298-0,1 |
Planetary nebula |
11 |
|
PK |
300-0,1 |
Planetary nebula |
11,7 |
|
PK |
298-1,2 |
Planetary nebula |
12,4 |
|
PK |
299+2,1 |
Planetary nebula |
12,7 |
|
PK |
300+0,1 |
Planetary nebula |
12,9 |
|
PK |
299-0,1 |
Planetary nebula |
13,6 |
|
PK |
300-1,1 |
Planetary nebula |
13,8 |
The most interesting cluster in the Southern Cross is the Jewel Box (NGC 4755):
|
Image: Space Telescope Science Institute. |
Image by astrophotographer Pedro Aguirre V. (http://astrosurf.com/pedro). |
Image: http://simbad.u-strasbg.fr/sim-fid.pl
Some magnitudes in the Jewel Box:
Table 6 - Source: http://www.seds.org/messier/xtra/ngc/n4755.html
|
Right ascension |
12h 53.6’ |
|
Declination |
-60 degrees 20’ |
|
Distance |
7600 light years |
|
Visual bright |
4,2 magnitude |
|
Apparent size |
10 arcmin |
Nicolas Lacaille discovers and then mentions the Jewel Box in Coelum Australe Stelliferum in 1763. This is a young star cluster, approximately 7 million years old. [10]
NGC 4755 is made up of diverse stars from which we highlight the following:
Table 7 - Source: http://simbad.u-strasbg.fr/Simbad
|
|
Name |
Star type |
B mag |
V mag |
Spectral class |
|
1 |
HD 111990 |
Star in Double System |
7.01 |
6.77 |
B1B2Ib |
|
2 |
SAO 252075 |
Ellipsoidal variable Star |
8.165 |
7.962 |
B0.5 Vn |
|
3 |
HD 111904 |
Variable Star |
6.09 |
5.80 |
B9Ia |
|
4 |
SAO 252073 |
Variable Star of irregular type |
9.82 |
7.66 |
M2Iab |
|
5 |
HD 111934 |
Variable Star |
7.15 |
6.91 |
B2Ib |
|
6 |
HD 111973 |
Star in Cluster |
6.10 |
5.9 |
B5Ia |
The most remarkable dark nebula of the South, located in the Southern Cross, is the Coal Sack. This nebula is on the galactic plane, about 150 pc from the Sun [6]. It is known since prehistory in this hemisphere. It was observed in 1499 by Vicente Yáñez Pinzón [10].
Some data about this nebula:
Table8 - Source: http://www.seds.org/messier/xtra/ngc/n4755.html
|
Right ascension |
12h 52’ |
|
Declination |
-63 degrees18’ |
|
Distance |
2000 light years |
|
Apparent size |
420 by 240 arcmin |
This nebula is composed of stellar dust that blocks the path of light. Here we see the Coal Sack (in Spanish: Saco de Carbón) in sheer splendour:
Image by astrophotographer Pedro Aguirre V. (http://astrosurf.com/pedro)
III. The Southern Cross in comparison to the Northern Cross.
Image: http://faculty.rmwc.edu/tmichalik/mlkywayc.htm
The image shows the two crosses: Cygnus to the left and Crux to the right. Both extend across the galactic equator. The following data illustrates similarities and differences between the crosses of both hemispheres.
|
|
Southern Cross |
Cygnus |
|
Icon |
|
|
|
Image |
|
|
|
Apparent magnitude |
Becrux 1.25 |
Deneb 1.25 |
|
Nebula |
Coal Sack (dark nebula) |
NGC 7000 (bright nebula) |
|
Cluster |
Jewel Box (NGC 4755) Open cluster, A-shaped. |
M29 Open cluster; shaped as a spoon. |
|
Name |
Southern Cross |
Northern Cross |
|
Stars of apparent magnitude < 3 |
4 |
4 |
|
Visible in the range of latitudes... |
20 to –90 degrees |
90 to –40 degrees |
|
Area |
68 square degrees |
804 square degrees |
IV. The Southern Cross and the mythology of the original cultures of the Andes.
In a legend about the origin of the Mapuche the Southern Cross is mentioned. In the “Book of Mapuche tales”, compiled by Alicia Morel, we read:
“ The children built a ruca (a Mapuche hut) and the Sun entered by the door facing East and left by the one facing West, following the ancient custom of the people of the land, respectful of the cardinal points and regarding the number four as sacred.
When at last the Maker of Rain was tired of riding over the clouds and returned to its hiding place behind the hills, water level began to descend and the rivers to follow their normal course. Then the coihue (a native tree) buried itself in the mud as a ship running aground, and when the wind dried the ground the Puma (a native feline) , the Chilla (a native mouse) and the children jumped from the log and looked for a hidden valley to live.
The first thing they did, even before building another ruca or looking for a cave to inhabit, was to name their adoptive children. Magical names that would protect them forever. The son was named Manque, the condor that soars in the sky looking after the Earth. The daughter was named Melipal, like the Southern Cross.”

