INX300_ProjectChoice2_VirtualAstronomy (1)
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Astronomy
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Dec 6, 2023
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INX300: Astronomy
Seneca College
2023
Choice 2: Exploring the Night Sky with Stellarium
Web
20% of the course mark. Due by Dec.1
.
In this project you will use the free browser-run version Stellarium
Web
https://stellarium-web.org/
to
virtually “observe” the night sky and the visible planets, to collect and analyze data of stars and
stellar clusters. Stellarium
Web
has the advantage that it does not require download and setting up of
multiple options, unlike the full version (also free and available from
https://stellarium.org
).
Stellarium
Web
has only a few basic settings, while still correctly representing the night sky for the
chosen times and locations.
In Part 1 of the project you will view planets visible in the evening sky and summarize their
properties. In Part 2 you will explore and analyze properties of stars in one constellation of the
season. In Part 3 you will analyze open clusters of stars.
You can choose to work in a group of 3 students and do all 3 parts of the project. It is recommended
to split the work in a way that you contribute to each part. If you work alone choose either Parts 1
and 2, or Parts 2 and 3.
Familiarize yourself with the
Stellarium
Web
options first:
Fig.1. The Stellarium
Web
screen with the viewing options.
Course Project - Choice 4
Prof. M. Nenkova
1
INX300: Astronomy
Seneca College
2023
Open Stellarium
Web
(
https://stellarium-web.org
)
,
set the observing location
to Toronto and the
time
to an evening in March 2023. Set the
viewing options
for constellations (on), landscape (on),
atmosphere (off for better seeing), deep sky objects (on).
In
View Settings
in the upper left corner set Ecliptic Line on. Fast forward the time controls by
holding the cursor over the arrows for minutes or hours. Scroll the mouse wheel to zoom in and out
and notice how the FOV (field of view) changes. Drag the mouse to look in different horizon
directions. Click on various objects (planets, stars, star clusters, galaxies) and read the
information panel appearing in the upper left. Center on the object by clicking on this
button,
then zoom on the centered object.
Part 1: Virtual Observations of Planets in Fall 2023
In your report state all planets that are above the horizon for your choice of an evening time and
date (in Fall 2023 semester). Write down their Stellarium magnitudes and distances from Earth (in
A.U.). Take a screenshot of Stellarium
Web
(with FOV between about 90
o
and 120
o
) that shows the
planets, the ecliptic line, the date and time of your virtual observation, and insert it in your report.
Jupiter and its Galilean moons.
Set the date and time to see Jupiter above the horizon, and turn off the atmosphere to darken
the sky.
Center on the planet. Zoom in the field of view to see details on Jupiter and its moons.
To
observe Jupiter’s rotation
click and hold the pointer on the minutes to fast-forward time.
Measure and record how much time the Great Red Spot needs to transit (to cross the visible
disk of Jupiter)
.
Adjust the zoom (the FOV) to
observe the orbital motions of the Galilean moons
(Io, Europa,
Ganymede and Callisto) and take a screenshot to insert in this part of your report.
Measure
the approximate transit times
of each moon (the time it takes to go across Jupiter) as you fast-
forward the minutes. Record your results in Table 1.
Explore the 4 Galilean Moons.
After recording the transit times record each moon’s radius, as
shown in Stellarium
Web
. Compare to Earth’s
Moon radius of 1,737 km
by showing the ratio of
each Jupiter’s Moon radius to Earth’s Moon’s radius. Ex., if a moon’s radius is 1560 km, you will
show the ratio of 0.90 in the table. (Round-off to 2 digits after the decimal point.)
Table 1
(adjust the column sizes as needed)
Jupiter’s moon
Io
Europa
Ganymede
Callisto
Time for Transit
(hrs:min)
Radius (km)
Jupiter’s moon
radius to Earth’s
Moon radius
Surface
Features seen
in Stellarium
Web
Course Project - Choice 4
Prof. M. Nenkova
2
INX300: Astronomy
Seneca College
2023
Write a paragraph summarizing the similarities and differences among these moons of Jupiter.
You will have to use external references (
https://solarsystem.nasa.gov/moons/jupiter-
moons/in-depth/
and or the textbook). Cite them in-text, and list them at the end of your work
in APA format.
Part 2: Analysis of Stars in a Constellation
Set the date and time for a fall evening in Toronto (or another location of your choice). Have FOV
about 100
o
for a realistic representation of what you could see in the sky if you were outside at the
set location and time
.
When you click on a star you will see the information panel with the star’s
names in various catalogues (see Fig.2). Under the star’s name is the apparent magnitude, distance
(in light years) and spectral type of the star.
Fig. 2 Screenshot of the night sky in Stellarium
Web
with selection of a bright star.
Explanation of stellar properties that you will virtually “measure” in Stellarium
Web
:
The
apparent brightness
of stars is measured in apparent visual magnitudes, denoted with the small
letter
m
. Stellarium
Web
lists the apparent magnitude, as seen in the sky. This is different than the
intrinsic power of stars, called luminosity. A star may appear dim, but this could be because the star is
far away, not because the star is not powerful. The
apparent magnitude scale
introduced by the
Ancient Greek astronomers has numbers increasing inversely to brightness. The brightest stars have
small numbers for apparent magnitudes (typically less than m=2.5), while the faintest stars, visible by
a person with perfect vision, have apparent magnitude of m=6.0.
A number of bright stars and
planets have m=0.0 and even negative magnitudes (see
Fig.17.2 in the OpenStax
astronomy
Course Project - Choice 4
Prof. M. Nenkova
3
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