AST - Mininger Lucas - Module8 Assignment The Phases of Venus
.docx
keyboard_arrow_up
School
Chattanooga State Community College *
*We aren’t endorsed by this school
Course
1010
Subject
Physics
Date
Feb 20, 2024
Type
docx
Pages
2
Uploaded by DrMantisMaster763
Phases of Venus – Exercise Materials - Student Name: Lucas Mininger 1.
Exercise Activities
Step 1. A.
Start Stellarium. It should be in the default configuration you setup in the Using Stellarium exercise. You should be viewing to your South and set the program to full screen. B.
Use the Date/Time Window to set the date to 2010/1/10 and the time to 17:00:00 and leave the Date/Time Window in the upper right hand corner of the screen. Set the FOV to between 30
°
and 35
°
. C.
Move the horizon until the West compass mark is on the far right side of the screen. Keep the horizon low on the screen. You are now facing Southwest just prior to sunset during a Superior Conjunction of Venus and therefore Venus is in a Full Phase (Venus appears very close to the Sun). D.
Now use the Search Window to locate Venus. E.
Now turn off the atmosphere and the landscape. Step 2. A.
Zoom into to a FOV of about 0.03° . You can see that, viewed from Earth, Venus is fully illuminated. B.
Use the Date/Time Window to advance the date by four months. Leave the Window up in the upper right
corner.
■
Question 1: What is the general phase of Venus at this point? 42 degrees 48’ 14.8’’ ■
Question 2: If you noticed any other change(s) in Venus' appearance, describe it/them.
Its dark on the left side, similar to how the moon looks sometimes ___________________________________________ A.
Advance the time by five months. you should be at 2010/10/10 . ■
Question 3: What is the general phase of Venus at this point? 142 degrees 00’ 55.4’’ ■
Question 4: You should now notice a significant change in Venus' appearance, can you describe it?
It looks the opposite as before. Similar to a toenail _______________________________________________________ ■
Question 5: Can you explain why this change in appearance has taken place?
The view from earth is changing over time because venus is orbiting and reflecting the sun differently
_______________________________________________________ A.
Continue to advance the time in one month intervals until Venus is in Full Phase. ■
Question 6: How many months have you advanced since you started the exercise? 9 ■
Question 7: What is this time in years (divide the number of months by 12 to get decimal years)?
.75
_______________ ■
Question 8: What is this time in days (multiply the number of decimal years by 365.25 to get decimal days)?
273.9375
_______________ ■
Question 9: Is this the Orbital Period, or the Synodic Period? sydonic Period Step 3. A.
Use the Date/Time Window to reset the date to 2010/1/10 and the time to 17:00:00 . B.
Using the Location Window, set the location to "Solar System Observer". You are now looking down on the plane of the Ecliptic. From here we can observe the orbits of the inner planets C.
Use the Search Window to select the Sun.
D.
Note the current position of Venus relative to the Sun
■
Question 10: What is the term for the currently set relationship between the Earth, Sun and Venus?
Superior conjunction
______________________________________ A.
Now use the Date/Time Window to advance the date by one month. B.
Notice that as you advance the time, that all the planets move, not just Venus. C.
Now continue to advance the date in one month increments until the Sun, Earth and Venus are once again close to alignment. ■
Question 11: What is the term for the currently set relationship between the Earth, Sun and Venus?
Inferior conjunction ______________________________________ ■
Question 12: About how many months did you advance to get to this configuration?
10
____________________ A.
Use the Date/Time Window to reset the date to 2010/1/10 and the time to 17:00:00 . B.
Again, note the position of Venus. C.
Advance the date in one month increments until Venus returns to a point close to the same location (relative to the Sun), but just past. D.
Now backup one month. ■
Question 13: About how many months did you advance to get to this configuration? (it will be
between two months, so just use the half month in between, e.g. between 1 and 2 would be 1.5 months, etc.)
7.5
____________________ ■
Question 14: How many years (in decimal) did it take for this period (divide the number of months you got by 12)?
.625
____________________ Step 4. A.
Using the actual values for Venus: ■
Orbital = 0.62 years ■
Synodic = 583.92 days and using Equation 1. to calculate % error.
A.
Question 15: What is your percent error for the Orbital period?
.005 B.
Question 16: What is your percent error for the Synodic period?
53%
1.
Exercise Materials
((Measured value - Actual value)/Actual value) x 100%
Your preview ends here
Eager to read complete document? Join bartleby learn and gain access to the full version
- Access to all documents
- Unlimited textbook solutions
- 24/7 expert homework help
Related Questions
Which of the following statements accurately describes our current understanding of the solar system?
a.
There are no metals in the solar system beyond Jupiter and its orbit.
b.
Terrestrial worlds are so small because their large atmospheres were stripped away in time by Jupiter.
c.
Jupiter and Saturn are made of strictly a combination of hydrogen and helium, and both objects lack a planetary core.
d.
Various ices can contribute to the mass of planetary cores if we are at a great enough distance from the sun.
arrow_forward
20.
DETAILS
PREVIOUS ANSWERS
SEEDSFOUNDATIONS14 21.P.007.
MY NOTES
PRACTICE ANOTHER
If the Magellan spacecraft transmitted radio signals down through the clouds on Venus and heard an echo from a certain spot 0.000115 second before the main echo, how high is the spot above the average surface of Venus in
m and km units? (Note: The speed of light is 3.00 x 10 m/s.)
in m
x m
in km
X km
Enter a number.
Need Help?
Read It
Submit Answer
arrow_forward
Johannes Kepler worked as an assistant to the observatory of Brahe at the age of 27.
Brahe collected astronomical observations, which were passed into Kepler, on his death.
Among the significant contributions of Brahe:
1. His observations on the planetary motion of Mars were used by later astronomers, including
Kepler to construct the present model of the solar system.
2. In 1572, he observed supernova as a star that appeared suddenly, became visible for 18
months before it faded from view. Nowadays, supernova is called an exploding star.
3. In 1577, he observed a comet by measuring its parallax. His claim contradicted the idea of
Aristotle that comets are "gases burning in the atmosphere." By measuring the parallax for
the comet, he was able to show that the comet was further away than the Moon.
4. His findings that stars do not have parallax, he concluded that either: (a). the earth was
motionless at the center of the universe; or (b). the stars were so far away that their parallax…
arrow_forward
Please answer parts C and D
arrow_forward
19. A laser beam takes 0.024s to jravel from a rocket to the reflective surface of a planet and back to the
rocket. How far is the rocket from this planet's surface?
a) 2400 km
b) 1200 km
c) 1800 km
d) 3600 km
e) 4800 km
Class comm
arrow_forward
QUESTION 1
Estimate The Temperature For A Planet In Other Solar System (Questions 1-3)
Let us assume scientists just discovered a planet orbiting a star in an extra-solar system. The star has a surface temperature Ts = 10000 Kelvins and a radius Sr = 1x109 meters. Scientists also measured the distance (D)
between the star and the planet as D = 2 AU - 3.0x1011 meters.
The solar power per unit area from the star's surface (Ps) can be calculated from the star's surface temperature Ts (10000 Kelvins) by the Stefen-Boltzman law Ps=0(Ts)4, where o is Stefen-Boltzman constant (5.67 x 10-8
Watt/meter2/Kelvin4). What is the solar power per unit area from the star's surface (Ps)?
O Ps ~ 2.87 x 108 Watt/meter2
O
Ps ~ 5.67 x 108 Watt/meter2
O
O
Ps ~ 2.87 x 10 Watt/meter2
Watt/meter²
Ps ~ 5.67 x 10⁹
QUESTION 2
The solar power (Ps) decreases from the star's surface to the distance at the planet. Assuming the solar power per unit area at the distance of the planet as Pp, we have Pp=Ps(Sr/D)2, where…
arrow_forward
Answer question based on spacecraft mission “SunL1”
arrow_forward
I. MULTIPLE CHOICE
For items 1-10
Directions: Read and understand the statements/questions. Write your best answer on the space provided.
(ERASURES ARE NOT ALLOWED)
1. Which of the following equations is not correct:
a. Density = Volume /Mass
b. Density = Volume /Mass
c. Density = Volume /Mass
d. Pressure = density x acceleration x height
2. Air pressure at sea level is 14.5 lbs/sq, inch. Why do we not feel this pressure pushing on us?
a. the amount is neglible to the feeling of gravity
b. we have grown accustomed to it since we were born
c. we have grown accustomed to it since we were born
d. the force of gravity negates the feeling of pressure
3. Where does the static fluid pressure at any given depth depend?
a. total mass
b. surface area
C. surface area
d. all of the above
4. In the equation for Pressure - P= rho xgxh. the units for g (SI system) are:
a. kg/m?
b. m/sec
C. kg - m/sec
d. m/sec?
5. What does Pascal's Principle state?
Any object, wholly or partially immersed in a fluid,…
arrow_forward
Q7
arrow_forward
step 2
Quecoon 4
It is hoped that the ExoMars
cover 100mper
Rover will be
Sol is a solar day on Mars
SOL. A SOL
and equal to 24 hoursko minubes.
calculate the average speed of
Show worlund
m 5-1 and bo bwo significant
the rover.
your
un
Signes
し
arrow_forward
PHYSICS
UPVOTE WILL BE GIVEN. NO LONG EXPLANATION NEEDED.
Which quantities are required to explain the orbital velocity of satellites in different celestial bodies?
a.Universal Gravitational Constant, mass, and r
b.Universal Gravitational Constant, frequency, and r
c.Mass and c (speed of light)
d.G, co, and radius
arrow_forward
Suppose there were a planet in our Solar System orbiting at a distance of 0.5 AU from theSun, and having ten times the mass and four times the radius of Earth. For reference, theEarth has a mass of 5.97 × 1024 kg and a radius of 6,378 km a) Calculate the density of this hypothetical planet.b) Based on your answer from part a), what do you think this planet would be made of?Explain your reasoning.c) Do this planet’s properties agree with the condensation theory for the formation of ourSolar System? Why or why not?
arrow_forward
Unit 3: Final Assessment
Use your Digital Interactive Notebook, Peardeck Notes, and
Science Weekly Reading for assistance.
Question #1:
Which evidence first supported the heliocentric model of the solar
system?
A. mapping of stars using the unaided eye
B. taking pictures of distant galaxies with satellite-based cameras
C. determining that planets orbit in elliptical paths with telescopes
D. observing the surface features of nearby planets and moons
with telescopes
arrow_forward
9
The discovery of Eris
A Was not surprising, because the existence of a massive "Planet X" had been predicted nearly a century ago.
B
Was surprising, due to its "backwards" orbit around the Sun.
C Was surprising, since we thought we knew about all large objects in the solar system.
Was not surprising, because other Kuiper belt objects approaching the size of Pluto had already been discovered.
D
arrow_forward
The close encounter hypothesis was rejected because of the following reasons except for this reason.
b. It explained the planets were formed by gravitational disruption
c. It failed to explain the orbital motions of planets
d. It failed to explain why the solar system have 2 types of planets: terrestrial and jovian
arrow_forward
Please explain in full detail as I am trying to understand this concept! thank you!
a. Sketch a diagram including Earth, Sun, and Mars, with attention to scale of distance (Mars is about 1.5 AU from the Sun) showing a faster trajectory from Earth to Mars than the minimal energy trajectory discussed in the lecture.
b. Without doing a calculation, how would the arrival velocity of the spacecraft at Mars for the case in (a) compare to the spacecraft arrival in the class example? The lecture example had the spacecraft arriving at Mars with a velocity of 22.49 km/sec.
c. The average velocity of Mars in orbit around the Sun is 24.08 km/sec. Comment on the trade-offs between trajectories, arrival velocities and velocity changes (delta V) required to enter an orbit around Mars.
arrow_forward
R4
arrow_forward
Which evidence first supported the heliocentric model of the solar system?
A. Mapping of stars using the unaided eye
B. Taking pictures of distant galaxies with statellite-based cameras
C. Determining that planets orbit in elliptical paths with telescope
D. Observing the surface features of nearby planets and moons with telescopes
arrow_forward
st edit was 20 minutes ago
eme
Transition
Put your answer in
the box
1.
Full Moon
2.
Waning Crescent
3.
Waxing Gibbous
4.
New Moon
5.
Waxing Crescent
DOO
6.
Waning Gibbous
7.
Waxing Quarter
8.
Waning Quarter
9. At which position would you find a full moon?
a.
A.
b.
B
C C
Sun
rays
d. D
Forth
10. At which position would you find a new moon?
a. A
b. B
d. D
11. Which moon phase is being shown to the right
Sun
Earh
a. Full Moon
b. Waxing Quarter
C. Waxing Gibbous
d. Waning Crescent
37n
12. Which moon phase is being shown to the right?
a. Full Moon
b. Waxing Quarter
C Waxing Gibbous
d. Waning Crescent
Omaon
Sun
11111!
arrow_forward
Answer question based on spacecraft mission “SunL1”
arrow_forward
Which of the following statements could be considered scientific statements ? 1. There is water on the surface of Mars. 2.
The universe contains atoms we will never detect. It is wrong to cheat.
O A. C. 1 2, and 3 are all scientific
B. None of the statements is scientific
OC.A. Only 1 is scientific
() D. B. 1 and 2 are scientific
arrow_forward
1. If people on Earth were viewing a total lunar eclipse, what would you see from your home on the Moon? Draw a diagram.
2. Why were the main reasons why the idea that the Earth was at the center of the universe lasted so long?
3. Discuss in 2 paragraphs the observations made by Galileo that disproved Geocentrism. Which one do you think was the most important?
4. Write down a hypothesis and observational experiment to test one of Newton’s laws of motion. EXPLAIN YOUR REASONING!
5. One of the first exoplanets discovered orbits the star 51 Pegasi with a period of just 4.2 days. 51 Pegasi is very similar to the Sun. Use Kepler’s laws to find the distance (in astronomical units) between the planet (unofficially named Bellerophon) and its star. SHOW YOUR WORK!
6. How does halving the distance between two objects affect the gravitational force between them?
7. Suppose the Sun were somehow replaced by a star with five times as much mass. What would happen to the gravitational force between…
arrow_forward
If we send astronauts to Mars, there will be a time delay anytime we send or receive messages to them here on Earth. Given that Mars is an average of 54.6 million km away from Earth, how long is this time delay for a 2-way 'round-trip' communication - sent to Earth, then back to Mars? (this might be important in emergency situations)
answer choices
a)About 4 minutes.
b)About 30 seconds.
c)About 10 seconds.
d)About 6 minutes.
arrow_forward
After completing this Lecture Tutorial, students should be able to:
distinguish between scientific hypotheses and nonscientific ideas.
Part 1: Comprehension of Hypotheses
A scientific hypothesis needs to (1) be supported by the majority of current data and (2) be
testable. An alien on Earth is wondering why a rubber ball falls back down to the ground
after it is thrown into the air. It comes up with several ideas about the ball.
a. Gravity is pulling the ball to the ground.
b.
A mystical force that cannot be measured is pushing the ball down.
c.
Earth's magnetic field is pulling on the rubber ball.
1. Which statement is NOT a hypothesis because it is not testable? a b c
2. Which statement is NOT a hypothesis because it is not supported by current data? a b c
3. Which statement IS a scientific hypothesis? a b c
Part 2: Application to Dinosaur Extinction
Below are possible scenarios explaining the extinction of the dinosaurs.
a. Dinosaurs were killed off by a virus.
b. A large meteorite…
arrow_forward
An astronomical unit
a.is the average distance from the Earth to the Sun.
b.is about 150 million kilometres.
c.is measured using radar signals bouncing off Venus.
d.has units of distance.
e.all of the mentioned choices.
Galileo made many discoveries. Which one of these is not attributed to him?
a.that the Moon has mountains, valleys and craters
b.that the Sun has imperfections known as sunspots
c.that four small points of light orbit the planet Jupiter
d.the invention of the telescope
e.that Venus shows a complete cycle of phases
Which one of these statements describes why the planet Venus is much warmer than Earth?
a.Venus has a denser and deeper atmosphere.
b.It is closer to the Sun than Earth.
c.It experienced a 'runaway greenhouse effect' long ago.
d.It produces more carbon dioxide than is absorbed by the surface.
e.all of the mentioned statements
arrow_forward
4
arrow_forward
SEE MORE QUESTIONS
Recommended textbooks for you
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Horizons: Exploring the Universe (MindTap Course ...
Physics
ISBN:9781305960961
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Related Questions
- Which of the following statements accurately describes our current understanding of the solar system? a. There are no metals in the solar system beyond Jupiter and its orbit. b. Terrestrial worlds are so small because their large atmospheres were stripped away in time by Jupiter. c. Jupiter and Saturn are made of strictly a combination of hydrogen and helium, and both objects lack a planetary core. d. Various ices can contribute to the mass of planetary cores if we are at a great enough distance from the sun.arrow_forward20. DETAILS PREVIOUS ANSWERS SEEDSFOUNDATIONS14 21.P.007. MY NOTES PRACTICE ANOTHER If the Magellan spacecraft transmitted radio signals down through the clouds on Venus and heard an echo from a certain spot 0.000115 second before the main echo, how high is the spot above the average surface of Venus in m and km units? (Note: The speed of light is 3.00 x 10 m/s.) in m x m in km X km Enter a number. Need Help? Read It Submit Answerarrow_forwardJohannes Kepler worked as an assistant to the observatory of Brahe at the age of 27. Brahe collected astronomical observations, which were passed into Kepler, on his death. Among the significant contributions of Brahe: 1. His observations on the planetary motion of Mars were used by later astronomers, including Kepler to construct the present model of the solar system. 2. In 1572, he observed supernova as a star that appeared suddenly, became visible for 18 months before it faded from view. Nowadays, supernova is called an exploding star. 3. In 1577, he observed a comet by measuring its parallax. His claim contradicted the idea of Aristotle that comets are "gases burning in the atmosphere." By measuring the parallax for the comet, he was able to show that the comet was further away than the Moon. 4. His findings that stars do not have parallax, he concluded that either: (a). the earth was motionless at the center of the universe; or (b). the stars were so far away that their parallax…arrow_forward
- Please answer parts C and Darrow_forward19. A laser beam takes 0.024s to jravel from a rocket to the reflective surface of a planet and back to the rocket. How far is the rocket from this planet's surface? a) 2400 km b) 1200 km c) 1800 km d) 3600 km e) 4800 km Class commarrow_forwardQUESTION 1 Estimate The Temperature For A Planet In Other Solar System (Questions 1-3) Let us assume scientists just discovered a planet orbiting a star in an extra-solar system. The star has a surface temperature Ts = 10000 Kelvins and a radius Sr = 1x109 meters. Scientists also measured the distance (D) between the star and the planet as D = 2 AU - 3.0x1011 meters. The solar power per unit area from the star's surface (Ps) can be calculated from the star's surface temperature Ts (10000 Kelvins) by the Stefen-Boltzman law Ps=0(Ts)4, where o is Stefen-Boltzman constant (5.67 x 10-8 Watt/meter2/Kelvin4). What is the solar power per unit area from the star's surface (Ps)? O Ps ~ 2.87 x 108 Watt/meter2 O Ps ~ 5.67 x 108 Watt/meter2 O O Ps ~ 2.87 x 10 Watt/meter2 Watt/meter² Ps ~ 5.67 x 10⁹ QUESTION 2 The solar power (Ps) decreases from the star's surface to the distance at the planet. Assuming the solar power per unit area at the distance of the planet as Pp, we have Pp=Ps(Sr/D)2, where…arrow_forward
- Answer question based on spacecraft mission “SunL1”arrow_forwardI. MULTIPLE CHOICE For items 1-10 Directions: Read and understand the statements/questions. Write your best answer on the space provided. (ERASURES ARE NOT ALLOWED) 1. Which of the following equations is not correct: a. Density = Volume /Mass b. Density = Volume /Mass c. Density = Volume /Mass d. Pressure = density x acceleration x height 2. Air pressure at sea level is 14.5 lbs/sq, inch. Why do we not feel this pressure pushing on us? a. the amount is neglible to the feeling of gravity b. we have grown accustomed to it since we were born c. we have grown accustomed to it since we were born d. the force of gravity negates the feeling of pressure 3. Where does the static fluid pressure at any given depth depend? a. total mass b. surface area C. surface area d. all of the above 4. In the equation for Pressure - P= rho xgxh. the units for g (SI system) are: a. kg/m? b. m/sec C. kg - m/sec d. m/sec? 5. What does Pascal's Principle state? Any object, wholly or partially immersed in a fluid,…arrow_forwardQ7arrow_forward
- step 2 Quecoon 4 It is hoped that the ExoMars cover 100mper Rover will be Sol is a solar day on Mars SOL. A SOL and equal to 24 hoursko minubes. calculate the average speed of Show worlund m 5-1 and bo bwo significant the rover. your un Signes しarrow_forwardPHYSICS UPVOTE WILL BE GIVEN. NO LONG EXPLANATION NEEDED. Which quantities are required to explain the orbital velocity of satellites in different celestial bodies? a.Universal Gravitational Constant, mass, and r b.Universal Gravitational Constant, frequency, and r c.Mass and c (speed of light) d.G, co, and radiusarrow_forwardSuppose there were a planet in our Solar System orbiting at a distance of 0.5 AU from theSun, and having ten times the mass and four times the radius of Earth. For reference, theEarth has a mass of 5.97 × 1024 kg and a radius of 6,378 km a) Calculate the density of this hypothetical planet.b) Based on your answer from part a), what do you think this planet would be made of?Explain your reasoning.c) Do this planet’s properties agree with the condensation theory for the formation of ourSolar System? Why or why not?arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
- AstronomyPhysicsISBN:9781938168284Author:Andrew Fraknoi; David Morrison; Sidney C. WolffPublisher:OpenStaxHorizons: Exploring the Universe (MindTap Course ...PhysicsISBN:9781305960961Author:Michael A. Seeds, Dana BackmanPublisher:Cengage Learning
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Horizons: Exploring the Universe (MindTap Course ...
Physics
ISBN:9781305960961
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning