Lecture- Tutorials for Introductory Astronomy
3rd Edition
ISBN: 9780321820464
Author: Edward E. Prather, Tim P. Slater, Jeff P. Adams, Gina Brissenden
Publisher: Addison-Wesley
expand_more
expand_more
format_list_bulleted
Concept explainers
Textbook Question
Chapter 5, Problem 6MOP
Figure 2 shows the extrasolar planet and star from the side or as seen edge-on. At theinstant shown, which direction is the planet moving (circle one)?
Expert Solution & Answer
Learn your wayIncludes step-by-step video
schedule01:56
Students have asked these similar questions
Using the center-of-mass equations or the Center of Mass Calculator (under Binary-Star Basics, above), you will investigate a specific binary-star system. Assume that Star 1 has
m1 = 3.2
solar masses, Star 2 has
m2 = 1.6
solar masses, and the total separation of the two (R) is 80 AU. (One AU is Earth's average distance from the Sun.)
(a)
What is the distance,
d1,
(in AU) from Star 1 to the center of mass?
Exoplanet orbital period (b)
For the system pictured in the previous problem (and using data given there), suppose that the star
has a mass of 0.025 solar masses, and the planet's mass is very small in comparison. Compute the
planet's orbit period. Assume the orbit is circular with a radius given by the distance listed in the
figure. Express your answer in years.
[Hint: this is a mildly challenging problem that requires plugging into a single formula but using
multiple unit conversions. You will need to use Kepler's 3rd law in its **general** form (not the
simplified form that is only applicable to objects orbiting our Sun). You will need to look up the
value of the constant G. Convert solar masses to kg, AU to m, and everything else to base Sl units;
find the period in seconds; then convert seconds to years.]
Using the center-of-mass equations or the Center of Mass Calculator (under
Binary-Star Basics, above), you will investigate a specific binary-star system.
Assume that Star 1 has
m₁ = 3.4 solar masses, Star 2 has m₂ = 1.4 solar masses, and the total
separation of the two (R) is 52 AU. (One AU is Earth's average distance from the
Sun.)
(a)What is the distance, d₁, (in AU) from Star 1 to the center of mass?
AU
(b)What is the distance, d2, (in AU) from Star 2 to the center of mass?
AU
Chapter 5 Solutions
Lecture- Tutorials for Introductory Astronomy
Ch. 5 - Prob. 1HRPCh. 5 - Prob. 2HRPCh. 5 - Prob. 3HRPCh. 5 - Prob. 4HRPCh. 5 - Prob. 5HRPCh. 5 - Prob. 6HRPCh. 5 - Stars of the same spectral type have the same...Ch. 5 - Prob. 8HRPCh. 5 - Prob. 9HRPCh. 5 - Prob. 1STP
Ch. 5 - Prob. 2STPCh. 5 - Prob. 3STPCh. 5 - Prob. 4STPCh. 5 - Prob. 5STPCh. 5 - Prob. 6STPCh. 5 - Prob. 7STPCh. 5 - Prob. 1BIPCh. 5 - Prob. 2BIPCh. 5 - Prob. 3BIPCh. 5 - Prob. 4BIPCh. 5 - Prob. 5BIPCh. 5 - Prob. 6BIPCh. 5 - Prob. 7BIPCh. 5 - At which of the times you drew would you measure...Ch. 5 - Prob. 9BIPCh. 5 - Prob. 10BIPCh. 5 - Prob. 11BIPCh. 5 - As an extrasolar planet orbits around a star, the...Ch. 5 - Which object takes a greater amount of time to...Ch. 5 - At the instant shown in Figure 1, which direction...Ch. 5 - At the instant shown in Figure 1, which direction...Ch. 5 - In general, how does the direction the extrasolar...Ch. 5 - Figure 2 shows the extrasolar planet and star from...Ch. 5 - Prob. 7MOPCh. 5 - Prob. 8MOPCh. 5 - Prob. 9MOPCh. 5 - Prob. 10MOPCh. 5 - Prob. 11MOPCh. 5 - Prob. 12MOPCh. 5 - In which extrasolar planet system(s) (AD) is the...Ch. 5 - In which extrasolar planet system(s) (AD) would we...Ch. 5 - Which system (AD) has the extrasolar planet that...Ch. 5 - Two students are discussing their answers to...Ch. 5 - Match each graph (EH) with the extrasolar planet...Ch. 5 - Prob. 18MOPCh. 5 - Given the location marked with the dot on the...Ch. 5 - Prob. 1STEPCh. 5 - Prob. 2STEPCh. 5 - The Sun’s position in the Milky Way is shown in...Ch. 5 - Prob. 2MIPCh. 5 - We normally consider Deneb to be a bright but...Ch. 5 - Are the stars from Question 2 inside or outside...Ch. 5 - Prob. 5MIPCh. 5 - Are these Messier objects part of the Milky Way...Ch. 5 - Prob. 7MIPCh. 5 - Prob. 8MIPCh. 5 - Prob. 9MIPCh. 5 - Are the objects listed in Question 9 inside or...Ch. 5 - SagDEG is approximately 11,000 ly across. Is this...Ch. 5 - Within the Local Group, the two largest galaxies...Ch. 5 - Prob. 1GAPCh. 5 - Prob. 2GAPCh. 5 - Prob. 3GAPCh. 5 - Prob. 4GAPCh. 5 - Do the galaxies that you identified in Question 4...Ch. 5 - Prob. 6GAPCh. 5 - Prob. 7GAPCh. 5 - Prob. 8GAPCh. 5 - Prob. 9GAPCh. 5 - Prob. 10GAPCh. 5 - Prob. 11GAPCh. 5 - Prob. 12GAPCh. 5 - Prob. 13GAPCh. 5 - Where is the vast majority of mass in the solar...Ch. 5 - Two students are discussing their answers to...Ch. 5 - How do the orbital speeds of planets farther from...Ch. 5 - How does the gravitational force on a planet far...Ch. 5 - Complete the blanks in the sentences of the...Ch. 5 - Imagine you were able to add a very, very large...Ch. 5 - Prob. 7DAPCh. 5 - Prob. 8DAPCh. 5 - Prob. 9DAPCh. 5 - Astronomers were surprised when they saw the real...Ch. 5 - Prob. 11DAPCh. 5 - Prob. 12DAPCh. 5 - Based on your answers to Question 12, would you...Ch. 5 - Based on the MWG’s real rotation curve and your...Ch. 5 - Prob. 15DAPCh. 5 - Prob. 16DAPCh. 5 - Prob. 17DAPCh. 5 - Prob. 1LOPCh. 5 - Prob. 2LOPCh. 5 - Prob. 3LOPCh. 5 - Prob. 4LOPCh. 5 - Prob. 5LOPCh. 5 - Prob. 6LOPCh. 5 - Prob. 7LOPCh. 5 - Prob. 8LOPCh. 5 - Prob. 9LOPCh. 5 - Prob. 1MAPCh. 5 - Prob. 2MAPCh. 5 - Prob. 3MAPCh. 5 - Prob. 4MAPCh. 5 - Prob. 5MAPCh. 5 -
One way to try to understand and envision the...Ch. 5 -
One way to try to understand and envision the...Ch. 5 - Prob. 8MAPCh. 5 -
One way to try to understand and envision the...Ch. 5 -
One way to try to understand and envision the...Ch. 5 -
One way to try to understand and envision the...Ch. 5 -
One way to try to understand and envision the...Ch. 5 -
The balloon analogy is a helpful way to think...Ch. 5 - Prob. 1HUPCh. 5 - Consider the small section of the universe...Ch. 5 - Consider the small section of the universe...Ch. 5 - Prob. 4HUPCh. 5 - Consider the small section of the universe...Ch. 5 - Prob. 6HUPCh. 5 - The relationship you described in Questions 4 and...Ch. 5 - Prob. 8HUPCh. 5 - Prob. 9HUPCh. 5 - Prob. 10HUPCh. 5 - Prob. 11HUPCh. 5 - Complete the sentence below using the words...Ch. 5 - Prob. 13HUPCh. 5 - Prob. 14HUPCh. 5 - Prob. 16HUPCh. 5 - Prob. 17HUPCh. 5 - Prob. 18HUPCh. 5 - Prob. 19HUPCh. 5 - Prob. 20HUPCh. 5 - The two drawings below represent the same group of...Ch. 5 - Prob. 2EXPCh. 5 - Prob. 3EXPCh. 5 - The two drawings below represent the same group of...Ch. 5 - Prob. 5EXPCh. 5 - The two drawings below represent the same group of...Ch. 5 - The two drawings below represent the same group of...Ch. 5 - The two drawings below represent the same group of...Ch. 5 - The two drawings below represent the same group of...Ch. 5 - The two drawings below represent the same group of...Ch. 5 - The two drawings below represent the same group of...Ch. 5 - The two drawings below represent the same group of...Ch. 5 - Prob. 1ELDPCh. 5 - When the universe was 4 billion years old, Galaxy...Ch. 5 - Prob. 3ELDPCh. 5 - Prob. 4ELDPCh. 5 - Prob. 5ELDPCh. 5 - Prob. 6ELDPCh. 5 - Prob. 7ELDPCh. 5 - Prob. 8ELDPCh. 5 - Prob. 9ELDPCh. 5 - When the universe was 4 billion years old, Galaxy...Ch. 5 - Consider the discussion between two students...Ch. 5 - Diagrams A and B below each represent a different...Ch. 5 - Diagrams A and B below each represent a different...Ch. 5 - Diagrams A and B below each represent a different...Ch. 5 - Prob. 4THPCh. 5 - Diagrams A and B below each represent a different...Ch. 5 - Consider the three diagrams (C, D, and E) shown...Ch. 5 - Consider the three diagrams (C, D, and E) shown...Ch. 5 - Imagine you could watch the history of the...Ch. 5 - Prob. 9THPCh. 5 - Prob. 10THPCh. 5 - Look at Diagram A again. Next to Diagram A, make a...
Additional Science Textbook Solutions
Find more solutions based on key concepts
3. Could a ladder on a level floor lean against a wall in static equilibrium if there were no friction forces? ...
College Physics: A Strategic Approach (4th Edition)
Explain all answers clearly, with complete sentences and proper essay structure if needed. An asterisk (*) desi...
Cosmic Perspective Fundamentals
3. What is free-fall, and why does it make you weightless? Briefly describe why astronauts are weightless in th...
The Cosmic Perspective
* EST Using Earths E field for flight Earth has an electric charge on its surface that produces a 150N/CE field...
College Physics
The diagram shows Bob’s view of the passing of two identical spaceships. Anna’s and his own, where v=2 . The le...
Modern Physics
A block of mass M is moving at speed r0 on a frictionless surface that ends in a rigid wall, heading toward a s...
Essential University Physics: Volume 1 (3rd Edition)
Knowledge Booster
Learn more about
Need a deep-dive on the concept behind this application? Look no further. Learn more about this topic, physics and related others by exploring similar questions and additional content below.Similar questions
- The best parallaxes obtained with Hipparcos have an accuracy of 0.001 arcsec. If you want to measure the distance to a star with an accuracy of 10%, its parallax must be 10 times larger than the typical error. How far away can you obtain a distance that is accurate to 10% with Hipparcos data? The disk of our Galaxy is 100,000 light-years in diameter. What fraction of the diameter of the Galaxy’s disk is the distance for which we can measure accurate parallaxes?arrow_forward(Astronomy) White Dwarf Size I. The density of Sirius B is 2×106 g/cm3 and its mass is 1.95×1030 kg. What is the radius of the white dwarf in km? (Hint: Density = mass/volume, and the volume of a sphere is 4/3πr3) Please round your answer to two significant digits.arrow_forwardLet’s say you’re looking for extrasolar planets. You observe a star that has a spectral shift in the line that is supposed to be at at 656.28011 nm – this star shows this line at 656.28005 nm. What is the radial velocity of star (in m/s) and in what direction in relation to you? a) 27.4 m/s, towards b) 27.4 km/s, away c) -27.4 m/s, toward d) -27.4 km/s, awayarrow_forward
- In a binary star system, the average separation between the stars is 5 AU and their orbital period is 4 years. What is the sum of their masses? (Enter your answer in terms of the mass of the Sun.) 781 Msun The average distance of Star A from the center of mass is 5 times that of Star B. What are their individual masses? (Enter your answers in terms of the mass of the Sun.) Star A How are the distances of each star from the center of mass related to their masses? Meun Star B Be sure you are entering the mass of Star B here. Mearrow_forward(Okay so its really astronomy) Star A and Star B are both 5 pc away, but Star A is at your zenith and Star B is at your nadir. How much more flux does Earth receive from Star A relative to Star B? Assume there are no interstellar clouds between you and each star.arrow_forwardFor each of the following parts, find the most possible type of object by considering the descriptions, and explain your answer. Each part is independent. The possible types are red giant, galaxy, planetary system, planet, dwarf planet, red dwarf, white dwarf, brown dwarf, satellite, asteroid, comet, protostar 2 star, star cluster, galaxy cluster, supercluster, emission nebula, reflection nebula, dark nebula (a) This object moves around the Sun. The nearest distance to the Sun is 0.5 AU, and the farthest distance from the Sun is 1000 AU. (b) This object is red in colour. The density is much lower than that of a star. (c) The mass of this object is the same as that of the Sun. It does not fuse hydrogen. (d) This object moves in a circular orbit about the Sun. Its orbit is between those of Mars and Jupiter. It is round in shape. (e) This object burns hydrogen in a region surrounding its helium core.arrow_forward
- In 3–5 sentences, explain how the shape of planetary orbits affects their orbital velocity. Include the proper law of planetary motion as part of your answer. In 3–5 sentences, explain how the shape of planetary orbits affects their orbital velocity. Include the proper law of planetary motion as part of your answer.arrow_forwardThe figure below shows the radial velocity of a star plotted as a function of time over the course of 20 days. Where is the planet in its orbit around the star when the star's radial velocity is 18 km/s? How do I determine this?arrow_forward(Astronomy) Binary Pulsar. Part A: Use the orbital period 27 min for the binary pulsar (two neutron stars orbit each other) to find the orbital separation of the pair in AU and solar radii. Assume a neutron star's mass is 3 solar masses. (Hints: Use the version of Kepler's third law for binary stars.) Part B: Is this system orbiting closer or further than Mercury is to the Sun?arrow_forward
- The Sun is moving at 220 ??/? around the Galactic Center at a more-or-less constant distance of 8.5 ???. To appreciate how remarkable this is, consider the following questions: a) How massive would the Sun have to be for the Earth to have an orbital velocity of 220 km/s at 1 AU? b) How fast would the Earth move if it was in orbit around the Sun at a distance of 8.5 kpc? Of course, you may ignore the effects of all other stars in this calculation.arrow_forward(Astronomy) (Part A) White Dwarf Size II. The white dwarf, Sirius B, contains 0.98 solar mass, and its density is about 2 × 106 g/cm3. Find the radius of the white dwarf in km to three significant digits. (Hint: Density = mass⁄volume, and the volume of a sphere is 4/3πr3). (Part B) Compare your answer with the radii of the planets listed in the Table A-10. Which planet is this white dwarf is closely equal to in size?arrow_forwardBRIEFLY ILLUSTRATE THE RELATIONSHIP OF ANGULAR MEASUREMENT TO CIRCULAR ARC LENGTH.arrow_forward
arrow_back_ios
SEE MORE QUESTIONS
arrow_forward_ios
Recommended textbooks for you
- Foundations of Astronomy (MindTap Course List)PhysicsISBN:9781337399920Author:Michael A. Seeds, Dana BackmanPublisher:Cengage LearningStars and Galaxies (MindTap Course List)PhysicsISBN:9781337399944Author:Michael A. SeedsPublisher:Cengage Learning
- Stars and GalaxiesPhysicsISBN:9781305120785Author:Michael A. Seeds, Dana BackmanPublisher:Cengage LearningAstronomyPhysicsISBN:9781938168284Author:Andrew Fraknoi; David Morrison; Sidney C. WolffPublisher:OpenStax
Foundations of Astronomy (MindTap Course List)
Physics
ISBN:9781337399920
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Stars and Galaxies (MindTap Course List)
Physics
ISBN:9781337399944
Author:Michael A. Seeds
Publisher:Cengage Learning
Stars and Galaxies
Physics
ISBN:9781305120785
Author:Michael A. Seeds, Dana Backman
Publisher:Cengage Learning
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax