Foundations of Astronomy (MindTap Course List)
14th Edition
ISBN: 9781337399920
Author: Michael A. Seeds, Dana Backman
Publisher: Cengage Learning
expand_more
expand_more
format_list_bulleted
Videos
Question
Chapter 24, Problem 3LTL
To determine
The reason for only one date range per year listed for each meteor shower.
Expert Solution & Answer
Trending nowThis is a popular solution!
Students have asked these similar questions
Consider an asteroid that orbits in a relatively circular orbit with a semimajor axis a = 2 au
from the Sun. A typical asteroid has an albedo, or reflectivity, A ~ 0.3. At our closest
approach to the asteroid, we make a measurement of the flux coming from the asteroid to
be F = 3 × 10-15 w m-2. What is the radius of the asteroid in km? Include a labelled
diagram along with your calculations.
A typical comet contains some 1013 kg of water ice. How many comets would have to strike Earth in order to account for the roughly 2×1021 kg of water presently found on our planet? (Hint: simple division) If this amount of water accumulated over a period of 500 million years, how frequently must Earth have been hit by comets during that time? (Hint: Calculate, on the average, how many comets hit the Earth per year during that time.)
Annual meteor showers occur when the Earth passes through the orbital path of acomet. The intensity of these showers vary from year to year. Which of the following may bethe reason for this?
Group of answer choices
- Meteor showers are not caused by comet debris
- Sun's temperature
- en distribution of debris along comet's orbit
- Earth's rotation axis
Chapter 24 Solutions
Foundations of Astronomy (MindTap Course List)
Ch. 24 - What is the difference between a meteoroid and an...Ch. 24 - What do Widmansttten patterns indicate about the...Ch. 24 - Why is it possible to acquire Moon rocks by...Ch. 24 - Prob. 4RQCh. 24 - Prob. 5RQCh. 24 - Prob. 6RQCh. 24 - Why do astronomers refer to carbonaceous...Ch. 24 - Prob. 8RQCh. 24 - Prob. 9RQCh. 24 - Of all the meteorites shown in Figure 24-2, which...
Ch. 24 - Meteorites were once part of which type of...Ch. 24 - Most sporadic meteors were once part of which...Ch. 24 - Meteors in showers were once part of which type of...Ch. 24 - Prob. 14RQCh. 24 - Prob. 15RQCh. 24 - Why do astronomers conclude that asteroids were...Ch. 24 - A fragment from the surface of a differentiated...Ch. 24 - What evidence indicates that the asteroids are...Ch. 24 - Prob. 19RQCh. 24 - Prob. 20RQCh. 24 - What evidence indicates that some asteroids once...Ch. 24 - How is the composition of meteorites related to...Ch. 24 - Prob. 23RQCh. 24 - Prob. 24RQCh. 24 - What is the difference between a centaur and a...Ch. 24 - What is the difference between a comets dust tail...Ch. 24 - What evidence indicates that a comets nucleus is...Ch. 24 - Why do most short-period comets have prograde...Ch. 24 - What are possible fates (or end-states) for...Ch. 24 - What are the hypotheses for how the bodies in the...Ch. 24 - Prob. 31RQCh. 24 - How would studying the chemical composition of...Ch. 24 - Assuming a night lasts 12 hours, how many total...Ch. 24 - Prob. 2PCh. 24 - If a single asteroid 1 km in diameter were to...Ch. 24 - If a trillion (1012) asteroids, each 1 km in...Ch. 24 - Prob. 5PCh. 24 - The asteroid Vesta has a mass of 2.6 1020 kg and...Ch. 24 - Prob. 7PCh. 24 - What is the maximum angular diameter of the dwarf...Ch. 24 - At what average distances from the Sun would you...Ch. 24 - Prob. 10PCh. 24 - If the velocity of the solar wind is about 4.0 ...Ch. 24 - What is the average distance of Comet Halley from...Ch. 24 - If you saw Comet Halley when the comet was 0.7 AU...Ch. 24 - What is the orbital period of a comet nucleus at...Ch. 24 - The mass of an average comets nucleus is about 1.0...Ch. 24 - Prob. 16PCh. 24 - Prob. 1SOPCh. 24 - Earth orbits 1 AU from the Sun, and the Oort cloud...Ch. 24 - Look at Figure 24-2d. Identify the chondrules by...Ch. 24 - Prob. 2LTLCh. 24 - Prob. 3LTLCh. 24 - Look at the images of Comet Mrkos on the left page...Ch. 24 - Prob. 5LTLCh. 24 - Prob. 6LTLCh. 24 - Prob. 7LTL
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
- Consider the differentiated meteorites. We think the irons are from the cores, the stony-irons are from the interfaces between mantles and cores, and the stones are from the mantles of their differentiated parent bodies. If these parent bodies were like Earth, what fraction of the meteorites would you expect to consist of irons, stony-irons, and stones? Is this consistent with the observed numbers of each? (Hint: You will need to look up what percent of the volume of Earth is taken up by its core, mantle, and crust.)arrow_forwardOf all the meteorites shown in Figure 24-2, which one is the most likely meteorite to be found on the ground? Why?arrow_forwardRefer to Example 13.1. How would the calculation change if a typical comet in the Oort cloud is larger-say, 50 km in diameter?arrow_forward
- Refer to Example 13.1. How would the calculation change if a typical comet in the Oort cloud is only 1 km in diameter?arrow_forwardWhat methods do scientists use to distinguish a meteorite from terrestrial material?arrow_forwardWhy is it more useful to classify meteorites according to whether they are primitive or differentiated rather than whether they are stones, irons, or stony-irons?arrow_forward
- Tutorial You observe a comet 0.32 AU from Earth with a tail that is 1.7 degrees long. How long is the tail in AU? How long is the tail in kilometers? How many times could the U.S. fit along the length of the tail? (The width of the U.S. is 4,313 km.) Part 1 of 3 You observe a comet 0.32 AU from Earth with a tail that is 1.7 degrees long. How long is the tail in AU? We use the small angle formula to calculate the length of the tail in AU. arc seconds d Ꮎ 2.06 x 105 D Solving for the linear distance gives: dAU = DAU dAU = = AU arc seconds 2.06 x 105arrow_forwardRe-order the numbers so the events occur in the correct order, with the oldest event as number 2, and the youngest event as number 13. 2. Now at roughly 100% of present-day mass and the asteroid bombardment over, Earth begins cooling and differentiating. As the outer layer of the Earth cools and solidifies, lighter elements and compounds rise to the surface while the denser ones sink to the core 3. The now differentiated ice, gas, and dust of the solar accretion disc conglomerates together into asteroids from gravity 4. "The Big Whack" A Mars-sized protoplanet we call Theia collides with primitive Earth, adding even more energy and mass 5. The Big Bang 6. As the early atmosphere cools, water vapor is eventually cool enough to condense into liquid water, eventually covering the planet in an ocean 7. The debris from the collision of Earth and Theia produce a ring in orbit. This ring eventually coalesces into the Moon, just as Earth coalesced from the solar accretion disc 8. A nebula…arrow_forwardWhy are there no chondrules in achondritic meteorites?arrow_forward
- The iron meteorite that created Barringer Crater (Arizona) was 50 m in diameter. It caused a crater 1.2 km (1200 m) in diameter, that is, 24 times bigger than the impactor. Keeping in mind that the size of the crater depends on many factors, such as the type of rocks present in the area, estimate the approximate size of the impactor that produced Mare Serenitatis.arrow_forwardThe asteroid Hygiea has a mass of 8.67 x 1019 kg and an average radius of about 216 km (2.16 x 102 km). What is its escape velocity (in m/s)? (Hints: Use the formula for escape velocity, 2GM ; remember to convert units to m, kg, and s.) r e m/s Could you jump off the asteroid? Yes No Need Help? Read It Submit Answerarrow_forwardWhy do astronomers refer to carbonaceous chondrites as unmodified or primitive material?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 Learning
AstronomyPhysicsISBN: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
Astronomy
Physics
ISBN:9781938168284
Author:Andrew Fraknoi; David Morrison; Sidney C. Wolff
Publisher:OpenStax
Kepler's Three Laws Explained; Author: PhysicsHigh;https://www.youtube.com/watch?v=kyR6EO_RMKE;License: Standard YouTube License, CC-BY