21ST CENT.ASTRONOMY(LL)W/CODE WKBK PKG.
6th Edition
ISBN: 9780393874921
Author: PALEN
Publisher: Norton, W. W. & Company, Inc.
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Question
Chapter 12, Problem 13QP
To determine
The most probable origin of an iron meteorite in the solar system.
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Explain the light emission by meteorite?
Which of the following events can NOT be explained by a giant impact event?
The large metallic core of Mercury
The extreme axis tilt of Uranus
The formation of the Moon
The backwards rotation of Venus
Re-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…
Chapter 12 Solutions
21ST CENT.ASTRONOMY(LL)W/CODE WKBK PKG.
Ch. 12.1 - Prob. 12.1CYUCh. 12.2 - Prob. 12.2CYUCh. 12.3 - Prob. 12.3ACYUCh. 12.3 - Prob. 12.3BCYUCh. 12.4 - Prob. 12.4CYUCh. 12.5 - Prob. 12.5CYUCh. 12 - Prob. 1QPCh. 12 - Prob. 2QPCh. 12 - Prob. 3QPCh. 12 - Prob. 4QP
Ch. 12 - Prob. 5QPCh. 12 - Prob. 6QPCh. 12 - Prob. 7QPCh. 12 - Prob. 8QPCh. 12 - Prob. 9QPCh. 12 - Prob. 10QPCh. 12 - Prob. 11QPCh. 12 - Prob. 12QPCh. 12 - Prob. 13QPCh. 12 - Prob. 14QPCh. 12 - Prob. 15QPCh. 12 - Prob. 16QPCh. 12 - Prob. 17QPCh. 12 - Prob. 18QPCh. 12 - Prob. 19QPCh. 12 - Prob. 20QPCh. 12 - Prob. 22QPCh. 12 - Prob. 23QPCh. 12 - Prob. 24QPCh. 12 - Prob. 25QPCh. 12 - Prob. 26QPCh. 12 - Prob. 27QPCh. 12 - Prob. 28QPCh. 12 - Prob. 29QPCh. 12 - Prob. 30QPCh. 12 - Prob. 31QPCh. 12 - Prob. 32QPCh. 12 - Prob. 33QPCh. 12 - Prob. 34QPCh. 12 - Prob. 35QPCh. 12 - Prob. 36QPCh. 12 - Prob. 37QPCh. 12 - Prob. 38QPCh. 12 - Prob. 39QPCh. 12 - Prob. 40QPCh. 12 - Prob. 41QPCh. 12 - Prob. 42QPCh. 12 - Prob. 43QPCh. 12 - Prob. 44QP
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- If a single asteroid 1 km in diameter were to be fragmented into meteoroids 1 m in diameter, how many would it yield? (Hint: The volume of a sphere 43r3 )arrow_forwardWhich meteorites are the most useful for defining the age of the solar system? Why?arrow_forwardSuppose a new primitive meteorite is discovered (sometime after it falls in a field of soybeans) and analysis reveals that it contains a trace of amino acids, all of which show the same rotational symmetry (unlike the Murchison meteorite). What might you conclude from this finding?arrow_forward
- A crater on the Moon is 28 km in diameter. If a typical meteorite is 11 times smaller than the diameter of the crater, what was the diameter (in km) of the original meteorite? km What is the estimated depth (in km) of the crater if its depth is one-ninth its diameter? kmarrow_forwardThe 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_forwardWhat is special about the asteroid Vesta? a It is an S-type asteroid that never underwent any geologic activity. b It is a C-type asteroid that is one of the most primitive asteroids known. c It is an M-type asteroid that reflects radar very brightly. d It differentiated and had volcanic activity, including eruptions of lava.arrow_forward
- The Tunguska asteroid is estimated to have had a diameter of 50 m, and to have produced an explosion equivalent to 10 megatons of TNT (1 megaton = 4.2 x 1015 joules). Assume that the asteroid was a sphere with density 2 g/cm3. Using the kinetic energy formula K = ½ mv2, where m is the mass and v is the speed, to estimate the speed of the asteroid. Assume that all kinetic energy is converted into the energy of the explosion. Give your answer in km/s with one significant figure.arrow_forwardWhy is the composition of a comet typically dominated by volatile materials (frozen ices)? choose one of the following: a. rock and metal could not condense out of the solar nebula at extreme distances from the sun b. most of the metal in the solar system is locked up inside the terrestrial planets c. metals are not stable in the outer solar system d. elements that form ices (as opposed to rock & metals) are more abundant in our solar systemarrow_forwardGive at least two reasons today’s astronomers are so interested in the discovery of additional Earthapproaching asteroids.arrow_forward
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