All Free Analytical and Logical Reasoning MCQs with Answers

Every Analytical and Logical Reasoning question in the bank, across all chapters, each with the correct answer and a written explanation. Free and unlimited, with no account needed.

2,989 questions · page 110 of 150

  • A. The force accelerating the cart becomes large enough so that the force of friction holding the block in place is overcome
  • B. The force of friction holding the block in place becomes large enough to overcome the force accelerating the cart
  • C. The mass of the cart becomes too large, and the load must be reduced for the cart to accelerate
  • D. The acceleration becomes nonuniform with this force

Explanation: When the force applied reaches 4.0 newtons, the added mass of the block increases the total mass of the cart.

Correct answer: The mass of the cart becomes too large, and the load must be reduced for the cart to accelerate
  • A. It was constant
  • B. It decreased by 10.0 m/s2 each interval
  • C. It decreased by 5.0 m/s2 each interval
  • D. It increased by 5.0 m/s2 each interval

Explanation: The correct answer is Option B: It decreased by 10.0 m/s2 each interval.

Correct answer: It decreased by 10.0 m/s2 each interval
  • A. Initially lower and decreasing
  • B. Initially lower and constant
  • C. The same
  • D. Initially higher but decreasing

Explanation: The correct answer is Option A: Initially lower and decreasing. When redoing Trial 3 with a force of 1.0 newton, the average acceleration…

Correct answer: Initially lower and decreasing

2188. Astronomers believe that stars develop from the condensation of interstellar gas clouds (IGCs) that are initially hundreds to even thousands of times more massive than the Sun. Two astronomers discuss the star formation process in these clouds.Astronomer X:Star formation begins when large fragments of a gas cloud collapse. Each of these fragments typically contains hundreds of times more gas than exists in an individual star. This collapse occurs when the gravitational attraction between the gas particles overcomes the sum of all outward forces. When collapsing gas particles in each fragment get close together, heat builds up. As a protostar begins with the inward movement of particles from the exterior of the protostar. Its collapse stops when outward forces, especially forces that result from the heating of the gas being compressed, balance the gravitational force. This brings a small region of the original cloud into equilibrium and a new star into a stable form.Astronomer Y:Stars develop when small fragments of gas clouds collapse. Calculations show that when fragmentation occurs, the fragments that form are much smaller in size than mature stars. Thus, stars develop from relatively small masses and volumes of the large IGCs called cores. A cold core collapses because of its own gravity. However, 95% of all localized cores are called protostars. The collapse of a cold core is stopped by outward forces that develop when the gas heats up. The protostar then gravitationally attracts for outer layers of the cold core together until the gas has completely transformed into a star. At early stages in development, the outer layers of the cold core are so thick that they prevent the core's light from escaping into space. Only after the outer layers have been incorporated into the star does the star become visible.In order to best test Astronomer Y's theory, how should a computer simulation look with respect to the density and temperature of a gas?

  • A. Similar to an IGC's cold core, to observe its collapse
  • B. Similar to a theoretical cold core, to observe its gravitational collapse
  • C. Higher than a typical IGC's temperature, to observe its expansion
  • D. Similar to a young star's core, to observe its fusion process

Explanation: The correct answer is Option B: Similar to a theoretical cold core, to observe its gravitational collapse.

Correct answer: Similar to a theoretical cold core, to observe its gravitational collapse

2189. Astronomers believe that stars develop from the condensation of interstellar gas clouds (IGCs) that are initially hundreds to even thousands of times more massive than the Sun. Two astronomers discuss the star formation process in these clouds.Astronomer X:Star formation begins when large fragments of a gas cloud collapse. Each of these fragments typically contains hundreds of times more gas than exists in an individual star. This collapse occurs when the gravitational attraction between the gas particles overcomes the sum of all outward forces. When collapsing gas particles in each fragment get close together, heat builds up. As a protostar begins with the inward movement of particles from the exterior of the protostar. Its collapse stops when outward forces, especially forces that result from the heating of the gas being compressed, balance the gravitational force. This brings a small region of the original cloud into equilibrium and a new star into a stable form.Astronomer Y:Stars develop when small fragments of gas clouds collapse. Calculations show that when fragmentation occurs, the fragments that form are much smaller in size than mature stars. Thus, stars develop from relatively small masses and volumes of the large IGCs called cores. A cold core collapses because of its own gravity. However, 95% of all localized cores are called protostars. The collapse of a cold core is stopped by outward forces that develop when the gas heats up. The protostar then gravitationally attracts for outer layers of the cold core together until the gas has completely transformed into a star. At early stages in development, the outer layers of the cold core are so thick that they prevent the core's light from escaping into space. Only after the outer layers have been incorporated into the star does the star become visible.Which of the following physical actions or properties most directly causes heating of a protostar?

  • A. Gravitational forces from other IGCs
  • B. Pressure from the surrounding gas
  • C. distant stars
  • D. Gas atoms that strike each other as the protostar collapses

Explanation: The correct answer is the option stating 'Gas atoms that strike each other as the protostar collapses.' In the process of star formation…

Correct answer: Gas atoms that strike each other as the protostar collapses

2190. Astronomers believe that stars develop from the condensation of interstellar gas clouds (IGCs) that are initially hundreds to even thousands of times more massive than the Sun. Two astronomers discuss the star formation process in these clouds.Astronomer X:Star formation begins when large fragments of a gas cloud collapse. Each of these fragments typically contains hundreds of times more gas than exists in an individual star. This collapse occurs when the gravitational attraction between the gas particles overcomes the sum of all outward forces. When collapsing gas particles in each fragment get close together, heat builds up. As a protostar begins with the inward movement of particles from the exterior of the protostar. Its collapse stops when outward forces, especially forces that result from the heating of the gas being compressed, balance the gravitational force. This brings a small region of the original cloud into equilibrium and a new star into a stable form.Astronomer Y:Stars develop when small fragments of gas clouds collapse. Calculations show that when fragmentation occurs, the fragments that form are much smaller in size than mature stars. Thus, stars develop from relatively small masses and volumes of the large IGCs called cores. A cold core collapses because of its own gravity. However, 95% of all localized cores are called protostars. The collapse of a cold core is stopped by outward forces that develop when the gas heats up. The protostar then gravitationally attracts for outer layers of the cold core together until the gas has completely transformed into a star. At early stages in development, the outer layers of the cold core are so thick that they prevent the core's light from escaping into space. Only after the outer layers have been incorporated into the star does the star become visible.Which of the following hypotheses would Astronomer Y most likely make if a new star suddenly appeared in IGC?

  • A. A cold core has incorporated its outer layers
  • B. A collapsing fragment of gas has become dense enough to begin shining
  • C. Reflected light from our sun is seen bouncing off the IGC
  • D. The force of gravity has joined several fragments of a collapsing cloud

Explanation: Astronomer Y's hypothesis would most likely be that a new star suddenly appeared in an IGC because a collapsing fragment of gas has become…

Correct answer: A collapsing fragment of gas has become dense enough to begin shining

2191. Astronomers believe that stars develop from the condensation of interstellar gas clouds (IGCs) that are initially hundreds to even thousands of times more massive than the Sun. Two astronomers discuss the star formation process in these clouds.Astronomer X:Star formation begins when large fragments of a gas cloud collapse. Each of these fragments typically contains hundreds of times more gas than exists in an individual star. This collapse occurs when the gravitational attraction between the gas particles overcomes the sum of all outward forces. When collapsing gas particles in each fragment get close together, heat builds up. As a protostar begins with the inward movement of particles from the exterior of the protostar. Its collapse stops when outward forces, especially forces that result from the heating of the gas being compressed, balance the gravitational force. This brings a small region of the original cloud into equilibrium and a new star into a stable form.Astronomer Y:Stars develop when small fragments of gas clouds collapse. Calculations show that when fragmentation occurs, the fragments that form are much smaller in size than mature stars. Thus, stars develop from relatively small masses and volumes of the large IGCs called cores. A cold core collapses because of its own gravity. However, 95% of all localized cores are called protostars. The collapse of a cold core is stopped by outward forces that develop when the gas heats up. The protostar then gravitationally attracts for outer layers of the cold core together until the gas has completely transformed into a star. At early stages in development, the outer layers of the cold core are so thick that they prevent the core's light from escaping into space. Only after the outer layers have been incorporated into the star does the star become visible.If Astronomer X is correct ,which of the following is most likely to initially occur when 2 ICGs in which no stars are forming collide?

  • A. Cold cores forming near the boundary of the collision
  • B. Cold cores forming far from the boundary of the collision
  • C. Individual stars collapsing near the boundary of the collision
  • D. Large volumes of gas collapsing together near the boundary of the collision

Explanation: In the scenario of 2 interstellar gas clouds colliding without any stars forming, the most likely initial occurrence would be the…

Correct answer: Cold cores forming near the boundary of the collision

2192. Astronomers believe that stars develop from the condensation of interstellar gas clouds (IGCs) that are initially hundreds to even thousands of times more massive than the Sun. Two astronomers discuss the star formation process in these clouds.Astronomer X:Star formation begins when large fragments of a gas cloud collapse. Each of these fragments typically contains hundreds of times more gas than exists in an individual star. This collapse occurs when the gravitational attraction between the gas particles overcomes the sum of all outward forces. When collapsing gas particles in each fragment get close together, heat builds up. As a protostar begins with the inward movement of particles from the exterior of the protostar. Its collapse stops when outward forces, especially forces that result from the heating of the gas being compressed, balance the gravitational force. This brings a small region of the original cloud into equilibrium and a new star into a stable form.Astronomer Y:Stars develop when small fragments of gas clouds collapse. Calculations show that when fragmentation occurs, the fragments that form are much smaller in size than mature stars. Thus, stars develop from relatively small masses and volumes of the large IGCs called cores. A cold core collapses because of its own gravity. However, 95% of all localized cores are called protostars. The collapse of a cold core is stopped by outward forces that develop when the gas heats up. The protostar then gravitationally attracts for outer layers of the cold core together until the gas has completely transformed into a star. At early stages in development, the outer layers of the cold core are so thick that they prevent the core's light from escaping into space. Only after the outer layers have been incorporated into the star does the star become visible.Is the observation by Astronomer X that almost all young stars are found in clusters consistent with the theory of Astronomer Y?

  • A. Yes: the sub-fragments of fragments of the cloud that form stars attract each other gravitationally
  • B. Yes: the gas cloud where individual stars form is a relatively compact object
  • C. No: the stars. Once formed drift away from each other
  • D. No: cold cores pull in all material close to them

Explanation: The correct answer is Option D: No, cold cores pull in all material close to them.

Correct answer: No: cold cores pull in all material close to them

2193. PASSAGE:Astronomers believe that stars develop from the condensation of interstellar gas clouds (IGCs) that are initially hundreds to even thousands of times more massive than the Sun. Two astronomers discuss the star formation process in these clouds.Astronomer X:Star formation begins when large fragments of a gas cloud collapse. Each of these fragments typically contains hundreds of times more gas than exists in an individual star. This collapse occurs when the gravitational attraction between the gas particles overcomes the sum of all outward forces. When collapsing gas particles in each fragment get close together, heat builds up. As a protostar begins with the inward movement of particles from the exterior of the protostar. Its collapse stops when outward forces, especially forces that result from the heating of the gas being compressed, balance the gravitational force. This brings a small region of the original cloud into equilibrium and a new star into a stable form.Astronomer Y:Stars develop when small fragments of gas clouds collapse. Calculations show that when fragmentation occurs, the fragments that form are much smaller in size than mature stars. Thus, stars develop from relatively small masses and volumes of the large IGCs called cores. A cold core collapses because of its own gravity. However, 95% of all localized cores are called protostars. The collapse of a cold core is stopped by outward forces that develop when the gas heats up. The protostar then gravitationally attracts for outer layers of the cold core together until the gas has completely transformed into a star. At early stages in development, the outer layers of the cold core are so thick that they prevent the core's light from escaping into space. Only after the outer layers have been incorporated into the star does the star become visible.If Astronomer X is correct, the density of a newly forming star, over time, should be predicted to:

  • A. Decrease forever
  • B. Decrease until it reaches a fairly constant value
  • C. Increase until it reaches a fairly constant value
  • D. Remain constant

Explanation: Astronomer X explains that the density of a newly forming star decreases over time as outward forces from heating and compression balance…

Correct answer: Decrease forever
  • A. Mass is inversely proportional to kinetic energy
  • B. Mass is directly proportional to kinetic energy
  • C. Mass squared is proportional to kinetic energy
  • D. Mass is directly proportional to kinetic energy squared

Explanation: The correct answer is that mass is directly proportional to kinetic energy.

Correct answer: Mass is directly proportional to kinetic energy
  • A. Make a bar graph of the concentration of formaldehyde in each trial
  • B. Plot the HCHO concentration against the time required for the color change
  • C. Plot the change in tHCHO and NaHSO3 in each trial against that in HCHO concentrations
  • D. Produce a dual cataloging: the differences between the times for the color change in successive trials

Explanation: The correct answer is to make a bar graph of the concentration of formaldehyde in each trial.

Correct answer: Make a bar graph of the concentration of formaldehyde in each trial