Worksheet: The Accretion Model of Planet Formation

In this worksheet, we will practice describing the process of accretion in protoplanetary disks that leads to the formation of planets.

Q1:

Which of the following statements most correctly describes what is meant by the term protoplanet?

  • AA protoplanet is a body that orbits a star, has a roughly spherical shape, and has cleared its orbit of other large objects.
  • BA protoplanet is a solid object that is held together by its own gravity, is greater than approximately 1,000 km in diameter, and has become gravitationally differentiated.
  • CA protoplanet is a small, solid particle comprising mainly water ice, methane ice, ammonia ice, and metals such as iron and nickel.
  • DA protoplanet is a solid object found in protoplanetary disks that is held together by its own gravity and that is approximately between 1 km and 1,000 km in diameter.

Q2:

Which of the following statements most correctly describes what is meant by the term “planetesimal”?

  • AA planetesimal is a small, solid particle comprising mainly of water ice, methane ice, ammonia ice, and metals such as iron and nickel.
  • BA planetesimal is a body that orbits a star, has a roughly spherical shape, and has cleared its orbit of other large objects.
  • CA planetesimal is a solid object that is held together by its own gravity, that is greater than approximately 1,000 km in diameter, and that has become gravitationally differentiated.
  • DA planetesimal is a solid object found in protoplanetary disks that is held together by its own gravity and that is approximately between 1 km and 1,000 km in diameter.

Q3:

Order the following in terms of size from least to greatest.

  1. A planet
  2. A planetesimal
  3. A dust grain in a protoplanetary disc
  4. A protoplanet
  • AA dust grain in a protoplanetary disc, a planetesimal, a planet, a protoplanet
  • BA planet, a protoplanet, a planetesimal, a dust grain in a protoplanetary disc
  • CA dust grain in a protoplanetary disc, a protoplanet, a planetesimal, a planet
  • DA dust grain in a protoplanetary disc, a planetesimal, a protoplanet, a planet
  • EA planet, a planetesimal, a protoplanet, a dust grain in a protoplanetary disc

Q4:

Which of the following statements most correctly describes how dust grains in a protoplanetary disc come together to form planetesimals?

  • ADust grains in a protoplanetary disc are large enough for the gravitational attraction between them to be significant. This causes them to collide, and over time they will eventually form planetesimals approximately 1 km across.
  • BDust grains in a protoplanetary disc are electrically charged. Positively charged dust grains are attracted to negatively charged dust grains. This causes the dust grains to collide, and over time they eventually form planetesimals approximately 1 km across.
  • CDust grains in a protoplanetary disc are too small for the gravitational attraction between them to be significant. However, due to their random motion, they will collide, and over time they will eventually form planetesimals approximately 1 km across.
  • DWhere the density of dust grains in a protoplanetary disc is slightly greater than the average, the gravitational field in that region will be greater than the average. This causes the dust grains to quickly coalesce into planetesimals over just a few years.

Q5:

Which of the following statements most correctly describes what is meant by the term “protoplanetary disk”?

  • AA protoplanetary disk is a disk of dust and gas that orbits a newly formed star.
  • BA protoplanetary disk is a disk of hot matter, usually ionized hydrogen, that surrounds a dense stellar remnant such as a neutron star or black hole.
  • CA protoplanetary disk is a disk of dust and gas that orbits the center of a galaxy.
  • DA protoplanetary disk is a disk of dust and gas that orbits a newly formed planet.
  • EA protoplanetary disk is a band of asteroids that orbits a star.

Q6:

Which of the following statements most correctly describes what is meant by the term “dust grain” when referring to a protoplanetary disc?

  • AA dust grain in a protoplanetary disc is a solid object that is held together by its own gravity, is greater than approximately 1,000 km in diameter, and has become gravitationally differentiated.
  • BA dust grain in a protoplanetary disc is an object that orbits a star, has a roughly spherical shape, and has cleared its orbit of other large objects.
  • CA dust grain in a protoplanetary disc is a solid object that is held together by its own gravity and that is approximately between 1 km and 1,000 km in diameter.
  • DA dust grain in a protoplanetary disc is a small, solid particle comprising mainly of water ice, methane ice, ammonia ice, and metals such as iron and nickel.

Q7:

Which of the following statements most correctly describes how planetesimals come together to form protoplanets?

  • APlanets and moons that have been ejected from other solar systems after supernovae become seed planets for new solar systems. Planetesimals collide with these other planets to form larger planets in the new solar system.
  • BPlanetesimals are not large enough for the gravitational attraction between them to be significant. However, due to their random motion, they will collide, and over time they will eventually form protoplanets larger than approximately 1,000 km in diameter.
  • CThe gravitational attraction between planetesimals is very strong, which causes them to coalesce into protoplanets over just a few years.
  • DPlanetesimals are large enough for the gravitational attraction between them to be significant. This causes them to collide, and over time they will eventually form protoplanets larger than approximately 1,000 km in diameter.

Nagwa uses cookies to ensure you get the best experience on our website. Learn more about our Privacy Policy.