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Questions and Answers
What is the diameter of Makemake compared to Haumea?
What is the diameter of Makemake compared to Haumea?
What is the primary component believed to cover the surface of Makemake?
What is the primary component believed to cover the surface of Makemake?
What is the distance of Makemake from the sun at this moment in time?
What is the distance of Makemake from the sun at this moment in time?
Why did Makemake manage to evade detection for many years?
Why did Makemake manage to evade detection for many years?
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What does the presence of methane and nitrogen on Makemake suggest?
What does the presence of methane and nitrogen on Makemake suggest?
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Why has Makemake lost its nitrogen over time?
Why has Makemake lost its nitrogen over time?
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What causes nitrogen to sublimate into a gas and be lost to space?
What causes nitrogen to sublimate into a gas and be lost to space?
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What is the primary reason for the depletion of nitrogen on Makemake?
What is the primary reason for the depletion of nitrogen on Makemake?
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What led to Pluto's reclassification as a dwarf planet?
What led to Pluto's reclassification as a dwarf planet?
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What distinguishes small solar system bodies (SSSBs) from dwarf planets?
What distinguishes small solar system bodies (SSSBs) from dwarf planets?
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What distinguishes Ceres from other objects in the asteroid belt?
What distinguishes Ceres from other objects in the asteroid belt?
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What is the main reason for the complicated terminology regarding minor planets, planetoids, and asteroids?
What is the main reason for the complicated terminology regarding minor planets, planetoids, and asteroids?
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What amendment did the International Astronomical Union make to the definition of a planet in 2006?
What amendment did the International Astronomical Union make to the definition of a planet in 2006?
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What is the significance of Ceres being named after the Roman goddess of corn and harvests?
What is the significance of Ceres being named after the Roman goddess of corn and harvests?
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What is the estimated diameter of Eris, the second largest dwarf planet in the solar system?
What is the estimated diameter of Eris, the second largest dwarf planet in the solar system?
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What is the estimated diameter of Haumea, a dwarf planet with an elongated egg shape?
What is the estimated diameter of Haumea, a dwarf planet with an elongated egg shape?
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What is the name of the spacecraft that made flybys of Ceres in 2015, sending back detailed images and giving clues to its past?
What is the name of the spacecraft that made flybys of Ceres in 2015, sending back detailed images and giving clues to its past?
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What is the composition of the highly reflective mounds on the surface of Ceres?
What is the composition of the highly reflective mounds on the surface of Ceres?
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What is the name of the region on Pluto's surface that is a large double-lobed plain of smooth volatile ice sheets?
What is the name of the region on Pluto's surface that is a large double-lobed plain of smooth volatile ice sheets?
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What is the leading theory about the formation of the Pluto-Charon system?
What is the leading theory about the formation of the Pluto-Charon system?
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What is the primary reason for the debate over the definition of a planet?
What is the primary reason for the debate over the definition of a planet?
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What is the significance of Tombaugh Regio on Pluto?
What is the significance of Tombaugh Regio on Pluto?
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What is the primary composition of the Kuiper Belt?
What is the primary composition of the Kuiper Belt?
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What is the main component of Ceres' composition?
What is the main component of Ceres' composition?
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What is the primary reason for the formation of frozen nitrogen ice sheets on Pluto?
What is the primary reason for the formation of frozen nitrogen ice sheets on Pluto?
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What distinguishes Haumea from other dwarf planets?
What distinguishes Haumea from other dwarf planets?
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Pluto was reclassified as a dwarf planet by the IAU in 2006, but Eris was not.
Pluto was reclassified as a dwarf planet by the IAU in 2006, but Eris was not.
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The Kuiper Belt is a sparsely populated disk of icy objects formed early in the solar system's life.
The Kuiper Belt is a sparsely populated disk of icy objects formed early in the solar system's life.
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Ceres is believed to be an embryonic planet that did not grow larger due to Jupiter's influence.
Ceres is believed to be an embryonic planet that did not grow larger due to Jupiter's influence.
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Pluto has a thick atmosphere and six moons, with Charon forming a barycenter with Pluto.
Pluto has a thick atmosphere and six moons, with Charon forming a barycenter with Pluto.
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Makemake is a relatively structured and shapely body with a bright patch and a prominent ring system.
Makemake is a relatively structured and shapely body with a bright patch and a prominent ring system.
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Eris, the second largest dwarf planet, is rocky and icy, almost the same size as Pluto, and has a small moon named Dysnomia.
Eris, the second largest dwarf planet, is rocky and icy, almost the same size as Pluto, and has a small moon named Dysnomia.
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Pluto lost its planetary status due to not meeting the revised definition and was reclassified as a dwarf planet
Pluto lost its planetary status due to not meeting the revised definition and was reclassified as a dwarf planet
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The International Astronomical Union amended the definition of a planet in 2006, adding a criterion that a planet must clear out its orbital path
The International Astronomical Union amended the definition of a planet in 2006, adding a criterion that a planet must clear out its orbital path
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Ceres, the first discovered dwarf planet, is located within the asteroid belt between the orbits of Mars and Jupiter
Ceres, the first discovered dwarf planet, is located within the asteroid belt between the orbits of Mars and Jupiter
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Ceres was initially mistaken for a comet and then for a planet before being reclassified as a dwarf planet
Ceres was initially mistaken for a comet and then for a planet before being reclassified as a dwarf planet
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Ceres is about 1000 kilometers in diameter and accounts for about a third of the asteroid belt's total mass
Ceres is about 1000 kilometers in diameter and accounts for about a third of the asteroid belt's total mass
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Dwarf planets are nearly spherical and dominate their surrounding space
Dwarf planets are nearly spherical and dominate their surrounding space
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Haumea is larger in diameter than Makemake.
Haumea is larger in diameter than Makemake.
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Makemake's bright surface is primarily covered in frozen methane.
Makemake's bright surface is primarily covered in frozen methane.
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Makemake is located within the Kuiper Belt.
Makemake is located within the Kuiper Belt.
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Makemake's orbit lies in sync with the solar system's ecliptic plane.
Makemake's orbit lies in sync with the solar system's ecliptic plane.
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Makemake has a thick atmosphere similar to that of Pluto.
Makemake has a thick atmosphere similar to that of Pluto.
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The primary reason for nitrogen depletion on Makemake is its inability to retain its atmosphere due to its small size.
The primary reason for nitrogen depletion on Makemake is its inability to retain its atmosphere due to its small size.
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Makemake's nitrogen ice sheets are primarily formed due to the excitement by the sun's light causing nitrogen to sublimate into a gas.
Makemake's nitrogen ice sheets are primarily formed due to the excitement by the sun's light causing nitrogen to sublimate into a gas.
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The presence of methane and nitrogen on Makemake suggests the potential existence of a transient atmosphere similar to Pluto.
The presence of methane and nitrogen on Makemake suggests the potential existence of a transient atmosphere similar to Pluto.
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Is Makemake smaller than Haumea?
Is Makemake smaller than Haumea?
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Makemake is the brightest trans-neptunian object after Pluto.
Makemake is the brightest trans-neptunian object after Pluto.
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Makemake's orbit lies in sync with the solar system's ecliptic plane.
Makemake's orbit lies in sync with the solar system's ecliptic plane.
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Makemake is located near the outer edge of the Kuiper Belt, over 50 astronomical units away from the sun.
Makemake is located near the outer edge of the Kuiper Belt, over 50 astronomical units away from the sun.
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The spectral data analysis suggests that Makemake's surface is covered in frozen methane and small quantities of nitrogen ice.
The spectral data analysis suggests that Makemake's surface is covered in frozen methane and small quantities of nitrogen ice.
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Makemake can retain its atmosphere when it expands due to its small size.
Makemake can retain its atmosphere when it expands due to its small size.
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Methane thaws at much higher temperatures than nitrogen.
Methane thaws at much higher temperatures than nitrogen.
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The presence of methane and nitrogen on Makemake suggests that it may have a transient atmosphere like Pluto.
The presence of methane and nitrogen on Makemake suggests that it may have a transient atmosphere like Pluto.
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Study Notes
The Solar System's Dwarf Planets
- Our solar system consists of eight conventional planets, including four rocky terrestrial planets and four gas giants.
- Beyond the eight planets lie dozens of small icy worlds known as minor planets, including Pluto, which was reclassified as a dwarf planet in 2006.
- There are almost 800,000 known minor planets in the solar system, archived by the Minor Planet Center.
- The terminology for minor planets, planetoids, and asteroids has become more complicated due to discoveries in the outer solar system, leading to the need for clarifications.
- In 2006, the International Astronomical Union amended the definition of a planet, adding a criterion that a planet must clear out its orbital path.
- Pluto lost its planetary status due to not meeting the revised definition and was reclassified as a dwarf planet.
- The IAU then reclassified the term "minor planet" into two new sub-categories: dwarf planets and small solar system bodies (SSSBs).
- Dwarf planets are nearly spherical but don't dominate their surrounding space, while SSSBs encompass anything else that isn't a comet.
- The first dwarf planet ever discovered and visited is Ceres, located within the asteroid belt between the orbits of Mars and Jupiter.
- Ceres was initially mistaken for a comet and then for a planet before being reclassified as a dwarf planet due to its large size and mass compared to other objects in the asteroid belt.
- Ceres was discovered in 1801 by Giuseppe Piazzi and named after the Roman goddess of corn and harvests.
- Ceres is about 1000 kilometers in diameter and accounts for about a third of the asteroid belt's total mass.
The Solar System's Dwarf Planets and Kuiper Belt
- In 2015, NASA's Dawn spacecraft made flybys of the dwarf planet Ceres, sending back detailed images and clues about its composition.
- Ceres is composed of rock and water ice, with a core and mantle thought to have a layer of ice, potentially holding more water than Earth in solid form.
- It is believed that Ceres may have had an ocean of magnesium salt water on its surface billions of years ago.
- The Kuiper Belt, located beyond all eight planets, is a vast, densely populated region consisting of icy objects and debris.
- The Kuiper Belt is home to hundreds of millions of cometary nuclei, thousands of objects larger than 100 kilometers in diameter, and cold dwarf planets.
- Pluto, a Kuiper Belt object and dwarf planet, was visited by NASA's New Horizons mission in 2015, revealing its detailed landscape and complex features.
- Pluto's surface temperatures can fall as low as -240 degrees Celsius, leading to the formation of frozen nitrogen ice sheets.
- Pluto's heart-shaped region, Tombaugh Regio, is a smooth plane of volatile ice sheets with evidence of convection currents below the surface.
- The debate over the definition of a planet was prompted by the discovery of new dwarf planets, including Eris, Haumea, and Makemake, in the Kuiper Belt between 2003 and 2005.
- Eris, the second largest dwarf planet in the solar system, was initially set to be classified as the 10th planet but was later reclassified as a dwarf planet, prompting the addition of a third criterion in the definition of a planet.
- Haumea, a dwarf planet, has an elongated egg shape and is thought to be the largest constituent of a collection of trans-neptunian objects left over from a large collision of debris.
- Makemake, another dwarf planet, was discovered in 2005 and is the third dwarf planet discovered by Mike Brown.
The Solar System's Dwarf Planets
- Our solar system consists of eight conventional planets, including four rocky terrestrial planets and four gas giants.
- Beyond the eight planets lie dozens of small icy worlds known as minor planets, including Pluto, which was reclassified as a dwarf planet in 2006.
- There are almost 800,000 known minor planets in the solar system, archived by the Minor Planet Center.
- The terminology for minor planets, planetoids, and asteroids has become more complicated due to discoveries in the outer solar system, leading to the need for clarifications.
- In 2006, the International Astronomical Union amended the definition of a planet, adding a criterion that a planet must clear out its orbital path.
- Pluto lost its planetary status due to not meeting the revised definition and was reclassified as a dwarf planet.
- The IAU then reclassified the term "minor planet" into two new sub-categories: dwarf planets and small solar system bodies (SSSBs).
- Dwarf planets are nearly spherical but don't dominate their surrounding space, while SSSBs encompass anything else that isn't a comet.
- The first dwarf planet ever discovered and visited is Ceres, located within the asteroid belt between the orbits of Mars and Jupiter.
- Ceres was initially mistaken for a comet and then for a planet before being reclassified as a dwarf planet due to its large size and mass compared to other objects in the asteroid belt.
- Ceres was discovered in 1801 by Giuseppe Piazzi and named after the Roman goddess of corn and harvests.
- Ceres is about 1000 kilometers in diameter and accounts for about a third of the asteroid belt's total mass.
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Description
Test your knowledge of the solar system's dwarf planets with this quiz. Explore the reclassification of Pluto, the criteria for dwarf planet status, and the discovery of Ceres, the first dwarf planet ever visited.