Ceres, the largest object in the asteroid belt, is often compared to Earth’s Moon, leading many to wonder how their sizes stack up; this comparison is crucial in understanding Ceres’ place in our solar system. At COMPARE.EDU.VN, we delve into the specifics of Ceres’ size compared to the Moon, highlighting the unique features and characteristics of each celestial body. Explore the size comparison, surface composition, and the implications for planetary science and future exploration of Ceres and the Moon.
1. Unveiling Ceres and the Moon: A Tale of Two Worlds
Ceres and the Moon, both celestial bodies in our solar system, invoke curiosity about their relative sizes and characteristics. Understanding the size disparity between Ceres and the Moon is not merely an exercise in astronomical trivia; it provides a foundational understanding of their respective roles in the solar system. Ceres, the largest object in the asteroid belt located between Mars and Jupiter, holds a unique position as a dwarf planet. The Moon, Earth’s only natural satellite, is a familiar presence in our night sky. This section explores the individual characteristics of Ceres and the Moon, setting the stage for a detailed size comparison.
1.1. Ceres: The Dwarf Planet in the Asteroid Belt
Ceres, discovered in 1801 by Giuseppe Piazzi, was initially classified as a planet but was later reclassified as an asteroid and eventually as a dwarf planet by the International Astronomical Union (IAU) in 2006. This reclassification reflects a deeper understanding of Ceres’ characteristics and its place within the solar system. Ceres has a diameter of approximately 940 kilometers (584 miles), making it the largest object in the asteroid belt. Its mass accounts for about one-third of the total mass of the asteroid belt, highlighting its significant presence.
Ceres’ surface composition is of particular interest to scientists. It is believed to consist of a rocky core surrounded by a thick mantle of ice. This composition suggests that Ceres may have formed in the outer solar system and migrated inward. NASA’s Dawn spacecraft, which orbited Ceres from 2015 to 2018, provided valuable data about its surface features, including the presence of bright spots, such as Cerealia Facula and Vinalia Faculae, located in Occator Crater. These bright spots are thought to be salt deposits left behind by the evaporation of briny water that percolated up from an underground reservoir.
The presence of water ice and possible liquid water beneath the surface makes Ceres a compelling target for future exploration. It raises questions about the potential for past or present habitability on this dwarf planet. Ceres’ relatively low density, about 2.2 grams per cubic centimeter, further supports the idea of a significant amount of water ice in its composition.
1.2. The Moon: Earth’s Constant Companion
The Moon, Earth’s only natural satellite, is a familiar and influential celestial body. With a diameter of about 3,476 kilometers (2,160 miles), the Moon is significantly larger than Ceres. Its mass is about 1.2% of Earth’s mass, making it the fifth-largest moon in the solar system. The Moon orbits Earth at an average distance of about 384,400 kilometers (238,900 miles), and its gravitational influence is responsible for Earth’s tides.
The Moon’s surface is characterized by a variety of features, including impact craters, maria (dark, basaltic plains), and highlands (bright, heavily cratered regions). These features provide insights into the Moon’s geological history and the processes that have shaped its surface over billions of years. The Moon lacks a significant atmosphere, resulting in extreme temperature variations between the sunlit and shadowed sides.
The Moon’s composition is primarily silicate rocks and metals. Samples collected during the Apollo missions have provided valuable information about the Moon’s origin and evolution. The prevailing theory suggests that the Moon formed from debris ejected into space after a giant impact between Earth and a Mars-sized object.
The Moon has been a subject of human exploration since the 1960s, with the Apollo program landing twelve astronauts on its surface between 1969 and 1972. These missions collected samples, conducted experiments, and provided invaluable insights into the Moon’s geology, composition, and history. Future missions, including those planned under the Artemis program, aim to return humans to the Moon and establish a sustained presence for scientific research and exploration.
Understanding the Moon’s characteristics is essential for comprehending its influence on Earth and its potential as a resource for future space exploration. Its proximity to Earth makes it a convenient testing ground for technologies and strategies that could be used for exploring other destinations in the solar system.
2. Size Matters: Ceres Versus the Moon
When comparing celestial bodies, size is a fundamental parameter that influences many other characteristics, such as gravity, surface area, and overall geological activity. In the case of Ceres and the Moon, the size difference is significant, leading to distinct properties and evolutionary paths. This section delves into the specifics of the size comparison between Ceres and the Moon, highlighting the key differences in diameter, mass, and surface area.
2.1. Diameter Disparity: A Visual Perspective
The most straightforward way to compare the size of Ceres and the Moon is by examining their diameters. Ceres has an average diameter of approximately 940 kilometers (584 miles), while the Moon has a diameter of about 3,476 kilometers (2,160 miles). This means that the Moon is roughly 3.7 times larger in diameter than Ceres.
To visualize this difference, imagine placing Ceres next to the Moon. Ceres would appear as a much smaller object, taking up only a fraction of the Moon’s apparent size. This difference in diameter has significant implications for their respective surface areas and volumes.
The Moon’s larger diameter allows it to have a much greater surface area than Ceres. The surface area of a sphere is proportional to the square of its diameter, so the Moon’s surface area is about 13.7 times larger than that of Ceres. This larger surface area provides more opportunities for geological activity, impact events, and the development of diverse surface features.
2.2. Mass and Density: Unveiling Internal Composition
While diameter provides a visual comparison of size, mass and density offer insights into the internal composition and structure of Ceres and the Moon. Mass is a measure of the amount of matter in an object, while density is the mass per unit volume.
Ceres has a mass of approximately 9.4 × 10^20 kilograms, which is about 1.3% of the Moon’s mass (7.3477 × 10^22 kg). This significant difference in mass reflects the Moon’s larger size and different composition. The Moon is primarily composed of silicate rocks and metals, while Ceres is believed to have a significant amount of water ice in its composition.
Density is calculated by dividing mass by volume. Ceres has a density of about 2.2 grams per cubic centimeter, while the Moon has a density of about 3.34 grams per cubic centimeter. The lower density of Ceres suggests that it has a higher proportion of lighter materials, such as water ice, compared to the Moon. The Moon’s higher density indicates a greater concentration of heavier materials, such as silicate rocks and metals.
These differences in mass and density provide valuable clues about the formation and evolution of Ceres and the Moon. They suggest that Ceres may have formed in a colder region of the solar system where water ice was more abundant, while the Moon formed from materials that were closer to the Sun and more depleted in volatile compounds.
2.3. Surface Area: Implications for Geological Processes
The surface area of a celestial body is closely related to its diameter and plays a crucial role in determining the extent of geological processes and the potential for surface features to develop. The Moon, with its larger diameter, has a significantly greater surface area than Ceres.
The Moon’s surface area is approximately 3.793 × 10^7 square kilometers, while Ceres’ surface area is about 2.77 × 10^6 square kilometers. This means that the Moon has about 13.7 times more surface area than Ceres. This larger surface area allows for a greater diversity of geological features, such as impact craters, maria, and highlands.
The Moon’s heavily cratered surface is a testament to its long history of bombardment by asteroids and comets. The absence of a significant atmosphere means that there is no erosion to wear down these craters, so they remain visible for billions of years. The maria, or dark plains, are vast expanses of basaltic lava that erupted onto the surface billions of years ago. The highlands are heavily cratered regions that represent the Moon’s original crust.
Ceres also has impact craters on its surface, but they are generally smaller and less numerous than those on the Moon. This may be due to Ceres’ weaker gravity, which makes it more difficult for impactors to create large craters. Additionally, Ceres’ icy composition may allow for some degree of surface modification over time, such as the gradual smoothing of craters.
The difference in surface area between Ceres and the Moon highlights the importance of size in determining the geological processes that shape celestial bodies. The Moon’s larger surface area allows for a greater diversity of features and a more complex geological history.
A visual comparison illustrating the size difference between Ceres and the Moon, highlighting their relative dimensions.
3. Orbital Dynamics and Locations: Ceres in the Asteroid Belt, the Moon Orbiting Earth
The location and orbital dynamics of a celestial body significantly influence its environment, interactions with other objects, and overall characteristics. Ceres resides in the asteroid belt between Mars and Jupiter, while the Moon is Earth’s natural satellite. This section explores the orbital characteristics and locations of Ceres and the Moon, highlighting the key differences and their implications.
3.1. Ceres in the Asteroid Belt: A Lonely Traveler
Ceres orbits the Sun within the asteroid belt, a region populated by millions of rocky and metallic objects ranging in size from small pebbles to large asteroids. Ceres is the largest object in the asteroid belt, accounting for about one-third of its total mass. Its orbit is relatively circular and lies at an average distance of about 2.77 astronomical units (AU) from the Sun, which is about 414 million kilometers (257 million miles).
Ceres’ orbital period, the time it takes to complete one orbit around the Sun, is about 4.6 Earth years. This means that Ceres moves much slower in its orbit than Earth or the Moon. Its orbital inclination, the angle between its orbit and the plane of Earth’s orbit, is about 10.6 degrees, which is relatively low compared to some other asteroids.
The asteroid belt is a dynamic environment, with frequent collisions between objects. These collisions can break asteroids apart, creating smaller fragments that contribute to the overall population of the belt. Ceres, being the largest object in the belt, is less likely to be significantly affected by these collisions. However, it may still experience occasional impacts from smaller asteroids and meteoroids.
Ceres’ location in the asteroid belt has important implications for its composition and evolution. The asteroid belt is thought to be a remnant of the early solar system, containing materials that never coalesced into a planet. Ceres may represent a protoplanet, an object that began to form into a planet but was disrupted by the gravitational influence of Jupiter.
3.2. The Moon Orbiting Earth: A Close Relationship
The Moon is Earth’s only natural satellite, orbiting our planet at an average distance of about 384,400 kilometers (238,900 miles). This close proximity has a significant influence on Earth, particularly through the tides. The Moon’s gravitational pull causes the oceans to bulge, creating high tides on the side of Earth facing the Moon and on the opposite side.
The Moon’s orbit around Earth is elliptical, meaning that its distance from Earth varies slightly over the course of its orbit. At its closest point, called perigee, the Moon is about 363,104 kilometers (225,623 miles) from Earth. At its farthest point, called apogee, the Moon is about 405,696 kilometers (252,088 miles) from Earth.
The Moon’s orbital period, the time it takes to complete one orbit around Earth, is about 27.3 days. However, the time it takes for the Moon to go through a complete cycle of phases, from new moon to new moon, is about 29.5 days. This difference is due to Earth’s motion around the Sun, which causes the Moon’s position relative to the Sun to change over time.
The Moon’s orbit is also tidally locked, meaning that it always shows the same face to Earth. This is because Earth’s gravity has slowed the Moon’s rotation over billions of years until its rotation period matches its orbital period. As a result, we only ever see one side of the Moon from Earth.
The Moon’s close relationship with Earth has had a profound influence on our planet’s history and evolution. The Moon’s gravity stabilizes Earth’s axis of rotation, preventing extreme variations in climate. The Moon also played a role in the early Earth’s geological activity, helping to stir up the mantle and create the conditions necessary for plate tectonics.
3.3. Gravitational Influence: A Tale of Two Gravities
Gravity is a fundamental force that shapes the characteristics and behavior of celestial bodies. The gravitational influence of Ceres and the Moon differs significantly due to their size and mass differences. This section explores the gravitational implications of Ceres and the Moon, highlighting the key differences and their effects.
Ceres, with its smaller size and mass, has a much weaker gravitational pull than the Moon. The surface gravity of Ceres is only about 0.029 g, where g is the acceleration due to gravity on Earth (9.8 m/s^2). This means that an object on the surface of Ceres would weigh only about 2.9% of what it would weigh on Earth.
The Moon, with its larger size and mass, has a significantly stronger gravitational pull. The surface gravity of the Moon is about 0.1654 g, which is about 16.54% of Earth’s gravity. This means that an object on the surface of the Moon would weigh about 16.54% of what it would weigh on Earth.
The difference in gravity between Ceres and the Moon has several important implications. First, it affects the ability of these bodies to retain an atmosphere. Ceres’ weak gravity makes it difficult for it to hold onto an atmosphere, which is why it has only a very thin exosphere. The Moon’s stronger gravity allows it to retain a very thin atmosphere, but it is still much less dense than Earth’s atmosphere.
Second, the difference in gravity affects the ability of these bodies to retain surface features. Ceres’ weak gravity makes it easier for impact craters to be eroded and smoothed out over time. The Moon’s stronger gravity helps to preserve impact craters, which is why its surface is heavily cratered.
Third, the difference in gravity affects the ease with which humans can explore these bodies. Walking on Ceres would be very different from walking on the Moon. On Ceres, you would feel very light and could jump very high. On the Moon, you would feel heavier and could not jump as high.
Ceres’s location in the asteroid belt contrasted with Earth, showcasing the different environments these celestial bodies inhabit.
4. Surface Composition and Features: Icy Ceres vs. Rocky Moon
The surface composition and features of a celestial body provide valuable clues about its formation, evolution, and potential for habitability. Ceres and the Moon have distinct surface characteristics that reflect their different origins and evolutionary histories. This section explores the surface composition and features of Ceres and the Moon, highlighting the key differences and their implications.
4.1. Ceres: An Icy World with Bright Spots
Ceres’ surface composition is believed to consist of a rocky core surrounded by a thick mantle of water ice. This composition suggests that Ceres may have formed in the outer solar system, where water ice was more abundant. NASA’s Dawn spacecraft provided valuable data about Ceres’ surface features, including the presence of bright spots, such as Cerealia Facula and Vinalia Faculae, located in Occator Crater.
These bright spots are thought to be salt deposits left behind by the evaporation of briny water that percolated up from an underground reservoir. The presence of these salt deposits suggests that Ceres may have had liquid water beneath its surface in the past, and perhaps even today.
Ceres’ surface also features impact craters, but they are generally smaller and less numerous than those on the Moon. This may be due to Ceres’ weaker gravity, which makes it more difficult for impactors to create large craters. Additionally, Ceres’ icy composition may allow for some degree of surface modification over time, such as the gradual smoothing of craters.
The overall appearance of Ceres is relatively smooth and featureless compared to the Moon. This may be due to the presence of a layer of dust and debris on its surface, which obscures smaller features.
4.2. The Moon: A Rocky World with Craters and Maria
The Moon’s surface composition is primarily silicate rocks and metals. Samples collected during the Apollo missions have provided valuable information about the Moon’s origin and evolution. The Moon’s surface is characterized by a variety of features, including impact craters, maria (dark, basaltic plains), and highlands (bright, heavily cratered regions).
The Moon’s heavily cratered surface is a testament to its long history of bombardment by asteroids and comets. The absence of a significant atmosphere means that there is no erosion to wear down these craters, so they remain visible for billions of years. The maria, or dark plains, are vast expanses of basaltic lava that erupted onto the surface billions of years ago. The highlands are heavily cratered regions that represent the Moon’s original crust.
The Moon’s surface also contains a layer of dust and debris called regolith, which is created by the constant bombardment of micrometeorites. The regolith is a fine-grained material that covers the entire surface of the Moon and can be several meters thick in some areas.
The overall appearance of the Moon is much more rugged and varied than that of Ceres. The presence of craters, maria, and highlands creates a diverse landscape that has been shaped by billions of years of geological activity.
4.3. Evidence of Water: A Key Difference
One of the most significant differences between Ceres and the Moon is the evidence of water. Ceres is believed to have a significant amount of water ice in its composition, while the Moon is generally considered to be dry.
The presence of bright spots on Ceres, which are thought to be salt deposits left behind by the evaporation of briny water, suggests that Ceres may have had liquid water beneath its surface in the past, and perhaps even today. This makes Ceres a potentially habitable world, as liquid water is essential for life as we know it.
The Moon, on the other hand, is generally considered to be dry. However, recent studies have found evidence of water ice in permanently shadowed craters near the Moon’s poles. This water ice may have been deposited by comets and asteroids that impacted the Moon’s surface.
The presence of water on both Ceres and the Moon has important implications for future space exploration. Water can be used to produce rocket fuel, oxygen, and drinking water, which could make it easier and cheaper to explore these bodies.
Occator Crater on Ceres with bright spots Cerealia Facula (left) and Vinalia Faculae (right).
5. Exploration and Future Missions: Dawn’s Legacy and Lunar Ambitions
The exploration of Ceres and the Moon has been a major focus of space agencies around the world. These missions have provided valuable data about the composition, geology, and history of these bodies. This section explores the past missions to Ceres and the Moon, as well as future missions that are planned or under consideration.
5.1. Dawn Mission to Ceres: Unveiling a Dwarf Planet
NASA’s Dawn mission was the first spacecraft to orbit Ceres, arriving in March 2015 and departing in November 2018. The Dawn mission provided valuable data about Ceres’ surface features, composition, and internal structure.
One of the most significant discoveries of the Dawn mission was the presence of bright spots on Ceres, such as Cerealia Facula and Vinalia Faculae, located in Occator Crater. These bright spots are thought to be salt deposits left behind by the evaporation of briny water that percolated up from an underground reservoir.
The Dawn mission also found evidence of water ice on Ceres’ surface, as well as organic molecules. These findings suggest that Ceres may have had liquid water beneath its surface in the past, and perhaps even today.
The Dawn mission helped to revolutionize our understanding of Ceres and its place in the solar system. It showed that Ceres is a complex and dynamic world with a potentially habitable environment.
5.2. Apollo Missions to the Moon: A Giant Leap for Mankind
The Apollo missions were a series of human spaceflights undertaken by NASA between 1961 and 1972. The Apollo program achieved its goal of landing humans on the Moon, with six successful landings between 1969 and 1972.
The Apollo missions provided valuable data about the Moon’s composition, geology, and history. Astronauts collected samples of lunar rocks and soil, which have been studied by scientists around the world. The Apollo missions also conducted experiments on the Moon’s surface, such as measuring the Moon’s magnetic field and seismic activity.
The Apollo missions helped to transform our understanding of the Moon and its place in the solar system. They showed that the Moon is a complex and dynamic world with a unique history.
5.3. Future Missions: Artemis and Beyond
Future missions to Ceres and the Moon are planned or under consideration by space agencies around the world. These missions aim to further our understanding of these bodies and their potential for future exploration and resource utilization.
NASA’s Artemis program aims to return humans to the Moon by 2025 and establish a sustained presence for scientific research and exploration. The Artemis program will build on the legacy of the Apollo missions and use new technologies to explore the Moon in greater detail than ever before.
Other missions to the Moon are planned by other countries, such as China, India, and Russia. These missions aim to study the Moon’s geology, composition, and potential for resource utilization.
Future missions to Ceres are also under consideration. These missions may focus on studying Ceres’ bright spots in more detail, searching for evidence of liquid water beneath the surface, and exploring the possibility of establishing a human presence on Ceres.
The future exploration of Ceres and the Moon promises to be an exciting and rewarding endeavor, with the potential to unlock new insights into the formation and evolution of our solar system and the potential for life beyond Earth.
6. Key Differences Between Ceres and the Moon: A Summary Table
| Feature | Ceres | Moon |
|---|---|---|
| Diameter | ~940 km (584 miles) | ~3,476 km (2,160 miles) |
| Mass | 9.4 × 10^20 kg | 7.3477 × 10^22 kg |
| Density | ~2.2 g/cm³ | ~3.34 g/cm³ |
| Surface Area | 2.77 × 10^6 km² | 3.793 × 10^7 km² |
| Location | Asteroid Belt | Orbits Earth |
| Surface | Icy, with bright spots | Rocky, with craters and maria |
| Water | Evidence of water ice and brine | Evidence of water ice in polar craters |
| Gravity | ~0.029 g | ~0.1654 g |
| Past Missions | Dawn | Apollo |
7. Why Does This Comparison Matter? Implications for Space Exploration
Understanding the differences between Ceres and the Moon is crucial for planning future space missions and understanding the potential of each body for resource utilization. Ceres, with its icy composition and potential for liquid water, could serve as a valuable source of water, oxygen, and rocket fuel for future missions to the outer solar system. The Moon, with its proximity to Earth and abundance of resources, could serve as a stepping stone for missions to Mars and beyond.
7.1. Ceres: A Potential Oasis in the Asteroid Belt
Ceres’ icy composition and potential for liquid water make it a valuable resource for future space exploration. Water can be used to produce rocket fuel, oxygen, and drinking water, which could make it easier and cheaper to explore the outer solar system.
Ceres could also serve as a base for mining operations. The asteroid belt is rich in minerals and metals, which could be used to build spacecraft and other infrastructure in space.
The exploration of Ceres could also provide valuable insights into the formation and evolution of the solar system. Ceres may represent a protoplanet, an object that began to form into a planet but was disrupted by the gravitational influence of Jupiter. Studying Ceres could help us to understand how planets form and why some planets are rocky while others are gaseous.
7.2. The Moon: A Stepping Stone to Mars
The Moon’s proximity to Earth and abundance of resources make it a valuable stepping stone for missions to Mars and beyond. The Moon could serve as a testing ground for new technologies and strategies that could be used for exploring other destinations in the solar system.
The Moon could also serve as a base for mining operations. The lunar regolith contains a variety of minerals and metals, which could be used to build spacecraft and other infrastructure in space.
The exploration of the Moon could also provide valuable insights into the history of the Earth-Moon system. The Moon is thought to have formed from debris ejected into space after a giant impact between Earth and a Mars-sized object. Studying the Moon could help us to understand the early history of Earth and the processes that have shaped our planet over billions of years.
7.3. Future of Space Exploration
The future of space exploration is bright, with many exciting missions planned to explore Ceres, the Moon, and other destinations in the solar system. These missions promise to revolutionize our understanding of the universe and our place within it.
The exploration of Ceres and the Moon is not only a scientific endeavor but also a human endeavor. It represents our innate desire to explore the unknown and to push the boundaries of what is possible. The exploration of these bodies will inspire future generations of scientists, engineers, and explorers and will help to create a brighter future for all of humanity.
The lunar surface as seen during the Apollo missions, a rocky landscape with craters.
8. COMPARE.EDU.VN: Your Guide to Understanding Celestial Comparisons
At COMPARE.EDU.VN, we strive to provide detailed and objective comparisons of various topics, including celestial bodies like Ceres and the Moon. Our goal is to help you understand the key differences and similarities between these objects, providing a comprehensive overview that supports informed decision-making.
8.1. Objective Comparisons
We ensure that all our comparisons are based on reliable data and scientific consensus. By presenting information in a clear and unbiased manner, we empower our readers to draw their own conclusions.
8.2. Comprehensive Overviews
Our articles cover a wide range of aspects, from size and composition to orbital dynamics and future exploration plans. This comprehensive approach ensures that you have a complete understanding of the subject matter.
8.3. Supporting Informed Decisions
Whether you are a student, a researcher, or simply curious about space, our comparisons are designed to provide you with the knowledge you need to make informed decisions. We break down complex topics into easy-to-understand formats, making learning accessible to everyone.
9. Frequently Asked Questions (FAQ)
Q1: How much bigger is the Moon compared to Ceres?
The Moon is approximately 3.7 times larger in diameter than Ceres.
Q2: What are the main differences in surface composition between Ceres and the Moon?
Ceres is primarily icy with evidence of salt deposits, while the Moon is rocky with craters, maria, and highlands.
Q3: Where are Ceres and the Moon located?
Ceres is located in the asteroid belt between Mars and Jupiter, while the Moon orbits Earth.
Q4: What past missions have explored Ceres and the Moon?
Ceres was explored by NASA’s Dawn mission, and the Moon was explored by the Apollo missions.
Q5: What is the significance of water on Ceres and the Moon?
Water on Ceres and the Moon could be used to produce rocket fuel, oxygen, and drinking water for future space missions.
Q6: How does the gravity of Ceres compare to the gravity of the Moon?
Ceres has a much weaker gravitational pull than the Moon, about 0.029 g compared to the Moon’s 0.1654 g.
Q7: What are some future missions planned for Ceres and the Moon?
NASA’s Artemis program aims to return humans to the Moon, and future missions to Ceres are under consideration to study its bright spots and search for liquid water.
Q8: How does COMPARE.EDU.VN provide value in understanding celestial comparisons?
COMPARE.EDU.VN offers objective, comprehensive, and easy-to-understand comparisons based on reliable data and scientific consensus.
Q9: What makes Ceres a potentially habitable world?
Ceres’ potential for liquid water makes it a potentially habitable world, as liquid water is essential for life as we know it.
Q10: Why is the Moon considered a stepping stone for missions to Mars?
The Moon’s proximity to Earth and abundance of resources make it a valuable testing ground for technologies and strategies for missions to Mars.
10. Conclusion: Embracing the Wonders of Space
The comparison between Ceres and the Moon highlights the diversity and complexity of our solar system. While Ceres is an icy dwarf planet in the asteroid belt, the Moon is a rocky satellite orbiting Earth. Understanding their differences and similarities is crucial for planning future space missions and unlocking the potential of these celestial bodies for resource utilization.
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