Convert Meter Second to Cosmic Velocity First and more • 39 conversions
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The meter per second (m/s) is the derived unit of speed in the International System of Units (SI). It quantifies the rate at which an object moves. Specifically, it expresses how many meters are traveled in one second, making it a crucial measurement in various fields such as physics, engineering, and everyday life. The m/s unit is dimensionally represented as [L][T]⁻¹, where [L] denotes length and [T] denotes time, indicating that speed is a measure of distance over time. The use of m/s is standardized worldwide, facilitating clear communication of speed metrics in scientific and engineering contexts.
The meter per second is widely employed in various fields, including physics, engineering, and everyday life. It serves as a standard unit for measuring speed in scientific research, automotive engineering, and aviation. In sports, performance metrics are often expressed in meters per second to indicate speed and efficiency. The m/s unit is also essential in calculating velocities in fluid dynamics, meteorology, and even in pedestrian traffic flow studies, making it a versatile and crucial unit of measure.
The speed of sound in air at sea level is approximately 343 m/s.
The first cosmic velocity, also known as escape velocity, is defined as the minimum speed required for an object to break free from the gravitational attraction of a celestial body without any further propulsion. This velocity depends on the mass and radius of the celestial body; mathematically, it can be expressed using the formula: v = √(2GM/R), where G is the gravitational constant, M is the mass of the celestial body, and R is the radius. For Earth, this velocity is approximately 11.2 km/s. It is crucial in astrophysics and aerospace engineering as it determines the energy requirements for spacecraft and satellites to leave a planet's gravitational pull.
Today, the first cosmic velocity is a fundamental parameter in the design and launch of spacecraft. Engineers and scientists calculate the minimum speed required to send satellites into orbit or to escape a planet's gravitational field when launching missions to other celestial bodies. This velocity is crucial for mission planning, trajectory calculations, and ensuring that spacecraft can achieve their intended destinations efficiently.
The escape velocity from the International Space Station is around 28,000 km/h (17,500 mph).
= × 1.00000To convert to , multiply the value by 1.00000. This conversion factor represents the ratio between these two units.
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speed • SI Unit
The meter per second (m/s) is the derived unit of speed in the International System of Units (SI). It quantifies the rate at which an object moves. Specifically, it expresses how many meters are traveled in one second, making it a crucial measurement in various fields such as physics, engineering, and everyday life. The m/s unit is dimensionally represented as [L][T]⁻¹, where [L] denotes length and [T] denotes time, indicating that speed is a measure of distance over time. The use of m/s is standardized worldwide, facilitating clear communication of speed metrics in scientific and engineering contexts.
The meter per second as a unit of speed emerged with the establishment of the metric system in France during the late 18th century. The metric system was designed to provide a universal standard for measurement, promoting ease of trade and communication. The meter was defined originally as one ten-millionth of the distance from the equator to the North Pole, while the second was defined based on the Earth's rotation, which evolved into the atomic definition we use today. These foundational concepts were formalized in the 1790s, leading to the introduction of the meter per second as a natural unit for speed.
Etymology: The term 'meter' originates from the Greek word 'metron', meaning 'measure'. The word 'second' comes from the Latin 'secunda', meaning 'second' in a series, referring to the division of time.
The meter per second is widely employed in various fields, including physics, engineering, and everyday life. It serves as a standard unit for measuring speed in scientific research, automotive engineering, and aviation. In sports, performance metrics are often expressed in meters per second to indicate speed and efficiency. The m/s unit is also essential in calculating velocities in fluid dynamics, meteorology, and even in pedestrian traffic flow studies, making it a versatile and crucial unit of measure.
speed • Non-SI
The first cosmic velocity, also known as escape velocity, is defined as the minimum speed required for an object to break free from the gravitational attraction of a celestial body without any further propulsion. This velocity depends on the mass and radius of the celestial body; mathematically, it can be expressed using the formula: v = √(2GM/R), where G is the gravitational constant, M is the mass of the celestial body, and R is the radius. For Earth, this velocity is approximately 11.2 km/s. It is crucial in astrophysics and aerospace engineering as it determines the energy requirements for spacecraft and satellites to leave a planet's gravitational pull.
The concept of escape velocity dates back to Isaac Newton's work in the 17th century, when he first formulated the laws of motion and universal gravitation. Newton proposed that an object needs to reach a certain speed to overcome gravitational forces. The term 'escape velocity' was later coined in the 20th century, as the understanding of celestial mechanics evolved with advancements in physics and engineering.
Etymology: The term 'cosmic' originates from the Greek word 'kosmos', which means 'order' or 'world', and 'velocity' comes from the Latin 'velocitas', meaning 'swiftness'.
Today, the first cosmic velocity is a fundamental parameter in the design and launch of spacecraft. Engineers and scientists calculate the minimum speed required to send satellites into orbit or to escape a planet's gravitational field when launching missions to other celestial bodies. This velocity is crucial for mission planning, trajectory calculations, and ensuring that spacecraft can achieve their intended destinations efficiently.
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