ECCENTRICITY PRACTICE Base your answers to questions 5 and 6 on the diagram below, which represents the current locations of two planets, Aand B, orbiting a star. Letter X indicates a position in the orbit of planet A. Numbers 1 through 4 indicate positions in the orbit of planet B. A) Mercury B) Jupiter C) Earth D) Mars
Jan 10, 2020 · Astronomy is the scientific study of all objects in space. The word comes to us from the ancient Greek term for "star law." Astrophysics, which is part of astronomy, goes a step further and applies the laws of physics to help us understand the origins of the universe and the objects in it.
The ellipse is vitally important in astronomy as celestial objects in periodic orbits around other celestial objects all trace out ellipses. An ellipse is defined as the locus of all points in the plane for which the sum of the distances r1 and r2 to two fixed points F1 and F2 (called the foci) separated by a distance 2c, is a given constant 2a.
Eccentricity is a measure of how an orbit deviates from circular. A perfectly circular orbit has an eccentricity of zero; higher numbers indicate more elliptical orbits. Neptune, Venus, and Earth are the planets in our solar system with the least eccentric orbits. Pluto and Mercury are the planets in our solar system with the most eccentric orbits.
As on Earth, Mars’ orbital elements (obliquity, eccentricity, argument of perihelion) exhibit oscillations known as Milankovitch cycles at periods varying from 50,000 to several million years. The obliquity and eccentricity oscillations are much larger in amplitude on Mars than on Earth (Fig. 8).
The orbital eccentricity (or eccentricity) is a measure of how much an elliptical orbit is ‘squashed’. It is one of the orbital elements that must be specified in order to completely define the shape and orientation of an elliptical orbit. The equation of an ellipse in polar coordinates is:
May 12, 2014 · Table of Contents: 00:12 - 00:56 - 02:38 - ESRT pg. 1: Equations Eccentricity can be calculated by: 03:53 - 05:11 - 2. Where is the Sun located in a planet's...
The eccentricity (e) of an ellipse is the ratio of the distance from the center to the foci (c) and the distance from the center to the vertices (a). e = c a As the distance between the center and the foci (c) approaches zero, the ratio of c a approaches zero and the shape approaches a circle.
The eccentricity of an elliptical orbit is a measure of the amount by which it deviates from a circle; it is found by dividing the distance between the focal points of the ellipse by the length of the major axis.
The orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptic orbit, 1 is a parabolic escape orbit, and greate
The orbital eccentricity (or eccentricity) is a measure of how much an elliptical orbit is ‘squashed’. It is one of the orbital elements that must be specified in order to completely define the shape and orientation of an elliptical orbit. The equation of an ellipse in polar coordinates is:
Jan 21, 2017 · The 100,000 year cycle in Earth’s orbital eccentricity is the dominant cycle contributing to cooling and warming. The other, shorter cycles make their contribution when they ‘sync’ up with the big one. We’ll talk about those cycles in future posts, beginning with axial obliquity. rjb
How To Pronounce Eccentricity (astronomy) How To Pronounce Eccentricity (behavior) How To Pronounce Eccentricity (behaviour) How To Pronounce Eccentricity (disambiguation) How To Pronounce Eccentricity (graph theory) How To Pronounce Eccentricity (math) How To Pronounce Eccentricity (mathematics) How To Pronounce Eccentricity (mechanics) How To ...
Jan 21, 2017 · The 100,000 year cycle in Earth’s orbital eccentricity is the dominant cycle contributing to cooling and warming. The other, shorter cycles make their contribution when they ‘sync’ up with the big one. We’ll talk about those cycles in future posts, beginning with axial obliquity. rjb
Eccentricity definition, an oddity or peculiarity, as of conduct: an interesting man, known for his eccentricities. See more.
Eccentricity is a measure of how an orbit deviates from circular. A perfectly circular orbit has an eccentricity of zero; higher numbers indicate more elliptical orbits. Neptune, Venus, and Earth are the planets in our solar system with the least eccentric orbits. Pluto and Mercury are the planets in our solar system with the most eccentric orbits.
eccentricity (symbol e) One of the elements of an orbit. It indicates how much an elliptical orbit departs from a circle. It is found by dividing the distance between the two foci of the ellipse by the length of the major axis. A circle has an eccentricity of 0, a parabola an eccentricity of 1.
eccentricity, in astronomy: see orbit orbit, in astronomy, path in space described by a body revolving about a second body where the motion of the orbiting bodies is dominated by their mutual gravitational attraction.
Eccentricity. Students are asked to explain the phrase "eccentricity is an acquired characteristic" in regards to the orbits of extrasolar planets. keywords: eccentricity, planet formation, planet migration. swf file: ca_extrasolarplanets_eccentricity.swf
The eccentricity may take the following values: circular orbit: e = 0 elliptic orbit: 0 < e < 1 (see ellipse) parabolic trajectory: e = 1 (see parabola) hyperbolic trajectory: e > 1 (see hyperbola)
The eccentricity (e) of an ellipse is the ratio of the distance from the center to the foci (c) and the distance from the center to the vertices (a). e = c a As the distance between the center and the foci (c) approaches zero, the ratio of c a approaches zero and the shape approaches a circle.
To calculate the eccentricity correct, compute the position of the Earth with respect to the Sun (Xrel = Xe - Xsand the velocity of the Earth with respect to the Sun (Vrel = Ve - Vs). Then compute the cross product of these two (Lrel = np.cross(Xrel, Vrel)to yield the specific angular momentum of the Sun-Earth system.
May 09, 2006 · Combined changes in eccentricity, obliquity, and precession alter the strength and location of sunlight falling on the Earth’s surface. (Graphs by Robert Simmon based on data from Berger 1992.) Evidence supporting Milankovitch’s theory of the precise timing of the ice ages first came from a series of fossil coral reefs that formed on a ...
2. Eccentricity is a measure of the degree of “flattening” of the ellipse. Mathematically, the eccentricity of an ellipse is defined as the distance from a focus to the center of the ellipse divided by the length of the semimajor axis. Calculate the eccentricity of the ellipse in Figure 6.1.
Eccentricity tells us the shape of the ellipse and its value ranges from 0 to 1. As the images on the screen show you, an ellipse with 0 eccentricity is a circle and as the eccentricity nears 1,...
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Eccentricity tells us the shape of the ellipse and its value ranges from 0 to 1. As the images on the screen show you, an ellipse with 0 eccentricity is a circle and as the eccentricity nears 1,...
The eccentricity of the earth's orbit is .01677, or about . noun In ancient astronomy, the distance of the center of the equant from the earth. noun Departure or deviation from that which is stated, regular, or usual; oddity; whimsicalness: as, the eccentricity of a man's genius or conduct.
Eccentricity is a measure of how an orbit deviates from circular. A perfectly circular orbit has an eccentricity of zero; higher numbers indicate more elliptical orbits. Neptune, Venus, and Earth are the planets in our solar system with the least eccentric orbits. Pluto and Mercury are the planets in our solar system with the most eccentric orbits.
The study, “Planet–planet scattering as the source of the highest eccentricity exoplanets,” was published in Astronomy & Astrophysics. The work was supported by the Nexus for Exoplanet System Science (NExSS), the NASA Astrobiology Postdoctoral Program (NPP), and the NASA Astrobiology Institute (NAI).
The eccentricity (e) of an ellipse is the ratio of the distance from the center to the foci (c) and the distance from the center to the vertices (a). e = c a As the distance between the center and the foci (c) approaches zero, the ratio of c a approaches zero and the shape approaches a circle.
The orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptic orbit, 1 is a parabolic escape orbit, and greate
The eccentricity of an orbit is a single number, between 0 and 1, which describes how stretched out the orbit is. Zero means the orbit is perfectly circular. An eccentricity close to 1 means the orbit is extremely elongated; only comets coming from the outer reaches of the solar system get close to this value. Another word for eccentricity. Find more ways to say eccentricity, along with related words, antonyms and example phrases at Thesaurus.com, the world's most trusted free thesaurus. May 12, 2014 · Table of Contents: 00:12 - 00:56 - 02:38 - ESRT pg. 1: Equations Eccentricity can be calculated by: 03:53 - 05:11 - 2. Where is the Sun located in a planet's... The ellipse is vitally important in astronomy as celestial objects in periodic orbits around other celestial objects all trace out ellipses. An ellipse is defined as the locus of all points in the plane for which the sum of the distances r1 and r2 to two fixed points F1 and F2 (called the foci) separated by a distance 2c, is a given constant 2a. The eccentricity may take the following values: circular orbit: e = 0 elliptic orbit: 0 < e < 1 (see ellipse) parabolic trajectory: e = 1 (see parabola) hyperbolic trajectory: e > 1 (see hyperbola)
Play this game to review Astronomy. A perfect circle has an eccentricity of _____.
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Jun 09, 2020 · Using these measurement techniques the authors find that GW170817 has an eccentricity of 0.012 +0.013-0.012 and GW190425 has an eccentricity of 0.025 +0.022-0.025. These values are consistent with a low eccentricity or circular orbit, but the authors note that this is not surprising, since these events were first detected using a search that ...
To calculate the eccentricity correct, compute the position of the Earth with respect to the Sun (Xrel = Xe - Xsand the velocity of the Earth with respect to the Sun (Vrel = Ve - Vs). Then compute the cross product of these two (Lrel = np.cross(Xrel, Vrel)to yield the specific angular momentum of the Sun-Earth system.
The eccentricity of an orbit is a single number, between 0 and 1, which describes how stretched out the orbit is. Zero means the orbit is perfectly circular. An eccentricity close to 1 means the orbit is extremely elongated; only comets coming from the outer reaches of the solar system get close to this value.
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Eccentricity measures the deviation of the Earth's orbit from a circular orbit. It ranges from 0 for a circular orbit at 1 in a highly elliptical orbit. But the eccentricity of Earth's orbit varies between 0 and 0.06 for every 100 000 years. Image: The eccentricity, obliquity and precession are used within the astronomical theory of paleoclimate. eccentricity, in astronomy: see orbit orbit, in astronomy, path in space described by a body revolving about a second body where the motion of the orbiting bodies is dominated by their mutual gravitational attraction.
Eccentricity definition, an oddity or peculiarity, as of conduct: an interesting man, known for his eccentricities. See more.
orbit of Mercury In Mercury: Orbital and rotational effects …it is also the most eccentric, or elongated planetary orbit. As a... In Mercury: Orbital and rotational effects …it is also the most eccentric, or elongated planetary orbit. As a result of... Neptune In Neptune: Basic astronomical data Its ...
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2. Eccentricity is a measure of the degree of “flattening” of the ellipse. Mathematically, the eccentricity of an ellipse is defined as the distance from a focus to the center of the ellipse divided by the length of the semimajor axis. Calculate the eccentricity of the ellipse in Figure 6.1.
The orbital eccentricity (or eccentricity) is a measure of how much an elliptical orbit is 'squashed'. It is one of the orbital elements that must be specified in order to completely define the shape and orientation of an elliptical orbit. The equation of an ellipse in polar coordinates is:... [>>>]

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The eccentricity of the earth's orbit is .01677, or about . noun In ancient astronomy, the distance of the center of the equant from the earth. noun Departure or deviation from that which is stated, regular, or usual; oddity; whimsicalness: as, the eccentricity of a man's genius or conduct.
May 12, 2014 · Table of Contents: 00:12 - 00:56 - 02:38 - ESRT pg. 1: Equations Eccentricity can be calculated by: 03:53 - 05:11 - 2. Where is the Sun located in a planet's...
The eccentricity of an orbit is a single number, between 0 and 1, which describes how stretched out the orbit is. Zero means the orbit is perfectly circular. An eccentricity close to 1 means the orbit is extremely elongated; only comets coming from the outer reaches of the solar system get close to this value.
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The eccentricity is actually how elliptical, or circle-like, a planet's orbit is. We can calculate it using an equation. The equation itself is listed below (refer to Laboratory Introduction resource), but it is actually a ratio between the distance between the two foci and the length of the major axis ( HSA-CED.A.2; HSA-CED.A.4 ).
History and Etymology for eccentricity. borrowed from Medieval Latin excentricitāt-, excentricitās, from ecentricus, excentricus "not having the earth exactly at its center, eccentric entry 1 " + Latin -itāt-, -itās -ity. Keep scrolling for more. Keep scrolling for more.
2. Eccentricity is a measure of the degree of “flattening” of the ellipse. Mathematically, the eccentricity of an ellipse is defined as the distance from a focus to the center of the ellipse divided by the length of the semimajor axis. Calculate the eccentricity of the ellipse in Figure 6.1.
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Earth's orbital eccentricity is less than 0.02. The orbit of Pluto is the most eccentric of any planet in our Solar System. Pluto's orbital eccentricity is almost 0.25. Many comets have extremely eccentric orbits. Halley's Comet, for instance, has an orbital eccentricity of almost 0.97! The Sun is not at the center of an elliptical orbit.
The eccentricity of an elliptical orbit is a measure of the amount by which it deviates from a circle; it is found by dividing the distance between the focal points of the ellipse by the length of the major axis.
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The eccentricity of the earth's orbit is .01677, or about . noun In ancient astronomy, the distance of the center of the equant from the earth. noun Departure or deviation from that which is stated, regular, or usual; oddity; whimsicalness: as, the eccentricity of a man's genius or conduct. The orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptic orbit, 1 is a parabolic escape orbit, and greate
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orbit of Mercury In Mercury: Orbital and rotational effects …it is also the most eccentric, or elongated planetary orbit. As a... In Mercury: Orbital and rotational effects …it is also the most eccentric, or elongated planetary orbit. As a result of... Neptune In Neptune: Basic astronomical data Its ... The eccentricity of an orbit is a single number, between 0 and 1, which describes how stretched out the orbit is. Zero means the orbit is perfectly circular. An eccentricity close to 1 means the orbit is extremely elongated; only comets coming from the outer reaches of the solar system get close to this value. Jan 21, 2017 · The 100,000 year cycle in Earth’s orbital eccentricity is the dominant cycle contributing to cooling and warming. The other, shorter cycles make their contribution when they ‘sync’ up with the big one. We’ll talk about those cycles in future posts, beginning with axial obliquity. rjb Mar 15, 2017 · But due to its high eccentricity of 0.0934, it ranges from a distance of 206,700,000 km (128,437,425 mi) at perihelion to 249,200,000 km (154,845,700 mi) at aphelion – or between 1.38 to 1.666 AUs. See full list on mathopenref.com The orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptic orbit, 1 is a parabolic escape orbit, and greate As on Earth, Mars’ orbital elements (obliquity, eccentricity, argument of perihelion) exhibit oscillations known as Milankovitch cycles at periods varying from 50,000 to several million years. The obliquity and eccentricity oscillations are much larger in amplitude on Mars than on Earth (Fig. 8). Eccentricity. Students are asked to explain the phrase &quot;eccentricity is an acquired characteristic&quot; in regards to the orbits of extrasolar planets. keywords: eccentricity, planet formation, planet migration. swf file: ca_extrasolarplanets_eccentricity.swf The eccentricity of an orbit is a single number, between 0 and 1, which describes how stretched out the orbit is. Zero means the orbit is perfectly circular. An eccentricity close to 1 means the orbit is extremely elongated; only comets coming from the outer reaches of the solar system get close to this value.
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orbit of Mercury In Mercury: Orbital and rotational effects …it is also the most eccentric, or elongated planetary orbit. As a... In Mercury: Orbital and rotational effects …it is also the most eccentric, or elongated planetary orbit. As a result of... Neptune In Neptune: Basic astronomical data Its ... Jan 10, 2020 · Astronomy is the scientific study of all objects in space. The word comes to us from the ancient Greek term for "star law." Astrophysics, which is part of astronomy, goes a step further and applies the laws of physics to help us understand the origins of the universe and the objects in it. Earth's orbital eccentricity is less than 0.02. The orbit of Pluto is the most eccentric of any planet in our Solar System. Pluto's orbital eccentricity is almost 0.25. Many comets have extremely eccentric orbits. Halley's Comet, for instance, has an orbital eccentricity of almost 0.97! The Sun is not at the center of an elliptical orbit.
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(Astronomy) a measure of the noncircularity of an elliptical orbit, the distance between the foci divided by the length of the major axis 4. (Mathematics) geometry a number that expresses the shape of a conic section: the ratio of the distance of a point on the curve from a fixed point (the focus) to the distance of the point from a fixed line (the directrix) Thanks for contributing an answer to Astronomy Stack Exchange! Please be sure to answer the question. Provide details and share your research! But avoid … Asking for help, clarification, or responding to other answers. Making statements based on opinion; back them up with references or personal experience. Use MathJax to format equations.
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Earth's orbital eccentricity is less than 0.02. The orbit of Pluto is the most eccentric of any planet in our Solar System. Pluto's orbital eccentricity is almost 0.25. Many comets have extremely eccentric orbits. Halley's Comet, for instance, has an orbital eccentricity of almost 0.97! The Sun is not at the center of an elliptical orbit. Jun 09, 2020 · Using these measurement techniques the authors find that GW170817 has an eccentricity of 0.012 +0.013-0.012 and GW190425 has an eccentricity of 0.025 +0.022-0.025. These values are consistent with a low eccentricity or circular orbit, but the authors note that this is not surprising, since these events were first detected using a search that ... Mar 15, 2017 · But due to its high eccentricity of 0.0934, it ranges from a distance of 206,700,000 km (128,437,425 mi) at perihelion to 249,200,000 km (154,845,700 mi) at aphelion – or between 1.38 to 1.666 AUs.
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History and Etymology for eccentricity. borrowed from Medieval Latin excentricitāt-, excentricitās, from ecentricus, excentricus "not having the earth exactly at its center, eccentric entry 1 " + Latin -itāt-, -itās -ity. Keep scrolling for more. Keep scrolling for more. May 09, 2006 · Combined changes in eccentricity, obliquity, and precession alter the strength and location of sunlight falling on the Earth’s surface. (Graphs by Robert Simmon based on data from Berger 1992.) Evidence supporting Milankovitch’s theory of the precise timing of the ice ages first came from a series of fossil coral reefs that formed on a ... 2. Eccentricity is a measure of the degree of “flattening” of the ellipse. Mathematically, the eccentricity of an ellipse is defined as the distance from a focus to the center of the ellipse divided by the length of the semimajor axis. Calculate the eccentricity of the ellipse in Figure 6.1. The orbital eccentricity (or eccentricity) is a measure of how much an elliptical orbit is ‘squashed’. It is one of the orbital elements that must be specified in order to completely define the shape and orientation of an elliptical orbit. The equation of an ellipse in polar coordinates is:
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The eccentricity of an orbit is a single number, between 0 and 1, which describes how stretched out the orbit is. Zero means the orbit is perfectly circular. An eccentricity close to 1 means the orbit is extremely elongated; only comets coming from the outer reaches of the solar system get close to this value. Eccentricity is a measure of how an orbit deviates from circular. A perfectly circular orbit has an eccentricity of zero; higher numbers indicate more elliptical orbits. Neptune, Venus, and Earth are the planets in our solar system with the least eccentric orbits. Pluto and Mercury are the planets in our solar system with the most eccentric orbits.
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To calculate the eccentricity correct, compute the position of the Earth with respect to the Sun (Xrel = Xe - Xsand the velocity of the Earth with respect to the Sun (Vrel = Ve - Vs). Then compute the cross product of these two (Lrel = np.cross(Xrel, Vrel)to yield the specific angular momentum of the Sun-Earth system. Eccentricity. Students are asked to explain the phrase &quot;eccentricity is an acquired characteristic&quot; in regards to the orbits of extrasolar planets. keywords: eccentricity, planet formation, planet migration. swf file: ca_extrasolarplanets_eccentricity.swf The eccentricity of an ellipse is a measure of how nearly circular the ellipse. Eccentricity is found by the following formula eccentricity = c/a where c is the distance from the center to the focus of the ellipse a is the distance from the center to a vertex Formula for the Eccentricity of an Ellipse The special case of a circle's eccentricity The orbital eccentricity (or eccentricity) is a measure of how much an elliptical orbit is 'squashed'. It is one of the orbital elements that must be specified in order to completely define the shape and orientation of an elliptical orbit. The equation of an ellipse in polar coordinates is:... [>>>] How To Pronounce Eccentricity (astronomy) How To Pronounce Eccentricity (behavior) How To Pronounce Eccentricity (behaviour) How To Pronounce Eccentricity (disambiguation) How To Pronounce Eccentricity (graph theory) How To Pronounce Eccentricity (math) How To Pronounce Eccentricity (mathematics) How To Pronounce Eccentricity (mechanics) How To ... The orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle. A value of 0 is a circular orbit, values between 0 and 1 form an elliptic orbit, 1 is a parabolic escape orbit, and greate
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Another word for eccentricity. Find more ways to say eccentricity, along with related words, antonyms and example phrases at Thesaurus.com, the world's most trusted free thesaurus. May 09, 2006 · Combined changes in eccentricity, obliquity, and precession alter the strength and location of sunlight falling on the Earth’s surface. (Graphs by Robert Simmon based on data from Berger 1992.) Evidence supporting Milankovitch’s theory of the precise timing of the ice ages first came from a series of fossil coral reefs that formed on a ... See full list on mathopenref.com
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Eccentricity: Eric Weisstein's World of Physics [home, info] eccentricity: Imagine the Universe! Dictionary [home, info] eccentricity: Mars Glossary [home, info] Eccentricity: Extragalactic Astronomy [home, info] eccentricity: Nine Planets Glossary [home, info] eccentricity: PlanetMath Encyclopedia [home, info] Tech (6 matching dictionaries) Astronomy 101 Problem Set #10 Solutions ... just recall that a circle is a special case of an ellipse with eccentricity zero --- that is, the major and minor axes are ...
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Eccentricity definition, an oddity or peculiarity, as of conduct: an interesting man, known for his eccentricities. See more. According to latest research results, Antikythera mechanism was likely also used as a geocentric planetarium, giving a cosmic view of that era. Considering that Mercury’s eccentricity is 3.7 bigger than moon’s, this article is discussing how Hipparchus could influenced the constructor to simulate the geocentric Mercury’s orbit. The eccentricity of an elliptical orbit is a measure of the amount by which it deviates from a circle; it is found by dividing the distance between the focal points of the ellipse by the length of the major axis.
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To calculate the eccentricity correct, compute the position of the Earth with respect to the Sun (Xrel = Xe - Xsand the velocity of the Earth with respect to the Sun (Vrel = Ve - Vs). Then compute the cross product of these two (Lrel = np.cross(Xrel, Vrel)to yield the specific angular momentum of the Sun-Earth system.
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