Convert Online Unit Length Kiloparsecs to Bohr radius
Convert Kiloparsecs to Bohr radius
Kiloparsecs
kpc ResetBohr radius
b Copy
How to use this Kiloparsecs to Bohr radius Converter 🤔 Follow these steps to convert given Kiloparsecs value from Kiloparsecs units to Bohr radius units.
Enter the input Kiloparsecs value in the text field. The given Kiloparsecs is converted to Bohr radius in realtime ⌚ using the formula, and displayed under the Bohr radius label. You may copy the resulting Bohr radius value using the Copy button. Calculation Calculation will be done after you enter a valid input.
Kiloparsecs to Bohr radius Conversion TableThe following table gives some of the most used conversions from Kiloparsecs to Bohr radius.
Kiloparsecs (kpc ) Bohr radius (b ) 0 kpc 0 b 1 kpc 5.831085118984171e+29 b 2 kpc 1.1662170237968342e+30 b 3 kpc 1.7493255356952512e+30 b 4 kpc 2.3324340475936683e+30 b 5 kpc 2.9155425594920857e+30 b 6 kpc 3.4986510713905025e+30 b 7 kpc 4.081759583288919e+30 b 8 kpc 4.6648680951873366e+30 b 9 kpc 5.247976607085754e+30 b 10 kpc 5.831085118984171e+30 b 20 kpc 1.1662170237968343e+31 b 50 kpc 2.9155425594920854e+31 b 100 kpc 5.831085118984171e+31 b 1000 kpc 5.831085118984171e+32 b 10000 kpc 5.83108511898417e+33 b 100000 kpc 5.831085118984171e+34 b
Kiloparsecs A kiloparsec (kpc) is a unit of length used in astronomy to measure astronomical distances. One kiloparsec is equivalent to 3,262 light-years or approximately 3.086 × 10^16 meters.
The kiloparsec is defined as one thousand parsecs, where one parsec is the distance at which one astronomical unit subtends an angle of one arcsecond.
Kiloparsecs are used to measure large distances between celestial objects, such as the size of galaxies or the distance between galactic structures. They provide a convenient scale for expressing vast distances in the universe.
Bohr radius The Bohr radius is a fundamental unit of length used in atomic physics to describe the size of the ground state orbit of an electron around a proton in a hydrogen atom. One Bohr radius is approximately 5.29177 × 10^(-11) meters or about 0.529 angstroms.
The Bohr radius is derived from the Bohr model of the atom, which describes the electron's orbit as quantized and stable. It provides a characteristic length scale for the electron's position in its lowest energy state, known as the ground state.
The Bohr radius is used in atomic and quantum physics to understand the size of atoms, atomic orbitals, and the fundamental structure of matter. It is a key parameter in the Bohr model and provides insight into the scale of atomic interactions and energy levels.
{
"conversion": "kiloparsecs-bohr_radius",
"x_slug": "kiloparsecs",
"y_slug": "bohr_radius",
"x": "kpc",
"y": "b",
"x_desc": "Kiloparsecs",
"y_desc": "Bohr radius",
"category": "Length",
"symbol": "m",
"formula": "x * 5.831085118984171e+29",
"precision": 16,
"examples": "<div class=\"example\">\n <div class=\"example_head\"><span class=\"example_n\">1</span>\n <h3 class=\"question\">Consider that the diameter of the Milky Way galaxy is about 30 kiloparsecs.<br>Convert this diameter from kiloparsecs to Bohr radius.</h3></div>\n <h4 class=\"answer\">Answer:</h4>\n <p><strong>Given:</strong></p>\n <p>The length in kiloparsecs is:</p>\n <p class=\"step\"><span>Length<sub>(Kiloparsecs)</sub></span> = 30</p>\n <p><strong>Formula:</strong></p>\n <p>The formula to convert length from kiloparsecs to bohr radius is:</p>\n <p class=\"formula step\"><span>Length<sub>(Bohr radius)</sub></span> = <span>Length<sub>(Kiloparsecs)</sub></span> × 5.831085118984171e+29</p>\n <p><strong>Substitution:</strong></p>\n <p>Substitute given weight <strong>Length<sub>(Kiloparsecs)</sub> = 30</strong> in the above formula.</p>\n <p class=\"step\"><span>Length<sub>(Bohr radius)</sub></span> = <span>30</span> × 5.831085118984171e+29</p>\n <p class=\"step\"><span>Length<sub>(Bohr radius)</sub></span> = 1.7493255356952512e+31</p>\n <p><strong>Final Answer:</strong></p>\n <p>Therefore, <strong>30 kpc</strong> is equal to <strong>1.7493255356952512e+31 b</strong>.</p>\n <p>The length is <strong>1.7493255356952512e+31 b</strong>, in bohr radius.</p>\n </div>\n <div class=\"example\">\n <div class=\"example_head\"><span class=\"example_n\">2</span>\n <h3 class=\"question\">Consider that the Sun is located approximately 8 kiloparsecs from the center of the Milky Way.<br>Convert this distance from kiloparsecs to Bohr radius.</h3></div>\n <h4 class=\"answer\">Answer:</h4>\n <p><strong>Given:</strong></p>\n <p>The length in kiloparsecs is:</p>\n <p class=\"step\"><span>Length<sub>(Kiloparsecs)</sub></span> = 8</p>\n <p><strong>Formula:</strong></p>\n <p>The formula to convert length from kiloparsecs to bohr radius is:</p>\n <p class=\"formula step\"><span>Length<sub>(Bohr radius)</sub></span> = <span>Length<sub>(Kiloparsecs)</sub></span> × 5.831085118984171e+29</p>\n <p><strong>Substitution:</strong></p>\n <p>Substitute given weight <strong>Length<sub>(Kiloparsecs)</sub> = 8</strong> in the above formula.</p>\n <p class=\"step\"><span>Length<sub>(Bohr radius)</sub></span> = <span>8</span> × 5.831085118984171e+29</p>\n <p class=\"step\"><span>Length<sub>(Bohr radius)</sub></span> = 4.6648680951873366e+30</p>\n <p><strong>Final Answer:</strong></p>\n <p>Therefore, <strong>8 kpc</strong> is equal to <strong>4.6648680951873366e+30 b</strong>.</p>\n <p>The length is <strong>4.6648680951873366e+30 b</strong>, in bohr radius.</p>\n </div>\n ",
"img": "<img class=\"conversion\" src=\"/images/unit/length/kiloparsecs-bohr_radius.webp\" height=\"360\" width=\"640\" alt=\"Kiloparsecs to Bohr radius Converter | kpc to b\" />",
"table1n": "<h2><span class=\"x\">Kiloparsecs</span> to <span class=\"y\">Bohr radius</span> Conversion Table</h2><p>The following table gives some of the most used conversions from Kiloparsecs to Bohr radius.</p><table><thead><tr><th scope=\"column\" role=\"columnheader\">Kiloparsecs (<span class=\"unit\">kpc</span>)</th><th scope=\"column\" role=\"columnheader\">Bohr radius (<span class=\"unit\">b</span>)</th><tr></thead><tbody><tr><td>0 <span class=\"unit\">kpc</span></td><td>0 <span class=\"unit\">b</span></td></tr><tr><td>1 <span class=\"unit\">kpc</span></td><td>5<span>.831085118984171e+29</span> <span class=\"unit\">b</span></td></tr><tr><td>2 <span class=\"unit\">kpc</span></td><td>1<span>.1662170237968342e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>3 <span class=\"unit\">kpc</span></td><td>1<span>.7493255356952512e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>4 <span class=\"unit\">kpc</span></td><td>2<span>.3324340475936683e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>5 <span class=\"unit\">kpc</span></td><td>2<span>.9155425594920857e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>6 <span class=\"unit\">kpc</span></td><td>3<span>.4986510713905025e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>7 <span class=\"unit\">kpc</span></td><td>4<span>.081759583288919e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>8 <span class=\"unit\">kpc</span></td><td>4<span>.6648680951873366e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>9 <span class=\"unit\">kpc</span></td><td>5<span>.247976607085754e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>10 <span class=\"unit\">kpc</span></td><td>5<span>.831085118984171e+30</span> <span class=\"unit\">b</span></td></tr><tr><td>20 <span class=\"unit\">kpc</span></td><td>1<span>.1662170237968343e+31</span> <span class=\"unit\">b</span></td></tr><tr><td>50 <span class=\"unit\">kpc</span></td><td>2<span>.9155425594920854e+31</span> <span class=\"unit\">b</span></td></tr><tr><td>100 <span class=\"unit\">kpc</span></td><td>5<span>.831085118984171e+31</span> <span class=\"unit\">b</span></td></tr><tr><td>1000 <span class=\"unit\">kpc</span></td><td>5<span>.831085118984171e+32</span> <span class=\"unit\">b</span></td></tr><tr><td>10000 <span class=\"unit\">kpc</span></td><td>5<span>.83108511898417e+33</span> <span class=\"unit\">b</span></td></tr><tr><td>100000 <span class=\"unit\">kpc</span></td><td>5<span>.831085118984171e+34</span> <span class=\"unit\">b</span></td></tr></table>",
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[
"vara_de_tarea",
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[
"vara_conuquera",
"Vara Conuquera",
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[
"vara_castellana",
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[
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[
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[
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"x_long_desc": "A kiloparsec (kpc) is a unit of length used in astronomy to measure astronomical distances. One kiloparsec is equivalent to 3,262 light-years or approximately 3.086 × 10^16 meters. </p><p>The kiloparsec is defined as one thousand parsecs, where one parsec is the distance at which one astronomical unit subtends an angle of one arcsecond.</p><p>Kiloparsecs are used to measure large distances between celestial objects, such as the size of galaxies or the distance between galactic structures. They provide a convenient scale for expressing vast distances in the universe.",
"y_long_desc": "The Bohr radius is a fundamental unit of length used in atomic physics to describe the size of the ground state orbit of an electron around a proton in a hydrogen atom. One Bohr radius is approximately 5.29177 × 10^(-11) meters or about 0.529 angstroms. </p><p>The Bohr radius is derived from the Bohr model of the atom, which describes the electron's orbit as quantized and stable. It provides a characteristic length scale for the electron's position in its lowest energy state, known as the ground state.</p><p>The Bohr radius is used in atomic and quantum physics to understand the size of atoms, atomic orbitals, and the fundamental structure of matter. It is a key parameter in the Bohr model and provides insight into the scale of atomic interactions and energy levels."
}