{"id":652,"date":"2026-07-25T06:11:02","date_gmt":"2026-07-25T06:11:02","guid":{"rendered":"https:\/\/physicsfundamentalsinfo.com\/blog\/?p=652"},"modified":"2026-08-29T21:49:21","modified_gmt":"2026-08-29T21:49:21","slug":"refractive-index","status":"publish","type":"post","link":"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/refractive-index\/","title":{"rendered":"Refractive Index (n = c\/v): Formula &amp; Table"},"content":{"rendered":"\n<div class=\"pf-citation\"><div class=\"eyebrow\">Definition<\/div><p>\n\nRefractive index (n) measures how much a material slows light: it is the ratio of the speed of light in a vacuum, c, to its speed in the material, v, so n = c\/v. Water has n = 1.33, typical glass about 1.5 and diamond 2.42 \u2014 the larger the value, the slower the light and the more strongly it bends.\n\n<\/p><\/div>\n\n<p>Hold a cheap cubic zirconia next to a real diamond and, at arm&#8217;s length, they look identical. Tilt them under a lamp, though, and the diamond erupts with far more flash. Almost the entire difference comes down to one number: 2.42 versus 2.16.<\/p>\n\n<p>That number is the refractive index, and this page is built around it. The full lookup table comes first, then the ratio behind it, how to measure it yourself, and where those decimal places quietly run the modern world \u2014 from spectacle lenses to fibre broadband.<\/p>\n\n<h2>Refractive Index Table: n Values for 15 Common Materials<\/h2>\n\n<p>The refractive index of common materials runs from exactly 1 for a vacuum, through 1.33 for water and about 1.5 for glass, up to 2.42 for diamond. Unless stated otherwise, the values below are measured with yellow sodium light (589 nm) at roughly 20 &deg;C \u2014 the standard reference conditions used in data tables.<\/p>\n\n<div class=\"pf-table-scroll\" style=\"display:block;width:100%;max-width:100%;overflow-x:auto;-webkit-overflow-scrolling:touch;margin:1.5em 0;\">\n<table style=\"width:100%;border-collapse:collapse;\">\n<thead>\n<tr>\n<th style=\"padding:10px 12px;border-bottom:2px solid #C8932A;text-align:left;\">Material<\/th>\n<th style=\"padding:10px 12px;border-bottom:2px solid #C8932A;text-align:left;\">Refractive index (n)<\/th>\n<th style=\"padding:10px 12px;border-bottom:2px solid #C8932A;text-align:left;\">Speed of light inside (v = c\/n)<\/th>\n<\/tr>\n<\/thead>\n<tbody>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Vacuum<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1 (exact)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">3.00 &times; 10<sup>8<\/sup> m\/s (c itself)<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Air (0 &deg;C, 1 atm)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.000293<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">&asymp; c (0.03% slower)<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Ice (0 &deg;C)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.31<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.29 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Water (20 &deg;C)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.333<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.25 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Ethanol<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.361<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.20 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Fused quartz (silica)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.458<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.06 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Olive oil<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.47<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.04 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Glycerol<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.473<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.04 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Crown glass<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.52<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.97 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Table salt (NaCl)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.544<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.94 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Polycarbonate<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.586<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.89 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Flint glass (dense)<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.62<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.85 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Sapphire<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.77<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.69 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Cubic zirconia<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.16<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.39 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<tr><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">Diamond<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">2.417<\/td><td style=\"padding:9px 12px;border-bottom:1px solid #D9CFB8;\">1.24 &times; 10<sup>8<\/sup> m\/s<\/td><\/tr>\n<\/tbody>\n<\/table>\n<\/div>\n\n<p>Notice the pattern as you read down. Gases barely rise above 1, everyday liquids cluster between 1.3 and 1.5, glasses and clear plastics sit around 1.5 to 1.6, and gemstones own the top of the chart.<\/p>\n\n<p>Even air&#8217;s tiny 1.000293 matters more than it looks. Laser interferometers measure lengths in wavelengths of light, so precision labs must correct for air&#8217;s index \u2014 <a href=\"https:\/\/emtoolbox.nist.gov\/wavelength\/documentation.asp\" target=\"_blank\" rel=\"noopener\">NIST maintains dedicated calculators<\/a> (the Ciddor and Edl&eacute;n equations) for exactly that correction.<\/p>\n\n<p>One caveat before you quote a value in an exam: n shifts in the third decimal place with the colour of the light and with temperature. More on that below.<\/p>\n\n<figure class=\"pf-figure\" style=\"margin:1.6em 0;\"><img src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/08\/refractive-index-bar-comparing-indices-vacuum-air.webp\" width=\"468\" height=\"336\" alt=\"Refractive index - Bar chart comparing the refractive indices of vacuum, air, water, crown glass, sapphire, cubic zirconia and diamond on a scale from 1 to 2.42\" loading=\"lazy\" decoding=\"async\" style=\"width:100%;height:auto;max-width:234px;display:block;margin:0 auto;\" \/><\/figure>\n<p style=\"text-align:center;font-size:14px;font-style:italic;\">The refractive index scale: every everyday transparent material sits between vacuum (1) and diamond (2.42).<\/p>\n\n<h2>What Is the Refractive Index?<\/h2>\n\n<p>The refractive index is a dimensionless number that tells you how many times slower light travels in a material than in a vacuum. Glass with n = 1.5 slows light to two-thirds of its vacuum speed; diamond, at 2.42, drags it to well under half.<\/p>\n\n<p>You will also see the same quantity called the <strong>index of refraction<\/strong> \u2014 the usual term in American textbooks \u2014 or described through &#8220;optical density&#8221;: the optically denser medium is simply the one with the higher n. The reference speed, c, is the fastest anything in the universe can travel, a story we unpack in our guide to <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/modern-physics\/speed-of-light\/\">the speed of light<\/a>.<\/p>\n\n<p>Why does light slow down at all, and why does slowing make a ray bend? That mechanism \u2014 waves, wavefronts and the marching-band turn \u2014 is the territory of our <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/reflection-and-refraction\/\">reflection and refraction guide<\/a>. Here, we stay with the number itself: what it equals, how to look it up, and how to use it.<\/p>\n\n<h2>The Refractive Index Formula: n = c\/v<\/h2>\n\n<p>The refractive index formula is n = c\/v: divide the speed of light in a vacuum by the speed of light in the material.<\/p>\n\n<div class=\"pf-formula\">n = c \/ v<\/div>\n\n<ul>\n<li><strong>n<\/strong> \u2014 refractive index of the material (dimensionless, no units)<\/li>\n<li><strong>c<\/strong> \u2014 speed of light in a vacuum = 299,792,458 m\/s, usually rounded to 3.00 &times; 10<sup>8<\/sup> m\/s<\/li>\n<li><strong>v<\/strong> \u2014 speed of light inside the material, in metres per second (m\/s)<\/li>\n<\/ul>\n\n<p>Because it is one speed divided by another, the units cancel completely \u2014 n is a pure number, and it is at least 1 for every ordinary transparent material. Rearranged, the same relationship hands you the speed directly:<\/p>\n\n<div class=\"pf-formula\">v = c \/ n<\/div>\n\n<p>That rearrangement is exactly how the third column of the table above was built. Try it once by hand \u2014 glass: v = 3.00 &times; 10<sup>8<\/sup> &divide; 1.5 = 2.00 &times; 10<sup>8<\/sup> m\/s \u2014 or work it out instantly either way round with our <a href=\"https:\/\/physicsfundamentalsinfo.com\/calculators\/refractive-index\">Refractive Index Calculator<\/a>, which solves for n or for v.<\/p>\n\n<p>A quick sanity check worth keeping: every transparent solid and liquid you are likely to meet has n between 1 and about 2.65. If your calculation returns 0.44 or 4.4, the ratio has almost certainly been flipped upside down.<\/p>\n\n<div class=\"pf-sim-slot\"><div class=\"pf-sim-slot-header\"><span class=\"icon-dot\"><\/span><span class=\"label\">Refractive Index Lab<\/span><\/div><div class=\"pf-sim-slot-body\">\n<style>\n.pf-sim-frame{\nwidth:100%;\nborder:none;\nheight:600px\n}\n@media(max-width:760px){\n.pf-sim-frame{\nheight:1000px\n}\n}\n<\/style>\n<iframe\nsrc=\"\/labs\/refractive-index.html?embed=1\"\nclass=\"pf-sim-frame\"\nloading=\"lazy\">\n<\/iframe>\n<\/div><\/div>\n\n<h2>Absolute vs Relative Refractive Index<\/h2>\n\n<p>An absolute refractive index compares a material with a vacuum, while a relative refractive index compares one material directly with another. Every value in the table above is absolute; the relative version is what you need when light crosses from one substance straight into a second.<\/p>\n\n<div class=\"pf-formula\">n<sub>21<\/sub> = n<sub>2<\/sub> \/ n<sub>1<\/sub> = v<sub>1<\/sub> \/ v<sub>2<\/sub><\/div>\n\n<p>Here n<sub>21<\/sub> is the index of medium 2 relative to medium 1. Take light passing from water (1.333) into crown glass (1.52): n<sub>21<\/sub> = 1.52 &divide; 1.333 = 1.14, so the light travels 1.14 times slower in the glass than it did in the water.<\/p>\n\n<p>Run the trip in reverse and you get 1.333 &divide; 1.52 = 0.88 \u2014 and yes, a relative index below 1 is perfectly fine. It simply says light speeds up crossing that boundary. One handy exam shortcut: air&#8217;s absolute index (1.0003) is so close to 1 that &#8220;from air into X&#8221; problems use the absolute values directly.<\/p>\n\n<h2>How Do You Measure Refractive Index?<\/h2>\n\n<p>You measure refractive index either by tracing how a light ray bends and applying Snell&#8217;s law, or by reading it straight off an instrument called a refractometer. Four methods cover almost every situation:<\/p>\n\n<ul>\n<li><strong>Glass-block ray tracing (the classroom method).<\/strong> Shine a ray into a rectangular block, mark the path, and measure the angles of incidence and refraction from the normal. Then n = sin &theta;<sub>1<\/sub> &divide; sin &theta;<sub>2<\/sub> for light arriving from air.<\/li>\n<li><strong>Critical-angle method.<\/strong> With a semicircular block, find the angle at which the emerging ray just grazes the surface; the index follows from n = 1 &divide; sin &theta;<sub>c<\/sub>.<\/li>\n<li><strong>Refractometer.<\/strong> A drop of liquid on an Abbe or handheld refractometer returns n to four decimal places in seconds \u2014 the standard tool in chemistry, brewing and gemmology, as this <a href=\"https:\/\/www.utsc.utoronto.ca\/webapps\/chemistryonline\/production\/refractive.php\" target=\"_blank\" rel=\"noopener\">University of Toronto lab guide<\/a> walks through.<\/li>\n<li><strong>Apparent depth.<\/strong> For a transparent liquid, n = real depth &divide; apparent depth \u2014 the same effect that makes a swimming pool look only about three-quarters as deep as it is.<\/li>\n<\/ul>\n\n<p>The single most common student slip? Measuring angles from the glass surface instead of from the normal \u2014 the imaginary line at 90&deg; to the boundary. Every angle in refraction work is measured from the normal, and marking that line first saves the lost mark.<\/p>\n\n<p>In practice, professionals also correct for temperature: a liquid&#8217;s reading drifts by roughly 0.0004 to 0.0005 per degree Celsius, which is why bench refractometers circulate temperature-controlled water around the sample.<\/p>\n\n<h2>Why Does Refractive Index Change with Wavelength?<\/h2>\n\n<p>Refractive index changes with wavelength because a material&#8217;s electrons respond more strongly to some frequencies of light than others, so violet light is slowed more than red. In a typical crown glass, n climbs from about 1.51 in the red to about 1.53 in the violet.<\/p>\n\n<p>That spread is called dispersion, and it is the whole reason a prism fans white light into a spectrum and raindrops split sunlight into a rainbow \u2014 a story we trace, prism in hand, in our guide to the <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/dispersion-of-light\/\">dispersion of light<\/a>.<\/p>\n\n<p>It is also why careful tables pin the wavelength down. The standard reference is the sodium D-line at 589 nm \u2014 the warm yellow of an old street lamp \u2014 so that two labs quoting &#8220;n = 1.52&#8221; for the same glass are genuinely measuring the same thing.<\/p>\n\n<p>Diamond takes dispersion to extremes. Its index climbs from about 2.41 in the red to about 2.44 in the violet, and that spread is the &#8220;fire&#8221; jewellers prize: each colour exits a facet at a slightly different angle, splashing tiny rainbows around the room.<\/p>\n\n<h2>Real-World Examples of Refractive Index<\/h2>\n\n<p>From gem testing to fibre broadband, the refractive index is a working number that whole industries measure, tune and buy by. Here are four places it earns its keep.<\/p>\n\n<h3>Spotting a fake diamond<\/h3>\n\n<p>Diamond (2.42), cubic zirconia (2.16) and moissanite (2.65) look similar at a glance, but their indices give them away through sparkle, fire and light return. Here is a working gemmologist&#8217;s detail: a standard contact refractometer only reads up to about 1.81, so diamond and its imitations all show &#8220;over the limit&#8221; \u2014 one reason testers lean on thermal conductivity instead.<\/p>\n\n<h3>Fibre-optic broadband<\/h3>\n\n<p>The glass core of an optical fibre has n &asymp; 1.468, so your data physically travels at roughly two-thirds of c \u2014 about 4.9 microseconds per kilometre. In practice that index, not the electronics, sets the floor on internet latency between continents.<\/p>\n\n<h3>Thinner spectacle lenses<\/h3>\n\n<p>A strong prescription in standard n = 1.5 plastic needs thick, heavy edges. High-index lens materials at 1.67 or 1.74 bend light more per millimetre, so the same correction fits in a visibly slimmer, lighter lens \u2014 you are literally paying for decimal places of n.<\/p>\n\n<h3>Sugar, beer and antifreeze<\/h3>\n\n<p>Dissolving sugar in water nudges its refractive index upward in a predictable way. A handheld Brix refractometer converts that shift straight into a sugar percentage, which is how brewers track fermentation and how winemakers time the harvest. The same trick, recalibrated, tests the strength of engine coolant.<\/p>\n\n<h2>Common Misconceptions About Refractive Index<\/h2>\n\n<p>Four wrong beliefs cause most refractive index mistakes. Clearing them now will save marks later.<\/p>\n\n<h3>&#8220;A higher refractive index means a denser material.&#8221;<\/h3>\n\n<p>Not necessarily \u2014 optical density and mass density are different things. Olive oil (n = 1.47) is optically denser than water (n = 1.333), yet it floats on top. The index tracks how strongly a material&#8217;s electrons respond to light, not how much the material weighs.<\/p>\n\n<h3>&#8220;Light changes frequency when it slows down.&#8221;<\/h3>\n\n<p>No \u2014 the frequency is fixed by the source and never changes at a boundary. What shrinks is the wavelength, to &lambda;\/n, exactly compensating for the lower speed; our <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/frequency-formula\/\">frequency formula guide<\/a> unpacks how v, f and &lambda; lock together. Since colour rides on frequency, red light stays red inside the glass.<\/p>\n\n<figure class=\"pf-figure\" style=\"margin:1.6em 0;\"><img src=\"https:\/\/physicsfundamentalsinfo.com\/blog\/wp-content\/uploads\/2026\/08\/refractive-index-light-wavefronts-crossing-glass-slab.webp\" width=\"360\" height=\"214\" alt=\"Refractive index - Diagram of light wavefronts crossing a glass slab: wavefront spacing shrinks from wavelength lambda in air to lambda divided by n inside the glass, while the frequency stays constant\" loading=\"lazy\" decoding=\"async\" style=\"width:100%;height:auto;max-width:180px;display:block;margin:0 auto;\" \/><\/figure>\n<p style=\"text-align:center;font-size:14px;font-style:italic;\">Inside the glass the wavefronts bunch up: wavelength drops to &lambda;\/n while the frequency stays exactly the same.<\/p>\n\n<h3>&#8220;A material&#8217;s refractive index is one fixed number.&#8221;<\/h3>\n\n<p>Any single value is a snapshot at one wavelength and one temperature. Crown glass runs from roughly 1.51 (red) to 1.53 (violet), and a warm liquid reads a few ten-thousandths lower than a cold one. For rough work, one number is fine; for precise work, quote the conditions.<\/p>\n\n<h3>&#8220;Nothing can have an index below 1.&#8221;<\/h3>\n\n<p>For visible light in ordinary transparent materials, n is indeed always above 1. But X-rays travelling through glass have n a whisker below 1: the wave&#8217;s phase pattern moves slightly faster than c. No energy or information ever outruns light in a vacuum, so relativity is perfectly safe.<\/p>\n\n<h2>How Refractive Index Relates to Refraction and Total Internal Reflection<\/h2>\n\n<p>The refractive index sets both how sharply light bends at a boundary and whether it can escape at all. Every headline behaviour of light at a surface is these table values fed into two short equations.<\/p>\n\n<p>The bending is governed by Snell&#8217;s law, which weighs the two indices against each other:<\/p>\n\n<div class=\"pf-formula\">n<sub>1<\/sub> sin &theta;<sub>1<\/sub> = n<sub>2<\/sub> sin &theta;<sub>2<\/sub><\/div>\n\n<p>Bigger jump in n, bigger bend \u2014 and that single line carries a five-step solving method, worked traps and all, in our dedicated <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/snells-law-explained\/\">Snell&#8217;s law guide<\/a>.<\/p>\n\n<p>Run light the other way, from a high-n material towards a low-n one, and there is an angle beyond which it cannot get out:<\/p>\n\n<div class=\"pf-formula\">sin &theta;<sub>c<\/sub> = n<sub>2<\/sub> \/ n<sub>1<\/sub><\/div>\n\n<p>That critical angle is about 41&deg; for glass into air, about 49&deg; for water into air, and a remarkably tight 24.4&deg; for diamond \u2014 which is precisely why a well-cut diamond traps light and fires it back out of the top. Past the critical angle, the boundary becomes a perfect mirror, the effect our <a href=\"https:\/\/physicsfundamentalsinfo.com\/blog\/waves\/total-internal-reflection\/\">total internal reflection guide<\/a> explores from optical fibres to sparkling gems.<\/p>\n\n<p>Look the numbers up once; the rest is trigonometry.<\/p>\n\n<h2>Worked Problems<\/h2>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 1<\/div><div class=\"pf-problem-question\">The refractive index of water is 1.333. Calculate the speed of light in water. Take c = 3.00 &times; 10^8 m\/s.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Rearrange the definition n = c\/v to solve for speed: v = c\/n.<\/p>\n<p>Step 2: Substitute with units: v = (3.00 &times; 10<sup>8<\/sup> m\/s) &divide; 1.333.<\/p>\n<p>Step 3: Solve: v = 2.2506 &times; 10<sup>8<\/sup> m\/s.<\/p>\n<p><strong>Answer: v = 2.25 &times; 10<sup>8<\/sup> m\/s (3 s.f.)<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 2<\/div><div class=\"pf-problem-question\">Light travels at 1.24 &times; 10^8 m\/s through a clear gemstone. Find its refractive index and identify the likely material using the table above.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Apply the definition directly: n = c\/v.<\/p>\n<p>Step 2: Substitute with units: n = (3.00 &times; 10<sup>8<\/sup> m\/s) &divide; (1.24 &times; 10<sup>8<\/sup> m\/s).<\/p>\n<p>Step 3: Solve: n = 2.42 (dimensionless \u2014 the units cancel).<\/p>\n<p><strong>Answer: n = 2.42, matching diamond (2.417) in the reference table.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 3<\/div><div class=\"pf-problem-question\">Light passes from water (n = 1.333) into crown glass (n = 1.52). Calculate the refractive index of the glass relative to the water.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Use the relative index formula: n<sub>21<\/sub> = n<sub>2<\/sub> \/ n<sub>1<\/sub>, with water as medium 1 and glass as medium 2.<\/p>\n<p>Step 2: Substitute: n<sub>21<\/sub> = 1.52 &divide; 1.333.<\/p>\n<p>Step 3: Solve: n<sub>21<\/sub> = 1.140.<\/p>\n<p><strong>Answer: n<sub>21<\/sub> = 1.14 \u2014 light travels 1.14 times slower in the glass than in the water.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 4<\/div><div class=\"pf-problem-question\">A ray of light in air strikes crown glass (n = 1.52) at an angle of incidence of 50.0&deg;. Find the angle of refraction. Take n(air) = 1.00.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Apply Snell&#8217;s law: n<sub>1<\/sub> sin &theta;<sub>1<\/sub> = n<sub>2<\/sub> sin &theta;<sub>2<\/sub>, both angles measured from the normal.<\/p>\n<p>Step 2: Substitute: (1.00)(sin 50.0&deg;) = (1.52)(sin &theta;<sub>2<\/sub>), so sin &theta;<sub>2<\/sub> = 0.766 &divide; 1.52 = 0.504.<\/p>\n<p>Step 3: Solve: &theta;<sub>2<\/sub> = sin<sup>-1<\/sup>(0.504) = 30.26&deg;.<\/p>\n<p><strong>Answer: &theta;<sub>2<\/sub> = 30.3&deg; \u2014 the ray bends towards the normal, as expected entering a higher-n medium.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 5<\/div><div class=\"pf-problem-question\">Calculate the critical angle for light travelling from diamond (n = 2.417) into air (n = 1.00).<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: Use the critical angle relation for light heading from a dense medium (1) to a rarer one (2): sin &theta;<sub>c<\/sub> = n<sub>2<\/sub> \/ n<sub>1<\/sub>.<\/p>\n<p>Step 2: Substitute: sin &theta;<sub>c<\/sub> = 1.00 &divide; 2.417 = 0.4137.<\/p>\n<p>Step 3: Solve: &theta;<sub>c<\/sub> = sin<sup>-1<\/sup>(0.4137) = 24.44&deg;.<\/p>\n<p><strong>Answer: &theta;<sub>c<\/sub> = 24.4&deg; \u2014 any ray inside the diamond hitting a facet beyond this shallow angle is totally internally reflected.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 6<\/div><div class=\"pf-problem-question\">Sodium light of wavelength 589 nm in a vacuum enters water (n = 1.333). Find its wavelength and its frequency inside the water.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: In a medium the wavelength shrinks to &lambda; = &lambda;<sub>0<\/sub>\/n, while the frequency f = c\/&lambda;<sub>0<\/sub> is unchanged.<\/p>\n<p>Step 2: Substitute for wavelength: &lambda; = 589 nm &divide; 1.333 = 441.9 nm. For frequency: f = (3.00 &times; 10<sup>8<\/sup> m\/s) &divide; (589 &times; 10<sup>-9<\/sup> m).<\/p>\n<p>Step 3: Solve: &lambda; = 442 nm; f = 5.09 &times; 10<sup>14<\/sup> Hz.<\/p>\n<p><strong>Answer: &lambda; = 442 nm inside the water; f = 5.09 &times; 10<sup>14<\/sup> Hz, exactly the same as in the vacuum.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 7<\/div><div class=\"pf-problem-question\">A swimming pool is really 1.50 m deep. Viewed from directly above, how deep does it appear? Take n(water) = 1.333.<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: For viewing along the normal, n = real depth &divide; apparent depth, so apparent depth = real depth &divide; n.<\/p>\n<p>Step 2: Substitute with units: apparent depth = 1.50 m &divide; 1.333.<\/p>\n<p>Step 3: Solve: apparent depth = 1.125 m.<\/p>\n<p><strong>Answer: about 1.13 m \u2014 the pool looks roughly three-quarters of its true depth, a genuine drowning hazard worth remembering.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<div class=\"pf-problem\"><div class=\"pf-problem-num\">Problem 8<\/div><div class=\"pf-problem-question\">A data pulse travels along 10.0 km of optical fibre whose glass core has n = 1.468. How long does the journey take, and how much longer is that than the same distance in a vacuum?<\/div><details><summary>Show Solution<\/summary><div class=\"pf-problem-solution\">\n<p><strong>Solution:<\/strong><\/p>\n<p>Step 1: The speed in the core is v = c\/n, so the transit time is t = distance &divide; v = nL\/c.<\/p>\n<p>Step 2: Substitute with units: t = (1.468 &times; 1.00 &times; 10<sup>4<\/sup> m) &divide; (3.00 &times; 10<sup>8<\/sup> m\/s).<\/p>\n<p>Step 3: Solve: t = 4.89 &times; 10<sup>-5<\/sup> s = 48.9 microseconds. In a vacuum: t = (1.00 &times; 10<sup>4<\/sup> m) &divide; (3.00 &times; 10<sup>8<\/sup> m\/s) = 3.33 &times; 10<sup>-5<\/sup> s = 33.3 microseconds.<\/p>\n<p>Step 4: Compare: 48.9 &minus; 33.3 = 15.6 microseconds of extra delay caused purely by the glass&#8217;s refractive index.<\/p>\n<p><strong>Answer: t = 4.89 &times; 10<sup>-5<\/sup> s (48.9 microseconds) \u2014 about 15.6 microseconds longer than in a vacuum.<\/strong><\/p>\n<\/div><\/details><\/div>\n\n<h2>Frequently Asked Questions<\/h2>\n\n<details class=\"pf-faq-item\"><summary>What is the refractive index of water?<\/summary><div class=\"pf-faq-item-answer\">\n\nWater&#8217;s refractive index is 1.333, measured with sodium light (589 nm) at 20 &deg;C. That means light travels 1.333 times slower in water than in a vacuum \u2014 about 2.25 &times; 10<sup>8<\/sup> m\/s. The value creeps down slightly as water warms, and seawater sits a little higher, near 1.34, because dissolved salt raises it.\n\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Does the refractive index have units?<\/summary><div class=\"pf-faq-item-answer\">\n\nNo \u2014 the refractive index is dimensionless. It is a ratio of two speeds, metres per second divided by metres per second, so the units cancel completely. That is why the same value, such as 1.52 for crown glass, works unchanged in any unit system without conversion.\n\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>How do you calculate refractive index?<\/summary><div class=\"pf-faq-item-answer\">\n\nDivide the speed of light in a vacuum by its speed in the material: n = c\/v. If you do not know the speed, use angles instead: for light entering from air, n equals sin of the incidence angle divided by sin of the refraction angle, both measured from the normal. The two routes give the same number.\n\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Which material has the highest refractive index?<\/summary><div class=\"pf-faq-item-answer\">\n\nAmong everyday transparent materials, diamond leads at 2.42. A few specialist crystals go higher \u2014 moissanite reaches about 2.65 and rutile roughly 2.6 in visible light \u2014 while semiconductors such as silicon reach around 3.5, though only for infrared light, since they are opaque to visible wavelengths.\n\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>Can a refractive index be less than 1?<\/summary><div class=\"pf-faq-item-answer\">\n\nYes, in special cases. For X-rays passing through glass, n dips just below 1, meaning the wave&#8217;s phase pattern moves slightly faster than c. No energy or information travels faster than light in a vacuum, so relativity survives intact. For visible light in ordinary transparent materials, n is always greater than 1.\n\n<\/div><\/details>\n\n<details class=\"pf-faq-item\"><summary>What is the difference between refractive index and optical density?<\/summary><div class=\"pf-faq-item-answer\">\n\nIn optics, calling one material more optically dense than another simply means it has the higher refractive index, so light travels more slowly through it. Optical density is not the same as mass density: olive oil is optically denser than water yet physically lighter, which is why it floats. In lab spectroscopy, &#8220;optical density&#8221; can also mean absorbance \u2014 a different quantity entirely.\n\n<\/div><\/details>\n","protected":false},"excerpt":{"rendered":"<p>The refractive index n = c\/v tells you how much a material slows light. 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