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To convert from degree (deg) to arcsecond (arcsec), use the following formula:
arcsecond (arcsec)
= 60 × 60× degree (deg)
= 3600× degree (deg)
Let's convert 5 degree (deg) to arcsecond (arcsec).
Using the formula:
5 × 3600 = 18000
Therefore, 5 degree (deg) is equal to 18000 arcsecond (arcsec).
How many degrees are in one arcsecond? One arcsecond (arcsec) contains 0.00027777777777777777778 degrees (deg) — the inverse of the factor above. Multiplying by 3600 takes you from degrees to arcseconds; multiplying by 0.00027777777777777777778 brings you back.
Put in words: one degree equals 3600 arcseconds, so the degree is the larger unit of this pair. Converting between them never changes the amount of angle being measured — only the size of the unit you count it in.
In geometry and everyday life, we measure angles using degrees.
A degree (represented by the universal symbol °) is the basic unit for measuring rotation. It helps us describe the amount of turn between two lines that meet at a point.
For instance, a perfect corner, like the edge of a book, is a 90° right angle, and one complete, full-circle rotation measures 360°.
The standard of a circle containing 360 degrees (360°) originated with the ancient Babylonians.
They used a base-60 (sexagesimal) number system, and 360 was a perfect number for them because it is highly divisible. Its large number of factors made it incredibly easy to perform fractional calculations in fields like astronomy and geometry.
For fields that require extreme precision, like astronomy, cartography (map-making), and GPS navigation, a single degree is broken down into even smaller units:
This system ensures that even the tiniest angles can be measured with high accuracy.
There is no physical reason a full turn must be 360 of anything. The number is an inheritance from Babylonian astronomy, and it survived for two reasons that still matter.
The first is the calendar. Babylonian astronomers worked with a year of roughly 360 days, so the Sun appeared to advance about one degree along the ecliptic each day — a convenient bookkeeping unit for tracking the sky.
The second is arithmetic, and it is the reason the convention outlived the astronomy. 360 has 24 divisors. It splits evenly into halves, thirds, quarters, fifths, sixths, eighths, ninths, tenths, twelfths, fifteenths, eighteenths, twentieths, twenty-fourths and more. Every common fraction of a turn lands on a whole number of degrees: a right angle is 90°, a third of a turn is 120°, an eighth is 45°. A base-10 alternative such as the gradian, with 400 to a circle, is better for decimal arithmetic but produces fractions for thirds and sixths — which is roughly why it never displaced the degree outside surveying.
Degrees are for people; radians are for mathematics and for machines.
The distinction is not stylistic. In calculus the derivative of sin(x) is cos(x) only when x is in radians; in degrees an awkward factor of π/180 appears and never leaves. Because of this, essentially every programming language's trigonometric library — JavaScript, Python, C, Java — takes radians, not degrees.
That mismatch is a reliable source of bugs. A value that looks plausible but is wrong by a factor of about 57.3 usually means degrees were passed where radians were expected. The conversions worth memorising are:
Scientific calculators expose the same trap through their DEG / RAD / GRAD mode switch, where an unnoticed mode is the classic cause of an answer that is confidently and completely wrong.
An arcsecond (arcsec) is a tiny unit of angular measurement, equal to 1/3600th of a degree.
To put that in perspective, one arcsecond is roughly the angular size of a dime viewed from over a mile away. As a unit in the International System of Units (SI), it's essential for measuring extremely small angles with high precision.
Arcseconds are fundamental in astronomy for measuring the apparent size and separation of celestial objects as seen from Earth.
Because stars and galaxies are so distant, their angular size in the sky is incredibly small. Astronomers use arcseconds to precisely quantify the separation between double stars, the diameter of distant galaxies, and the intricate details of nebulae.
This level of precision is also critical for calculating stellar parallax. This is a method used to determine the distances to nearby stars by measuring their slight shift in position against a distant background as the Earth orbits the Sun over six months.
The arcsecond is directly used to define the parsec (pc), a primary unit for measuring astronomical distances.
A parsec is defined as the distance at which a star would have a parallax angle of exactly one arcsecond. In other words, if an object is one parsec away, it will appear to shift by one arcsecond in the sky as the Earth moves from one side of its orbit to the other.
This direct relationship makes the arcsecond indispensable for building the cosmic distance ladder and mapping the vastness of space.
Beyond the cosmos, arcseconds are crucial for high-precision geography, cartography, and navigation right here on Earth.
Latitude and longitude coordinates are expressed in degrees, minutes, and arcseconds. One arcsecond of latitude corresponds to a nearly constant distance of about 30.92 meters (101.4 feet) on the Earth's surface.
This allows for the highly accurate location pinpointing that is essential for modern GPS systems, land surveying, aviation, and any application requiring precise geographic positioning.
Here are some quick reference conversions from degree (deg) to arcsecond (arcsec):
| degrees | arcseconds |
|---|---|
| 0.000001 deg | 0.0036 arcsec |
| 0.001 deg | 3.6 arcsec |
| 0.1 deg | 360 arcsec |
| 1 deg | 3600 arcsec |
| 2 deg | 7200 arcsec |
| 3 deg | 10800 arcsec |
| 4 deg | 14400 arcsec |
| 5 deg | 18000 arcsec |
| 6 deg | 21600 arcsec |
| 7 deg | 25200 arcsec |
| 8 deg | 28800 arcsec |
| 9 deg | 32400 arcsec |
| 10 deg | 36000 arcsec |
| 20 deg | 72000 arcsec |
| 30 deg | 108000 arcsec |
| 40 deg | 144000 arcsec |
| 50 deg | 180000 arcsec |
| 100 deg | 360000 arcsec |
| 1000 deg | 3600000 arcsec |
| 10000 deg | 36000000 arcsec |