Polaris and your latitude
From Seoul, at latitude 37.6° north, Polaris stands about 37.6° above the northern horizon.
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The star that hardly moves
In the last unit the whole sky turned round the celestial poles. Look north from Korea and there is a moderately bright star almost exactly at the northern pole: Polaris, the North Star. It is not the brightest star in the sky. Its catalogue magnitude is 2.02, so dozens of stars outshine it. What makes it special is its place. In the Yale Bright Star Catalogue, which gives positions for the year 2000, its declination is 89.26°, about 0.74° from the pole. Precession has since brought it a little closer, to about 0.63° in 2026, a bit more than the width of the full Moon. As the sky turns, Polaris traces a tiny circle and stays almost still while everything else wheels round it.
Polaris has not always been the pole star, and it will not stay one. Earth's axis wobbles slowly like a spinning top, a motion called precession that takes about 26,000 years for one full circle (NASA). Working the precession formulas forward from the catalogue position, the pole comes closest to Polaris around 2100, at about 0.46°, and then drifts away. NASA's StarChild pages note that in about 13,000 years the bright star Vega will be the pole star.
Why the pole's height equals your latitude
Picture yourself at the North Pole. Earth's axis points straight up, so the celestial pole is at your zenith and Polaris is overhead at altitude 90°, which is also your latitude. Now walk south to the equator, latitude 0°. You have walked a quarter of the way round Earth, and your idea of "straight up" has tipped by 90° with you. The axis now lies flat along the northern horizon, so Polaris sits on the horizon at altitude 0°. Anywhere between, the tilt is in proportion: every degree of latitude you move south lowers the pole by one degree. That is why the altitude of the celestial pole equals your latitude.
Sailors used this for centuries. Measure the height of Polaris above the sea horizon with a quadrant or sextant, add a small correction for the offset of about 0.6°, and you have your latitude without any map. Try it in the model: Seoul's latitude is 37.57° and the card shows Polaris at about 37.9° on the night of 18 October 2026. The extra few tenths are that offset; the model uses the catalogue's year-2000 positions, so its offset is the slightly larger 0.74°.
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Stars that never set
Near the pole some stars circle without ever touching the horizon. They are circumpolar. A star stays up all night, all year, if its distance from the pole is less than the pole's height. At Seoul the pole is 37.6° up, so any star with a declination above 90° − 37.6° = 52.4° never sets. Dubhe, at declination 61.8°, is circumpolar from Seoul and never dips below about 9° altitude. Alkaid, the end of the Dipper's handle at 49.3°, is not: for a short while each day it slips about 3° below the northern horizon. Go farther north and more stars become circumpolar; at the North Pole every visible star is, and at the equator none is.
The southern sky
The same rule works in reverse for stars far to the south: a star whose declination is more than 52.4° south of the celestial equator never rises at Seoul. Canopus, the second brightest star at night, has a declination of −52.7°, just past that limit. EarthSky notes that Canopus never rises for places north of about 37° north. From Seogwipo on Jeju, at about 33.3° north, it climbs about 4° above the southern horizon on winter evenings, and the Seogwipo astronomy centre holds viewing nights for it each February. Korean tradition calls it Noinseong, the star of the old man, linked with long life. The Southern Cross is farther south still: its brightest star, Acrux, is at declination −63.1°, so it only rises south of about 27° north.
The south celestial pole has no bright marker. The nearest naked-eye star, Sigma Octantis, is magnitude 5.47 in the catalogue, too faint to see from most towns. Southern navigators instead use the long axis of the Southern Cross, which points roughly towards the pole. Pick Sydney in the model and look south.
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- Busan is at about 35.2° north. About how high above the northern horizon is Polaris there?
- Where is Polaris for someone on the equator?
- Overhead
- On the northern horizon
- Never visible from anywhere
- At latitude 37.6° N, stars with a declination above how many degrees never set?
- Alkaid has declination 49.3°. Is it circumpolar from Seoul?
- Yes
- No, it dips about 3° below the horizon
- Canopus has declination −52.7°. What is its highest altitude seen from Seogwipo at 33.25° N? (one decimal)
- Why does Polaris hardly move during the night?
- It is the closest star
- It lies within about 1° of the celestial pole
- It is the brightest star
- Which stars in the Big Dipper point to Polaris?
- Merak and Dubhe, the end of the bowl
- Mizar and Alkaid, the handle
- Megrez and Phecda
- Dubhe to Polaris is 28.7° and Merak to Dubhe is 5.4°. How many Merak to Dubhe gaps is that? (one decimal)
- Polaris will come closest to the pole around which year?
- 1900
- 2100
- 14,000
- Acrux, the brightest star of the Southern Cross, is at declination −63.1°. South of what latitude in degrees north can it rise above the horizon? (one decimal)
- Polaris is magnitude 2.02 but sits within about 0.7° of the north celestial pole (0.63° in 2026).
- The altitude of the celestial pole equals your latitude.
- Stars closer to the pole than its altitude are circumpolar: above 52.4° declination at Seoul.
- Canopus (−52.7°) never rises at Seoul but is visible low in the south from Seogwipo.
- The south celestial pole has no bright star; the Southern Cross points towards it.
Sources for this course (20)
- Yale Bright Star Catalogue 5th Revised Ed. (Hoffleit and Warren 1991, CDS V/50, cdsarc.cds.unistra.fr/ftp/V/50/, NASA HEASARC BSC5P)
- public domain
- IAU The Constellations (iau.org/public/themes/constellations)
- IAU Catalog of Star Names, WGSN (iau.org/public/themes/naming_stars, list pas.rochester.edu/~emamajek/WGSN/IAU-CSN.txt)
- US Naval Observatory sidereal time formula (aa.usno.navy.mil/faq/GAST)
- NASA Glenn "Telling Time by the Stars" (grc.nasa.gov/WWW/k-12/Numbers/Math/Mathematical_Thinking/telling_time_by_the_stars.htm)
- NASA Space Place "What Are Constellations?" (spaceplace.nasa.gov/constellations) and "How Long Is One Day on Other Planets?" (spaceplace.nasa.gov/days)
- NASA Earth Fact Sheet (nssdc.gsfc.nasa.gov/planetary/factsheet/earthfact.html)
- JPL Approximate Positions of the Planets, Standish and Williams (ssd.jpl.nasa.gov/planets/approx_pos.html)
- spot-checked against JPL Horizons for 2026-10-18
- IAU Office of Astronomy for Education glossary "Zodiac" (astro4edu.org/resources/glossary/term/391)
- Sky and Telescope "A Sign of the Times" (skyandtelescope.org/astronomy-news/observing-news/a-sign-of-the-times)
- EarthSky "Sun enters Ophiuchus" (earthsky.org/astronomy-essentials/sun-in-ophiuchus-november-30-to-december-18)
- NASA StarChild "Why is Polaris the North Star?" (starchild.gsfc.nasa.gov/docs/StarChild/questions/question64.html)
- IAU press release iau1603 on the WGSN and 227 star names (iau.org/news/pressreleases/detail/iau1603)
- Huntington Library on Bayer's Uranometria, 1603 (huntington.org/uranometria)
- Wikipedia Apparent magnitude for Pogson 1856 (cross-check)
- EarthSky "Can you see Canopus" (earthsky.org/brightest-stars/few-know-the-second-brightest-star-canopus)
- Seogwipo Astronomy Science Center notices on Canopus (jejumaeil.net/news/articleView.html?idxno=112240)
- KASI (kasi.re.kr) for Korean star names.
Checked: 2026-10-18