Fifty-seven navigational stars and additionally the star Polaris are given a special status in the field of celestial navigation. Of the approximately six thousand stars visible to the naked eye under optimal conditions, these selected stars are among the brightest and span thirty-eight constellations of the celestial sphere from the declination of −70° to +89°. Many of the selected stars were named in antiquity by the Babylonians, Greeks, Romans, and Arabs.
The star Polaris, often called either the "Pole Star" or the "North Star", is treated specially due to its proximity to the north celestial pole. When navigating in the Northern Hemisphere, a simple and quick technique can be used with Polaris to determine the observers latitude or, for larger maritime vessels can be used to calculate any gyrocompass error that may exist. The other fifty-seven selected stars have daily positions given in nautical almanacs, aiding the navigator in efficiently performing observations on them. A second group of 115 "tabulated stars" can also be used for celestial navigation, but are often less familiar to the navigator and require extra calculations.
Although Polaris can quickly and simply give a solution for latitude in the northern hemisphere, it can not participate in giving a position fix including longitude - it is for this reason it is excluded from the list of 57 primary navigational stars, each of which can be used to produce (in conjunction with each other, known time in relation to the prime meridian and a set of sight reduction tables) an actual latitudinal and longitudinal positional fix.
For purposes of identification, the positions of navigational stars — expressed as declination and sidereal hour angle — are often rounded to the nearest degree. In addition to tables, star charts provide an aid to the navigator in identifying the navigational stars, showing constellations, relative positions, and brightness.
In practical use for sight reductions whilst at sea, tables can further assist a navigator by giving approximate altitudes (angles above the horizon) and azimuths (degrees as read from the compass) from an assumed or estimated position, usually helping to quickly determine the location and then quickly identify a particular navigational star that may be useful for a sight reduction.
Under optimal conditions, approximately six thousand stars are visible to the naked eye of an observer on Earth. [1] Of these, fifty-eight stars are known in the field of navigational astronomy as "selected stars", including nineteen stars of the first magnitude, thirty-eight stars of the second magnitude, and Polaris. [1] The selection of the stars is made by His Majesty's Nautical Almanac Office and the US Naval Observatory, in the production of the yearly Nautical Almanac which the two organizations have published jointly since 1958. [2] Criteria in the choice of stars includes their distribution across the celestial sphere, brightness, and ease of identification. [3] Information for another 115 stars, known as "tabulated stars", is also available to the navigator. [1] This list provides information on the name, approximate position in the celestial sphere, and apparent magnitude of the 58 selected stars in tabular form and by star charts.
These stars are typically used in two ways by the navigator. The first is to obtain a line of position by use of a sextant observation and the techniques of celestial navigation. [4] Multiple lines of position can be intersected to obtain a position known as a celestial fix. The second typical use of the navigational stars is to determine gyrocompass error by computing the azimuth of a star and comparing it to an azimuth measured using the ship's gyrocompass. [5] Numerous other applications also exist.
Navigators typically refer to stars using one of two naming systems for stars: common names and Bayer's designations. [1] All of the selected stars have had a common name since 1953, and many were named in antiquity by the Arabs, Greeks, Romans, and Babylonians. [1] Bayer's naming convention has been in use since 1603, and consists of a Greek letter combined with the possessive form of the star's constellation. [1] Both names are shown for each star in the tables and charts below.
Each star's approximate position on the celestial sphere is given using the equatorial coordinate system. The celestial sphere is an imaginary globe of infinite size with the Earth at its center. [6] Positions on the celestial sphere are often expressed using two coordinates: declination and sidereal hour angle, which are similar to latitude and longitude on the surface of the Earth. To define declination, the Earth's equator is projected out to the celestial sphere to construct the celestial equator, and declination is measured in degrees north or south of this celestial equator. [6] Sidereal hour angle is a measurement between 0° and 360°, indicating how far west a body is from an arbitrarily chosen point on the celestial sphere called the First Point of Aries . Note that right ascension, as used by astronomers, is 360° minus the sidereal hour angle.
The final characteristic provided in the tables and star charts is the star's brightness, expressed in terms of apparent magnitude. Magnitude is a logarithmic scale of brightness, designed so that a body of one magnitude is approximately 2.512 times brighter than a body of the next magnitude. [Note 1] [7] Thus, a body of magnitude 1 is 2.5125 (~100) times brighter than a body of magnitude 6. [8] The dimmest stars that can be seen through a 200-inch terrestrial telescope are of the 20th magnitude, and very bright objects like the Sun and a full Moon have magnitudes of −26.7 and −12.6 respectively. [8]
Key to the table | |
---|---|
Column title | Description |
No. | The number used to identify stars in navigation publications and star charts. [Note 2] |
Common name | The name of the star commonly used navigation publications and star charts. |
Bayer designation | Another name of the star which combines a Greek letter with the possessive form of its constellation's Latin name. |
Etymology of common name | Etymology of the common name. [9] |
SHA | Sidereal hour angle (SHA), the angular distance west of the vernal equinox. |
Dec. | Declination, the angular distance north or south of the celestial equator. |
App. magnitude | Apparent magnitude, an indicator of the star's brightness. |
The table of navigational stars provides several types of information. In the first column is the identifying index number, followed by the common name, the Bayer designation, and the etymology of the common name. Then the star's approximate position, suitable for identification purposes, is given in terms of declination and sidereal hour angle, followed by the star's magnitude. The final column presents citations to the sources of the data, The American Practical Navigator and the star's entry at the SIMBAD database, a project of the Strasbourg Astronomical Data Center or CDS.
No. [Note 2] | Common name | Bayer designation | Etymology of common name | SHA | Declination | App. magnitude | References |
---|---|---|---|---|---|---|---|
1 | Alpheratz | Andromedae | αthe horse's navel | 358 | N 29° | 2.06 | [9] [10] |
2 | Ankaa | Phoenicis | αcoined name, "phoenix bird" in Arabic | 354 | S 42° | 2.37 | [9] [11] |
3 | Schedar | Cassiopeiae | αthe breast (of Cassiopeia) | 350 | N 56° | 2.25 | [9] [12] |
4 | Diphda | Ceti | βthe second frog (Fomalhaut was once the first) | 349 | S 18° | 2.04 | [9] [13] |
5 | Achernar | Eridani | αend of the river (Eridanus) | 336 | S 57° | 0.50 | [9] [14] |
6 | Hamal | Arietis | αfull-grown lamb | 328 | N 23° | 2.00 | [9] [15] |
7 | Acamar | Eridani | θanother form of Achernar | 316 | S 40° | 3.2 | [9] [16] |
8 | Menkar | Ceti | αnose (of the whale) | 315 | N 04° | 2.5 | [9] [17] |
9 | Mirfak | Persei | αelbow of the Pleiades | 309 | N 50° | 1.82 | [9] [18] |
10 | Aldebaran | Tauri | αfollower (of the Pleiades) | 291 | N 16° | 0.85 var [Note 3] | [9] [19] |
11 | Rigel | Orionis | βfoot (left foot of Orion) | 282 | S 08° | 0.12 | [9] [20] |
12 | Capella | Aurigae | αlittle she-goat | 281 | N 46° | 0.71 | [9] [21] |
13 | Bellatrix | Orionis | γfemale warrior | 279 | N 06° | 1.64 | [9] [22] |
14 | Elnath | Tauri | βone butting with the horns | 279 | N 29° | 1.68 | [9] [23] |
15 | Alnilam | Orionis | εstring of pearls | 276 | S 01° | 1.70 | [9] [24] |
16 | Betelgeuse | Orionis | αthe hand of al-Jauzā (i.e. Orion) | 271 | N 07° | 0.58 var [Note 3] | [9] [25] |
17 | Canopus | Carinae | αcity of ancient Egypt | 264 | S 53° | −0.72 | [9] [26] |
18 | Sirius | Canis Majoris | αthe scorching one (popularly, the dog star) | 259 | S 17° | −1.47 | [9] [27] |
19 | Adhara | Canis Majoris | εthe virgin(s) | 256 | S 29° | 1.51 | [9] [28] |
20 | Procyon | Canis Minoris | αbefore the dog (rising before the dog star, Sirius) | 245 | N 05° | 0.34 | [9] [29] |
21 | Pollux | Geminorum | βZeus' other twin son (Castor, α Gem, is the first twin) | 244 | N 28° | 1.15 | [9] [30] |
22 | Avior | Carinae | ε1coined name | 234 | S 59° | 2.4 | [9] [31] |
23 | Suhail | Velorum | λshortened form of Al Suhail, one Arabic name for Canopus | 223 | S 43° | 2.23 | [9] [32] |
24 | Miaplacidus | Carinae | βquiet or still waters | 222 | S 70° | 1.70 | [9] [33] |
25 | Alphard | Hydrae | αsolitary star of the serpent | 218 | S 09° | 2.00 | [9] [34] |
26 | Regulus | Leonis | αthe prince | 208 | N 12° | 1.35 | [9] [35] |
27 | Dubhe | Ursae Majoris | α1the bear's back | 194 | N 62° | 1.87 | [9] [36] |
28 | Denebola | Leonis | βtail of the lion | 183 | N 15° | 2.14 | [9] [37] |
29 | Gienah | Corvi | γright wing of the raven | 176 | S 17° | 2.80 | [9] [38] |
30 | Acrux | Crucis | α1coined from Bayer name | 174 | S 63° | 1.40 | [9] [39] |
31 | Gacrux | Crucis | γcoined from Bayer name | 172 | S 57° | 1.63 | [9] [40] |
32 | Alioth | Ursae Majoris | εanother form of Capella | 167 | N 56° | 1.76 | [9] [41] |
33 | Spica | Virginis | αthe ear of corn | 159 | S 11° | 1.04 | [9] [42] |
34 | Alkaid | Ursae Majoris | ηleader of the daughters of the bier | 153 | N 49° | 1.85 | [9] [43] |
35 | Hadar | Centauri | βleg of the centaur | 149 | S 60° | 0.60 | [9] [44] |
36 | Menkent | Centauri | θshoulder of the centaur | 149 | S 36° | 2.06 | [9] [45] |
38 | Rigil Kentaurus | Centauri | α1foot of the centaur | 140 | S 61° | −0.01 | [9] [46] |
37 | Arcturus | Bootis | αthe bear's guard | 146 | N 19° | −0.04 var [Note 3] | [9] [47] |
39 | Zubenelgenubi | Librae | αsouthern claw (of the scorpion) | 138 | S 16° | 3.28 | [9] [48] |
40 | Kochab | Ursae Minoris | βshortened form of "north star" (named when it was that, [Note 4] ca. 1500 BC – AD 300). | 137 | N 74° | 2.08 | [9] [49] |
41 | Alphecca | Corona Borealis | αfeeble one (in the crown) | 127 | N 27° | 2.24 | [9] [50] |
42 | Antares | Scorpii | αrival of Mars (in color) | 113 | S 26° | 1.09 | [9] [51] |
43 | Atria | Trianguli Australis | αcoined from Bayer name | 108 | S 69° | 1.92 | [9] [52] |
44 | Sabik | Ophiuchi | ηsecond winner or conqueror | 103 | S 16° | 2.43 | [9] [53] |
45 | Shaula | Scorpii | λcocked-up part of the scorpion's tail | 097 | S 37° | 1.62 | [9] [54] |
46 | Rasalhague | Ophiuchi | αhead of the serpent charmer | 096 | N 13° | 2.10 | [9] [55] |
47 | Eltanin | Draconis | γhead of the dragon | 091 | N 51° | 2.23 | [9] [56] |
48 | Kaus Australis | Sagittarii | εsouthern part of the bow (of Sagittarius) | 084 | S 34° | 1.80 | [9] [57] |
49 | Vega | Lyrae | αthe falling eagle or vulture | 081 | N 39° | 0.03 | [9] [58] |
50 | Nunki | Sagittarii | σconstellation of the holy city (Eridu) | 076 | S 26° | 2.06 | [9] [59] |
51 | Altair | Aquilae | αflying eagle or vulture | 063 | N 09° | 0.77 | [9] [60] |
52 | Peacock | Pavonis | αCoined from the English name of the constellation | 054 | S 57° | 1.91 | [9] [61] |
53 | Deneb | Cygni | αtail of the hen | 050 | N 45° | 1.25 | [9] [62] |
54 | Enif | Pegasi | εnose of the horse | 034 | N 10° | 2.40 | [9] [63] |
55 | Al Na'ir | Gruis | αbright one (of the southern fish's tail) | 028 | S 47° | 1.74 | [9] [64] |
56 | Fomalhaut | Piscis Austrini | αmouth of the southern fish | 016 | S 30° | 1.16 | [9] [65] |
57 | Markab | Pegasi | αsaddle (of Pegasus) | 014 | N 15° | 2.49 | [9] [66] |
[Note 2] | *Polaris [9] | Ursae Minoris | αthe pole (star) | 319 | N 89° | 2.01 var [Note 3] | [9] [67] |
Navigators often use star charts to identify a star by its position relative to other stars. References like the Nautical Almanac and The American Practical Navigator provide four star charts, covering different portions of the celestial sphere. Two of these charts are azimuthal equidistant projections of the north and south poles. The other two cover the equatorial region of the celestial sphere, from the declination of 30° south to 30° north. The two equatorial charts are mercator projections, one for the eastern hemisphere of the celestial sphere and one for the western hemisphere. Note that unlike familiar maps, east is shown to the left and west is shown to the right. With this orientation, the navigator can hold the star chart overhead, and the arrangement of the stars on the chart will resemble the stars in the sky. [1]
In the star charts, constellations are labelled with capital letters and indicated by dotted lines collecting their stars. The 58 selected stars for navigation are shown in blue and labelled with their common name, star number, and a Greek letter to indicate their Bayer designation. The additional 115 tabulated stars that can also be used for navigation are shown in red and labelled with a Greek letter to indicate their Bayer designation. Some additional stars not suitable for navigation are also included on the charts to indicate constellations, they are presented as unlabelled small red dots.
The equatorial region of the celestial sphere's eastern hemisphere includes 17 navigational stars from Alpheratz in the constellation Andromeda to Denebola in Leo. It also includes stars from the constellations Cetus, Aries, Taurus, Orion, Canis Major and Minor, Gemini, and Hydra. Of particular note among these stars are "the dog star" Sirius, the brightest star in the sky, and four stars of the easily identified constellation Orion.
The equatorial region of the celestial sphere's western hemisphere includes 13 navigational stars from Gienah in the constellation Corvus to Markab in Pegasus. It also includes stars from the constellations Virgo, Bootes, Libra, Corona Borealis, Scorpio, Ophiuchus, Sagittarius, and Aquila. The variable star Arcturus is the brightest star in this group.
The 11 northern stars are those with a declination between 30° north and 90° north. They are listed in order of decreasing sidereal hour angle, or from the vernal equinox westward across the sky. Starting with Schedar in the constellation Cassiopeia, the list includes stars from the constellations Auriga, the Great and Little Bears, Draco, Lyra and Cygnus. The two brightest northern stars are Vega and Capella.
In the star chart to the right, declination is shown by the radial coordinate, starting at 90° north in the center and decreasing to 30° north at the outer edge. Sidereal hour angle is shown as the angular coordinate, starting at 0° at the left of the chart, and increasing counter-clockwise.
The 18 southern stars are those with a declination between 30° south and 90° south. They are listed in order of decreasing sidereal hour angle, or from the vernal equinox westward across the sky. Starting with Ankaa in the constellation Phoenix, the list includes stars from the constellations Eridanus, Carina, Crux, Centaurus, Libra, Triangulum Australe, Scorpio, Sagittarius, Pavo, and Grus. Canopus, Rigil Kentaurus, Achernar, and Hadar are the brightest stars in the southern sky.
In the star chart to the right, declination is shown by the radial coordinate, starting at 90° south in the center and decreasing to 30° south at the outer edge. Sidereal hour angle is shown as the angular coordinate, starting at 0° at the right of the chart, and increasing clockwise.
Aries is one of the constellations of the zodiac. It is located in the Northern celestial hemisphere between Pisces to the west and Taurus to the east. The name Aries is Latin for ram. Its old astronomical symbol is (♈︎). It is one of the 48 constellations described by the 2nd century astronomer Ptolemy, and remains one of the 88 modern constellations. It is a mid-sized constellation ranking 39th in overall size, with an area of 441 square degrees.
Boötes is a constellation in the northern sky, located between 0° and +60° declination, and 13 and 16 hours of right ascension on the celestial sphere. The name comes from Latin: Boōtēs, which comes from Ancient Greek: Βοώτης, romanized: Boṓtēs 'herdsman' or 'plowman'.
Corona Australis is a constellation in the Southern Celestial Hemisphere. Its Latin name means "southern crown", and it is the southern counterpart of Corona Borealis, the northern crown. It is one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and it remains one of the 88 modern constellations. The Ancient Greeks saw Corona Australis as a wreath rather than a crown and associated it with Sagittarius or Centaurus. Other cultures have likened the pattern to a turtle, ostrich nest, a tent, or even a hut belonging to a rock hyrax.
Hydrus is a small constellation in the deep southern sky. It was one of twelve constellations created by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman and it first appeared on a 35-cm (14 in) diameter celestial globe published in late 1597 in Amsterdam by Plancius and Jodocus Hondius. The first depiction of this constellation in a celestial atlas was in Johann Bayer's Uranometria of 1603. The French explorer and astronomer Nicolas Louis de Lacaille charted the brighter stars and gave their Bayer designations in 1756. Its name means "male water snake", as opposed to Hydra, a much larger constellation that represents a female water snake. It remains below the horizon for most Northern Hemisphere observers.
Tucana is a constellation in the southern sky, named after the toucan, a South American bird. It is one of twelve constellations conceived in the late sixteenth century by Petrus Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. Tucana first appeared on a 35-centimetre-diameter (14 in) celestial globe published in 1598 in Amsterdam by Plancius and Jodocus Hondius and was depicted in Johann Bayer's star atlas Uranometria of 1603. French explorer and astronomer Nicolas Louis de Lacaille gave its stars Bayer designations in 1756. The constellations Tucana, Grus, Phoenix and Pavo are collectively known as the "Southern Birds".
Triangulum Australe is a small constellation in the far Southern Celestial Hemisphere. Its name is Latin for "the southern triangle", which distinguishes it from Triangulum in the northern sky and is derived from the acute, almost equilateral pattern of its three brightest stars. It was first depicted on a celestial globe as Triangulus Antarcticus by Petrus Plancius in 1589, and later with more accuracy and its current name by Johann Bayer in his 1603 Uranometria. The French explorer and astronomer Nicolas Louis de Lacaille charted and gave the brighter stars their Bayer designations in 1756.
Ursa Minor, also known as the Little Bear, is a constellation located in the far northern sky. As with the Great Bear, the tail of the Little Bear may also be seen as the handle of a ladle, hence the North American name, Little Dipper: seven stars with four in its bowl like its partner the Big Dipper. Ursa Minor was one of the 48 constellations listed by the 2nd-century astronomer Ptolemy, and remains one of the 88 modern constellations. Ursa Minor has traditionally been important for navigation, particularly by mariners, because of Polaris being the north pole star.
The north and south celestial poles are the two points in the sky where Earth's axis of rotation, indefinitely extended, intersects the celestial sphere. The north and south celestial poles appear permanently directly overhead to observers at Earth's North Pole and South Pole, respectively. As Earth spins on its axis, the two celestial poles remain fixed in the sky, and all other celestial points appear to rotate around them, completing one circuit per day.
Phoenix is a minor constellation in the southern sky. Named after the mythical phoenix, it was first depicted on a celestial atlas by Johann Bayer in his 1603 Uranometria. The French explorer and astronomer Nicolas Louis de Lacaille charted the brighter stars and gave their Bayer designations in 1756. The constellation stretches from roughly −39° to −57° declination, and from 23.5h to 2.5h of right ascension. The constellations Phoenix, Grus, Pavo and Tucana, are known as the Southern Birds.
Andromeda is one of the 48 constellations listed by the 2nd-century Greco-Roman astronomer Ptolemy, and one of the 88 modern constellations. Located in the northern celestial hemisphere, it is named for Andromeda, daughter of Cassiopeia, in the Greek myth, who was chained to a rock to be eaten by the sea monster Cetus. Andromeda is most prominent during autumn evenings in the Northern Hemisphere, along with several other constellations named for characters in the Perseus myth. Because of its northern declination, Andromeda is visible only north of 40° south latitude; for observers farther south, it lies below the horizon. It is one of the largest constellations, with an area of 722 square degrees. This is over 1,400 times the size of the full moon, 55% of the size of the largest constellation, Hydra, and over 10 times the size of the smallest constellation, Crux.
In observational astronomy, culmination is the passage of a celestial object across the observer's local meridian. These events are also known as meridian transits, used in timekeeping and navigation, and measured precisely using a transit telescope.
Auriga is a constellation in the northern celestial hemisphere. It is one of the 88 modern constellations; it was among the 48 constellations listed by the 2nd-century astronomer Ptolemy. Its name is Latin for '(the) charioteer', associating it with various mythological beings, including Erichthonius and Myrtilus. Auriga is most prominent during winter evenings in the northern Hemisphere, as are five other constellations that have stars in the Winter Hexagon asterism. Because of its northern declination, Auriga is only visible in its entirety as far south as −34°; for observers farther south it lies partially or fully below the horizon. A large constellation, with an area of 657 square degrees, it is half the size of the largest, Hydra.
Pictor is a constellation in the Southern Celestial Hemisphere, located between the star Canopus and the Large Magellanic Cloud. Its name is Latin for painter, and is an abbreviation of the older name Equuleus Pictoris. Normally represented as an easel, Pictor was named by Abbé Nicolas-Louis de Lacaille in the 18th century. The constellation's brightest star is Alpha Pictoris, a white main-sequence star around 97 light-years away from Earth. Pictor also hosts RR Pictoris, a cataclysmic variable star system that flared up as a nova, reaching apparent (visual) magnitude 1.2 in 1925 before fading into obscurity.
Leo Minor is a small and faint constellation in the northern celestial hemisphere. Its name is Latin for "the smaller lion", in contrast to Leo, the larger lion. It lies between the larger and more recognizable Ursa Major to the north and Leo to the south. Leo Minor was not regarded as a separate constellation by classical astronomers; it was designated by Johannes Hevelius in 1687.
Pavo is a constellation in the southern sky whose name is Latin for 'peacock'. Pavo first appeared on a 35-cm (14 in) diameter celestial globe published in 1598 in Amsterdam by Petrus Plancius and Jodocus Hondius and was depicted in Johann Bayer's star atlas Uranometria of 1603, and was likely conceived by Plancius from the observations of Pieter Dirkszoon Keyser and Frederick de Houtman. French explorer and astronomer Nicolas-Louis de Lacaille gave its stars Bayer designations in 1756. The constellations Pavo, Grus, Phoenix and Tucana are collectively known as the "Southern Birds".
Sigma Octantis is a solitary star in the Octans constellation that forms the pole star of the Southern Hemisphere. Its name is also written as σ Octantis, abbreviated as Sigma Oct or σ Oct, and it is officially named Polaris Australis. The star is positioned one degree away from the southern celestial pole of the Southern Hemisphere, lying in nearly opposite direction to the North Star on the celestial sphere.
A pole star is a visible star that is approximately aligned with the axis of rotation of an astronomical body; that is, a star whose apparent position is close to one of the celestial poles. On Earth, a pole star would lie directly overhead when viewed from the North or the South Pole.
Spherical astronomy, or positional astronomy, is a branch of observational astronomy used to locate astronomical objects on the celestial sphere, as seen at a particular date, time, and location on Earth. It relies on the mathematical methods of spherical trigonometry and the measurements of astrometry.
Iota Herculis is a fourth-magnitude variable star system in the constellation Hercules, consisting of at least four stars all about 139 parsecs away. The brightest is a β Cephei variable, a pulsating star.
NGC 1624, also known as Sh2-212 in the Sharpless catalog, is a very young open cluster in the constellation Perseus inside an emission nebula. It was discovered by German-British astronomer William Herschel in 1790. NGC 1624 is about 20,000 ly from Earth, and latest estimates give it an age of less than 4 million years. Its apparent magnitude is 11.8, and apparent diameter is about 3.0 arc minutes. Its celestial location is right ascension (α) 04h 40m 36.0s and declination (δ) +50° 27′ 42″. It is potentially an area of massive star formation.