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Right ascension

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167: 809: 1299: 862: 1323: 946: 1275: 185: 1311: 1287: 744:. Coordinates from different epochs must be mathematically rotated to match each other, or to match a standard epoch. Right ascension for "fixed stars" on the equator increases by about 3.1 seconds per year or 5.1 minutes per century, but for fixed stars away from the equator the rate of change can be anything from negative infinity to positive infinity. (To this must be added the 928:. As the equatorial mount became widely adopted for observation, the equatorial coordinate system, which includes right ascension, was adopted at the same time for simplicity. Equatorial mounts could then be accurately pointed at objects with known right ascension and declination by the use of 407:, is similar to right ascension but increases westward rather than eastward. Usually measured in degrees (°), it is the complement of right ascension with respect to 24. It is important not to confuse sidereal hour angle with the astronomical concept of 202:
lies toward the grey arrow, the star marked by a green arrow will appear to rise somewhere in the east about midnight (the Earth drawn from "above" turns anticlockwise). After the observer reaches the green arrow, dawn will over-power (see blue sky
268:(apart from the sun) do so at the September equinox. On those dates at midnight, such objects will reach ("culminate" at) their highest point (their meridian). How high depends on their declination; if 0° declination (i.e. on the 920:, it became possible for astronomers to observe celestial objects in greater detail, provided that the telescope could be kept pointed at the object for a period of time. The easiest way to do that is to use an 20: 924:, which allows the telescope to be aligned with one of its two pivots parallel to the Earth's axis. A motorized clock drive often is used with an equatorial mount to cancel out the 207:) the star's light for about six hours, before it sets on the western horizon. The Right ascension of the star is about 18. 18 means it is a March early-hours star and in 287:. Astronomers have chosen this unit to measure right ascension because they measure a star's location by timing its passage through the highest point in the sky as the 257:. Right ascension is measured continuously in a full circle from that alignment of Earth and Sun in space, that equinox, the measurement increasing towards the east. 740:(including right ascension) are inherently relative to the year of their observation, and astronomers specify them with reference to a particular year, known as an 965:(green)) and increases eastward (towards the left). The lines of right ascension (blue) from pole to pole divide the sky into 24 hours, each equivalent to 15°. 1177:
U.S. Naval Observatory Nautical Almanac Office; U.K. Hydrographic Office; H.M. Nautical Almanac Office (2008). "Time Scales and Coordinate Systems, 2010".
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could have been chosen for right ascension, but it is customarily measured in hours (), minutes (), and seconds (), with 24 being equivalent to a
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is increasing quickly—in AD 2000 it was 2.5h, but when it gets closest to the north celestial pole in 2100 its right ascension will be 6h. The
752:
increase in right ascension by 24h, or about 5.6' per century, whereas stars within 23.5° of an ecliptic pole undergo a net change of
1343: 295:, is the projection of a longitude line onto the celestial sphere. Since a complete circle contains 24 of right ascension or 360° ( 1176: 1087:
Solis, stellæ, aut alterius cujusdam signi, est gradus æquatorus cum quo simul exoritur in sphæra recta"; roughly translated, "
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who measured stars in equatorial coordinates in the 2nd century BC. But Hipparchus and his successors made their
234: 76: 35: 830: 736:, causes the coordinates of stationary celestial objects to change continuously, if rather slowly. Therefore, 938: 46:(blue). Right ascension is measured eastward up to 24 along the celestial equator from the primary direction. 1006: 996: 737: 220: 96: 1091:
of the Sun, stars, or any other sign, is the degree of the equator that rises together in a right sphere"
976: 88: 1265: 910: 388:), they can be used to time the positions of objects in the sky. For example, if a star with RA = 792: 728:
The Earth's axis traces a small circle (relative to its celestial equator) slowly westward about the
215:
the March equinox. If 6 RA the star would be a March late-hours star, at its high (meridian) at dusk.
229:. Both right ascension and longitude measure an angle from a primary direction (a zero point) on an 1236: 869:
got its name. Ancient astronomy was very concerned with the rise and set of celestial objects. The
1132: 819: 254: 765: 208: 146:, the point on the celestial equator that rises with any celestial object as seen from most 1108: 412: 404: 292: 238: 212: 8: 1327: 925: 769: 761: 748:
of a star.) Over a precession cycle of 26,000 years, "fixed stars" that are far from the
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U.S. Naval Observatory Nautical Almanac Office (1992). Seidelmann, P. Kenneth (ed.).
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or parallel sphere). An object's right ascension was its ascension on a right sphere.
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are longest visible (appear throughout the night) at the March equinox; those with 0
1279: 1210: 921: 878: 784: 733: 723: 242: 178: 119: 92: 64: 31: 1216: 1102: 355:(also written as 15″). A full circle, measured in right-ascension units, contains 19: 1021: 929: 166: 1243: 1348: 981: 933: 729: 296: 107: 1204: 1046: 1337: 1026: 749: 745: 684: 560: 473: 397: 155: 131: 1291: 1072: 906: 882: 788: 411:, which measures the angular distance of an object westward from the local 280: 1255: 1232: 986: 435: 291:. The line which passes through the highest point in the sky, called the 174: 139: 84: 80: 27: 1011: 902: 833: in this section. Unsourced material may be challenged and removed. 732:, completing one cycle in about 26,000 years. This movement, known as 408: 379: 189: 901:
The concept of right ascension has been known at least as far back as
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or oblique sphere). At the poles, objects did not rise or set (right,
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in the morning. If 12 RA, the star would be a March all-night star as
1247: 917: 877:(red) which rose or set at the same time as an object (green) on the 352: 332: 226: 932:. The first star catalog to use right ascension and declination was 889:
or right sphere). From almost anywhere else, they were not (center,
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will be on the/at its meridian (at its apparent highest point) 18.5
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As seen from Earth (except at the poles), objects noted to have 12
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of the) point in question above the Earth. When paired with
118:, or the point on the celestial equator that rises with any 225:
Right ascension is the celestial equivalent of terrestrial
1286: 1051:. University Science Books, Mill Valley, CA. p. 735. 315:
of a circle is measured as 1 of right ascension, or 15°;
272:) then at Earth's equator they are directly overhead (at 199: 72: 1205:
MEASURING THE SKY A Quick Guide to the Celestial Sphere
198:
Assuming the day of the year is the March equinox: the
1263: 1107:. Wells and Lilly and J.W. Burditt, Boston. pp.  776:
are always at right ascension 18 and 6 respectively.
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on Earth, where the celestial equator intersects the
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A Compendious Treatise on the Use of Globes and Maps
791:. Prior to J2000.0, astronomers used the successive 331:
of a circle is measured as 1 of right ascension, or
384:Because right ascensions are measured in hours (of 1049:Explanatory Supplement to the Astronomical Almanac 913:, and the use of RA was limited to special cases. 233:. Right ascension is measured from the Sun at the 67:of a particular point measured eastward along the 1335: 392:is at its meridian, then a star with RA = 351:of a circle contains 1 of right ascension, or 265: 261: 34:. The primary direction of the system is the 1017:Right ascension of the ascending node (RAAN) 418: 1225:"(α,δ) – Right Ascension & Declination" 881:. As seen from the equator, both were on a 192:are depicted here. The symbol ♈︎ marks the 1179:The Astronomical Almanac for the Year 2010 1217:Celestial Equatorial Coordinate Explorers 1181:. U.S. Govt. Printing Office. p. B2. 949:The entire sky, divided into two halves. 849:Learn how and when to remove this message 944: 860: 787:. The prefix "J" indicates that it is a 717: 183: 165: 18: 1121: 1100: 1033: 91:specify the location of a point on the 1354:Technical factors of Western astrology 1336: 1222: 1211:Celestial Equatorial Coordinate System 1207:James B. Kaler, University of Illinois 957:(at right, at the intersection of the 1071: 779:The currently used standard epoch is 1131:. Macmillan Co., New York. pp.  831:adding citations to reliable sources 802: 783:, which is January 1, 2000 at 12:00 16:Astronomical equivalent of longitude 13: 1081:. Apud Johannem Blaeu. p. 65. 14: 1365: 1198: 249:from south to north at the March 177:(green) as seen from outside the 1321: 1309: 1297: 1285: 1273: 807: 253:and is currently located in the 1344:Astronomical coordinate systems 818:needs additional citations for 795:B1875.0, B1900.0, and B1950.0. 1219:University of Nebraska-Lincoln 1213:University of Nebraska-Lincoln 1185: 1169: 1160: 1148: 1139: 1115: 1094: 1065: 1040: 161: 130:, where the celestial equator 1: 939:Historia Coelestis Britannica 403:Sidereal hour angle, used in 30:as seen on the inside of the 1128:An Introduction to Astronomy 1007:Geographic coordinate system 997:Equatorial coordinate system 649: 541: 469: 241:, which is the place on the 221:Equatorial coordinate system 97:equatorial coordinate system 38:, the ascending node of the 7: 977:Celestial coordinate system 969: 756:0h. The right ascension of 688: 564: 477: 335:(also written as 15′); and 10: 1370: 1166:Moulton (1916), pp. 92–95. 916:With the invention of the 798: 721: 377: 245:where the Sun crosses the 218: 885:from pole to pole (left, 440: 434: 431: 428: 425: 419:Symbols and abbreviations 1237:University of Nottingham 89:astronomical coordinates 1191:Blaeu (1668), p. 40–41. 1145:Moulton (1916), p. 126. 1155:Explanatory Supplement 1101:Lathrop, John (1821). 1078:Institutio Astronomica 966: 898: 738:equatorial coordinates 216: 181: 111: 47: 1223:Merrifield, Michael. 953:(blue) begins at the 948: 873:was the point on the 864: 718:Effects of precession 386:rotation of the Earth 187: 169: 22: 1034:Notes and references 911:ecliptic coordinates 827:improve this article 405:celestial navigation 255:constellation Pisces 239:First Point of Aries 142:. It contrasts with 1175:see, for instance, 1123:Moulton, Forest Ray 770:South Ecliptic Pole 762:North Ecliptic Pole 205:Rayleigh scattering 1002:Equinoctial colure 967: 899: 217: 182: 48: 1250:) – to determine 895:sphaera parallela 875:celestial equator 859: 858: 851: 715: 714: 353:15 seconds of arc 333:15 minutes of arc 270:celestial equator 247:celestial equator 144:oblique ascension 69:celestial equator 44:celestial equator 1361: 1326: 1325: 1324: 1314: 1313: 1312: 1302: 1301: 1300: 1290: 1289: 1278: 1277: 1276: 1269: 1244:Sidereal pointer 1240: 1192: 1189: 1183: 1182: 1173: 1167: 1164: 1158: 1152: 1146: 1143: 1137: 1136: 1119: 1113: 1112: 1098: 1092: 1082: 1073:Blaeu, Guilielmi 1069: 1063: 1062: 1044: 926:Earth's rotation 922:equatorial mount 879:celestial sphere 854: 847: 843: 840: 834: 811: 803: 793:Besselian epochs 755: 724:Axial precession 710: 708: 707: 706: 705: 699: 696: 695: 682: 680: 679: 676: 673: 666: 664: 663: 660: 657: 646: 644: 643: 642: 641: 635: 632: 625: 623: 622: 621: 620: 614: 611: 604: 602: 601: 598: 595: 581: 579: 578: 575: 572: 571: 558: 556: 555: 552: 549: 538: 536: 535: 534: 533: 527: 524: 517: 515: 514: 511: 508: 494: 492: 491: 488: 485: 484: 466: 464: 463: 460: 457: 423: 422: 395: 391: 374: 373: 372: 364: 363: 362: 350: 348: 347: 344: 341: 330: 328: 327: 324: 321: 314: 312: 311: 308: 305: 267: 263: 243:celestial sphere 179:celestial sphere 120:celestial object 114:) refers to the 93:celestial sphere 65:angular distance 61: 32:celestial sphere 1369: 1368: 1364: 1363: 1362: 1360: 1359: 1358: 1334: 1333: 1332: 1322: 1320: 1310: 1308: 1298: 1296: 1284: 1274: 1272: 1264: 1201: 1196: 1195: 1190: 1186: 1174: 1170: 1165: 1161: 1153: 1149: 1144: 1140: 1120: 1116: 1099: 1095: 1089:Right ascension 1070: 1066: 1059: 1045: 1041: 1036: 1031: 1022:Setting circles 972: 951:Right ascension 930:setting circles 891:sphaera obliqua 867:right ascension 855: 844: 838: 835: 824: 812: 801: 753: 730:celestial poles 726: 720: 703: 701: 700: 697: 693: 692: 691: 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856: 815: 813: 806: 800: 797: 750:ecliptic poles 722:Main article: 719: 716: 713: 712: 687: 650: 648: 588: 584: 583: 563: 542: 540: 501: 497: 496: 476: 470: 468: 450: 446: 445: 439: 433: 430: 427: 420: 417: 398:sidereal hours 297:degrees of arc 219:Main article: 163: 160: 112:ascensio recta 15: 9: 6: 4: 3: 2: 1366: 1355: 1352: 1350: 1347: 1345: 1342: 1341: 1339: 1329: 1319: 1317: 1307: 1305: 1295: 1293: 1288: 1283: 1281: 1271: 1270: 1267: 1259: 1258: 1253: 1249: 1245: 1242: 1238: 1234: 1230: 1229:Sixty Symbols 1226: 1221: 1218: 1215: 1212: 1209: 1206: 1203: 1202: 1188: 1180: 1172: 1163: 1156: 1151: 1142: 1134: 1130: 1129: 1124: 1118: 1110: 1106: 1105: 1097: 1090: 1086: 1080: 1079: 1074: 1068: 1060: 1058:0-935702-68-7 1054: 1050: 1043: 1039: 1028: 1027:Sidereal time 1025: 1023: 1020: 1018: 1015: 1013: 1010: 1008: 1005: 1003: 1000: 998: 995: 993: 990: 988: 985: 983: 980: 978: 975: 974: 964: 960: 956: 955:March equinox 952: 947: 943: 941: 940: 935: 931: 927: 923: 919: 914: 912: 908: 907:star catalogs 904: 896: 892: 888: 887:sphaera recta 884: 880: 876: 872: 868: 863: 853: 850: 842: 832: 828: 822: 821: 816:This section 814: 810: 805: 804: 796: 794: 790: 786: 782: 777: 775: 771: 767: 763: 759: 751: 747: 746:proper motion 743: 739: 735: 731: 725: 686: 651: 589: 586: 585: 562: 543: 502: 499: 498: 475: 471: 451: 448: 447: 444: 437: 424: 416: 414: 410: 406: 401: 399: 387: 381: 376: 354: 334: 298: 294: 290: 289:Earth rotates 286: 282: 277: 275: 271: 258: 256: 252: 248: 244: 240: 236: 235:March equinox 232: 228: 222: 214: 210: 206: 201: 195: 194:March equinox 191: 186: 180: 176: 172: 168: 159: 157: 156:oblique angle 153: 149: 145: 141: 137: 133: 129: 125: 122:as seen from 121: 117: 113: 109: 105: 102:An old term, 100: 98: 94: 90: 86: 82: 78: 77:March equinox 74: 70: 66: 62: 56: 53:(abbreviated 52: 45: 42:(red) on the 41: 37: 36:March equinox 33: 29: 25: 21: 1328:Solar System 1256: 1251: 1228: 1187: 1178: 1171: 1162: 1154: 1150: 1141: 1127: 1117: 1103: 1096: 1088: 1084: 1077: 1067: 1048: 1042: 950: 937: 915: 900: 894: 890: 886: 883:great circle 870: 866: 845: 836: 825:Please help 820:verification 817: 789:Julian epoch 778: 727: 402: 383: 281:angular unit 278: 259: 224: 170: 143: 115: 103: 101: 58: 54: 50: 49: 23: 1316:Outer space 1304:Spaceflight 1233:Brady Haran 987:Declination 436:Sexagesimal 285:full circle 196:direction. 190:hour angles 175:declination 173:(blue) and 162:Explanation 140:right angle 85:declination 81:hour circle 28:declination 1338:Categories 1012:Hour angle 903:Hipparchus 734:precession 409:hour angle 380:Hour angle 378:See also: 367:24 × 60 = 132:intersects 1280:Astronomy 1248:Torquetum 918:telescope 871:ascension 375:, or 24. 237:i.e. the 227:longitude 148:latitudes 116:ascension 71:from the 63:) is the 57:; symbol 1235:for the 1125:(1916). 1075:(1668). 992:Ecliptic 970:See also 959:ecliptic 839:May 2012 768:and the 605:minute, 413:meridian 394:20 00 00 293:meridian 213:opposite 209:blue sky 188:Various 87:, these 79:to the ( 40:ecliptic 1266:Portals 963:equator 799:History 781:J2000.0 758:Polaris 709:⁠ 690:⁠ 681:⁠ 669:⁠ 665:⁠ 653:⁠ 645:⁠ 628:⁠ 624:⁠ 607:⁠ 603:⁠ 591:⁠ 587:Second 580:⁠ 566:⁠ 557:⁠ 545:⁠ 537:⁠ 520:⁠ 516:⁠ 504:⁠ 500:Minute 493:⁠ 479:⁠ 465:⁠ 453:⁠ 443:radians 400:later. 390:1 30 00 349:⁠ 337:⁠ 329:⁠ 317:⁠ 313:⁠ 301:⁠ 251:equinox 231:equator 152:horizon 136:horizon 128:equator 95:in the 75:at the 1055:  774:Dorado 754:  647:circle 626:hour, 539:circle 518:hour, 467:circle 438:system 432:Symbol 274:zenith 154:at an 1349:Angle 1292:Stars 1135:–126. 1111:, 39. 766:Draco 742:epoch 683:′, 15 559:°, 15 449:Hour 429:Value 365:, or 346:86400 138:at a 124:Earth 108:Latin 1053:ISBN 865:How 711:rad 582:rad 495:rad 426:Unit 326:1440 279:Any 134:the 26:and 1257:DEC 1133:125 1083:, " 936:'s 909:in 829:by 772:in 764:in 704:200 667:°, 662:240 640:400 619:600 577:720 532:440 441:In 371:440 361:400 299:), 276:). 200:Sun 126:'s 73:Sun 1340:: 1252:RA 1231:. 1227:. 1109:29 785:TT 702:43 638:86 600:60 513:60 490:12 472:15 462:24 415:. 359:86 310:24 266:RA 262:RA 158:. 110:: 99:. 55:RA 1268:: 1260:. 1254:/ 1246:( 1239:. 1061:. 852:) 846:( 841:) 837:( 823:. 698:/ 694:π 685:″ 678:4 675:/ 672:1 659:/ 656:1 634:/ 631:1 617:3 613:/ 610:1 597:/ 594:1 574:/ 570:π 561:′ 554:4 551:/ 548:1 530:1 526:/ 523:1 510:/ 507:1 487:/ 483:π 474:° 459:/ 456:1 369:1 343:/ 340:1 323:/ 320:1 307:/ 304:1 106:( 60:α

Index


declination
celestial sphere
March equinox
ecliptic
celestial equator
angular distance
celestial equator
Sun
March equinox
hour circle
declination
astronomical coordinates
celestial sphere
equatorial coordinate system
Latin
celestial object
Earth
equator
intersects
horizon
right angle
latitudes
horizon
oblique angle

declination
celestial sphere

hour angles

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