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Dhaptar lintang ing rasi lintang Vulpecula

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rasi lintang vulpecula

Pratélan lintang ing rasi lintang vulpécula inggih punika satunggaling pratélan rasi lintang ingkang ngewrat nama- nama lintang ingkang wonten ing rasi lintang vulpécula. Ing ngandhap punika inggih lintang-lintang ingkang wonten ing rasi lintang Vulpecula.

Vulpecula

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Vulpecula inggih punika salah satunggaling konstelasi ingkang alit, saha lemes ingkang wonten ing belahan bumi sisih lor. Ing basa Latin, Vulpecula gadhah teges "rubah alit". Konstelasi Vulpecula inggih dipuntepangaken sepisanan déning astronom Semir, inggih punika Johannes Hevelius ing abad kaping 17. Nama aslinipun inggih punika "Vulpecula et Anser" ("rubah alit lan angsa) lan kagambaraken minangka rubah ingkang nembé nyepeng angsa ing rahangipun. Lajeng rubah lan angsanipun dipunpisah lajeng dados konstelasi ingkang kepisah lan ing satunggaling wekdal saged nggabung dados satunggal malih. Angsa punika ing wekdal sapunika dipunwujudaken dados lintang [8981] Anser, alpha Vulpecula.

Vulpecula boten gadhah kathah lintang ingkang padhang ingkang langkung saking magnitude kaping sekawan. [8981] alpha Vulpecula, ugi dipunmangertosi minangka Anser, Lucida Anseris lan Lukida, inggih punika satunggaling giant abrit kanthi magnitude ingkang cetha inggih punika 4,44. Punika inggih lintang ingkang padhang piyambak wonten ing konstelasi punika. Lintang punika tebihipun kirang langkung 296, 5 taun dahya saking bumi. Punika inggih satunggaling lintang optik binar.[1] Pulsar ingkang sepisanan inggih punika PSR B1919+21, kapanggih ing Vulpecula ing Cambridge ing taun 1967. Punika kapanggih déning astronom radio[2] lan ingkang menang bebungah Nobel Hewish Antony lan astrofisikawan [[Jocelyn Bell Burnell.[3] Vulpecula ngewrat kalih bendha langit ingkang misuwur inggih punika Dumbbell Nebula lan Brocchi’s Cluster. Dumbbell Nebula (Messier 27) inggih punika planit nebula ingkang sepusanan kapanggih déning astronom Prancis inggih punika Charles Messier ing taun 1764. Nebula punika inggih padhang, amba lan gampil kapanggih kanthi teleskop. Planet nebula punika dumunung ing jarak ingkang tebihipun kirang langkung 1.360 taun cahya saking bumi. Pusatipun lintang ing Dumbbell Nebula inggih punika kurcaci pethak ingkang langkung ageng tinimbang kurcaci pethak sanèsipun ingkang sampun misuwur.

Nama B F HD HIP RA Dec vis.
mag. 		abs.
mag. 		Jarak (tc) Sp. class Kondisi Nama
lain 		Asal
basa 		Arti
CK Vul 11[4] 19j 47m 38.1d +27° 18′ 48″ 2.7 (max) ea Nova Vulpeculae 1670[5]
α Vul α 6 183439 95771 19j 28m 42.41d +24° 39′ 54.6″ 4.44 −0.35 296 M0 comp Anser[6] Latin angsa
23 Vul 23 192806 99874 20j 15m 46.16d +27° 48′ 51.2″ 4.50 −0.51 328 K3III
31 Vul (r)[7] 31 198809 103004 20j 52m 07.73d +27° 05′ 49.7″ 4.56 0.45 216 G8III
13 Vul 13 188260 97886 19j 53m 27.68d +24° 04′ 46.3″ 4.57 −0.64 359 B9.5III
15 Vul 15 189849 98543 20j 01m 06.01d +27° 45′ 12.8″ 4.66 0.49 222 A4III
1 Vul 1 180554 94703 19j 16m 13.04d +21° 23′ 25.6″ 4.76 −2.47 911 B4IV
QR Vul 192685 99824 20j 15m 15.89d +25° 35′ 31.1″ 4.79 −3.04 1199 B3V
29 Vul 29 196724 101867 20j 38m 31.29d +21° 12′ 04.2″ 4.81 0.73 213 A0V
12 Vul 12 187811 97679 19j 51m 04.09d +22° 36′ 36.3″ 4.90 −1.49 619 B2.5V V395 Vul[8]
30 Vul 30 197752 102388 20j 44m 52.52d +25° 16′ 15.8″ 4.92 −0.32 365 K2III
9 Vul 9 184606 96275 19j 34m 34.89d +19° 46′ 24.2″ 5.00 −1.35 608 B8IIIn
32 Vul (q)[7] 32 199169 103200 20j 54m 33.64d +28° 03′ 27.5″ 5.03 −1.75 739 K4III
28 Vul 28 196740 101868 20j 38m 31.91d +24° 06′ 57.5″ 5.06 −0.84 493 B5IV
17 Vul 17 190993 99080 20j 06m 53.40d +23° 36′ 51.9″ 5.08 −0.80 488 B3V
4 Vul 4 182762 95498 19j 25m 28.54d +19° 47′ 54.7″ 5.14 0.84 237 K0III
22 Vul 22 192713 99853 20j 15m 30.24d +23° 30′ 32.1″ 5.18 −5.44 4347 G2Ib SB QS Vul[9]
21 Vul 21 192518 99738 20j 14m 14.52d +28° 41′ 41.5″ 5.19 0.18 327 A7IVn
3 Vul 3 182255 95260 19j 22m 50.88d +26° 15′ 44.7″ 5.22 −0.24 402 B6III V377 Vul[10]
16 Vul 16 190004 98636 20j 02m 01.37d +24° 56′ 16.3″ 5.23 1.17 211 F2III
24 Vul 24 192944 99951 20j 16m 47.08d +24° 40′ 16.1″ 5.30 −0.50 472 G8III
33 Vul 33 199697 103511 20j 58m 16.35d +22° 19′ 33.3″ 5.30 −0.13 397 K4III
35 Vul 35 204414 105966 21j 27m 40.03d +27° 36′ 30.8″ 5.39 1.66 182 A1V
2 Vul 2 180968 94827 19j 17m 43.64d +23° 01′ 32.0″ 5.46 −3.39 1918 B0.5IV
10 Vul 10 186486 97077 19j 43m 42.92d +25° 46′ 18.7″ 5.50 0.31 356 G8III
25 Vul 25 193911 100435 20j 22m 03.43d +24° 26′ 46.0″ 5.50 −3.21 1801 B8IIIn
18 Vul 18 191747 99404 20j 10m 33.52d +26° 54′ 14.9″ 5.51 −0.04 420 A3III
19 Vul 19 192004 99518 20j 11m 47.97d +26° 48′ 32.5″ 5.51 −2.96 1614 K3II-III
187982 97765 19j 52m 01.59d +24° 59′ 31.8″ 5.54 −3.15 1781 A1Iab
188485 97961 19j 54m 31.06d +24° 19′ 09.8″ 5.56 −0.25 472 A0III
27 Vul 27 196504 101716 20j 37m 04.66d +26° 27′ 43.1″ 5.59 0.73 305 B9V
5 Vul 5 182919 95560 19j 26m 13.24d +20° 05′ 52.2″ 5.60 1.47 218 A0V
T Vul 198726 102949 20j 51m 28.24d +28° 15′ 01.9″ 5.66 −2.89 1672 F5Ib
203925 105703 21j 24m 33.97d +26° 10′ 28.4″ 5.67 1.53 220 A8III
14 Vul 14 189410 98375 19j 59m 10.58d +23° 06′ 04.6″ 5.68 2.26 158 F0
194577 100754 20j 25m 40.52d +21° 24′ 34.8″ 5.68 −0.43 543 G6III
203803 105652 21j 23m 58.74d +24° 16′ 26.7″ 5.70 1.98 181 F1IV
178187 93845 19j 06m 38.36d +24° 15′ 02.7″ 5.78 0.74 332 A4III
8 Vul 8 183491 95785 19j 28m 57.08d +24° 46′ 07.3″ 5.82 −0.04 484 K0III
182955 95582 19j 26m 28.69d +19° 53′ 29.8″ 5.84 0.12 455 M0III
189944 98609 20j 01m 44.71d +24° 48′ 01.5″ 5.88 −0.69 672 B4V
184010 96016 19j 31m 21.61d +26° 37′ 01.6″ 5.89 2.03 193 K0III-IV
20 Vul 20 192044 99531 20j 12m 00.70d +26° 28′ 43.8″ 5.91 −1.81 1140 B7Ve...
196753 101870 20j 38m 34.99d +23° 40′ 49.8″ 5.91 −3.00 1976 K0II-III+..
187193 97402 19j 47m 48.50d +25° 23′ 02.8″ 6.00 0.56 400 K0II-III
179648 94382 19j 12m 36.72d +21° 33′ 16.4″ 6.02 −1.43 1006 A2Vn
196821 101919 20j 39m 10.63d +21° 49′ 02.7″ 6.08 −1.19 926 A0III
201051 104172 21j 06m 23.45d +26° 55′ 27.9″ 6.13 0.99 348 K0II-III
182807 95492 19j 25m 25.87d +24° 54′ 51.5″ 6.19 3.97 90 F7V
203858 105660 21j 24m 07.42d +25° 18′ 44.6″ 6.20 −0.17 612 A2V
178476 93975 19j 08m 03.49d +21° 41′ 55.5″ 6.22 3.01 143 F3V
191877 99479 20j 11m 21.02d +21° 52′ 29.9″ 6.24 −8.55 29636 B1Ib
193094 100018 20j 17m 31.54d +29° 08′ 51.0″ 6.24 0.98 367 G9III
186518 97091 19j 43m 55.97d +27° 08′ 07.5″ 6.27 −4.35 4347 B7V + G1:III
V0387 Vul[8] 176541 93270 18j 59m 58.12d +22° 48′ 52.2″ 6.28 −0.55 756 M4III
203206 105344 21j 20m 14.07d +22° 01′ 34.2″ 6.29 0.20 539 B6IV
182761 95487 19j 25m 22.40d +20° 16′ 18.4″ 6.31 0.87 400 A0V
184961 96417 19j 36m 08.35d +22° 35′ 08.8″ 6.33 0.11 571 B9sp...
7 Vul 7 183537 95818 19j 29m 20.90d +20° 16′ 47.2″ 6.34 −0.50 760 B5Vn
203886 105689 21j 24m 23.11d +24° 31′ 42.3″ 6.35 0.39 508 K0III
195692 101300 20j 31m 58.19d +25° 48′ 18.1″ 6.37 1.82 264 Am
182422 95340 19j 23m 46.93d +20° 15′ 51.7″ 6.40 −1.30 1132 B9.5V
26 Vul 26 196362 101641 20j 36m 08.32d +25° 52′ 57.4″ 6.40 −0.26 701 A5III
186021 96856 19j 41m 14.65d +22° 27′ 10.0″ 6.43 −1.80 1442 K0Iab:
176971 93443 19j 01m 49.42d +22° 15′ 51.8″ 6.44 0.92 414 A4V
V379 Vul[10] 187640 97572 19j 49m 54.72d +28° 26′ 22.8″ 6.45 −2.13 1698 B5V
190322 98772 20j 03m 38.81d +22° 56′ 27.9″ 6.45 0.46 513 K2
187614 97573 19j 49m 55.81d +27° 05′ 06.6″ 6.46 0.64 475 G8III
189671 98458 20j 00m 15.36d +26° 11′ 16.5″ 6.49 −1.79 1475 G8II
196035 101505 20j 34m 09.98d +20° 59′ 06.7″ 6.49 −1.79 1475 B3IV
185436 96601 19j 38m 17.79d +20° 47′ 00.5″ 6.50 0.28 572 K0III
190066 98661 20j 02m 22.11d +22° 09′ 05.4″ 6.50 −3.75 3663 B1Iab
BW Vul 199140 103191 20j 54m 22.39d +28° 31′ 19.2″ 6.55 −2.13 1772 B2IIIvar
HD 190228 190228 98714 20j 03m 00.77d +28° 18′ 24.7″ 7.31 3.34 203 G5IV memiliki planit (b)
HD 189733 189733 98505 20j 00m 43.71d +22° 42′ 39.1″ 7.68 6.26 62.9 K1-K2 memiliki planit (b)
HD 188015 188015 97769 19j 52m 04.54d +28° 06′ 01.4″ 8.22 4.61 172 G5IV memiliki planit (b)
PY Vul 19j 37m 13.17d +27° 43′ 18.1″ 12.97 DA bintang katai putih
Gliese 1235 19j 21m 38.68d +20° 52′ 03.1″ 13.38 33.13 M4.5 Proxima Vulpeculae[11]
PSR B1919+21 19j 21m 44.81d +21° 53′ 02.3″ 2283

Uga delengen

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Rujukan

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  • ESA (1997). "The Hipparcos and Tycho Catalogues". Diarsip saka sing asli ing 2003-05-28. Dibukak ing 2013-02-10.
  • Kostjuk, N. D. (2002). "HD-DM-GC-HR-HIP-Bayer-Flamsteed Cross Index". Diarsip saka sing asli ing 2005-10-26. Dibukak ing 2013-02-10.
  • Roman, N. G. (1987). "Identification of a Constellation from a Position". Diarsip saka sing asli ing 2006-11-24. Dibukak ing 2013-02-10.
  1. ↑ Vulpecula page at SEDS (Students for the Exploration and Development of Space)
  2. ↑ Hewish, A.; Bell, S. J.; Pilkington, J. D. H.; Scott, P. F.; Collins, R. A. (1968). "Observation of a Rapidly Pulsating Radio Source". Nature. 217 (5130): 709–713. Bibcode:1968Natur.217..709H. doi:10.1038/217709a0. Dibukak ing 2007-07-06.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  3. ↑ [1] Archived 2012-03-06 at the Wayback Machine. (dipunundhuh tanggal 12 Pebruari 2013)
  4. ↑ Wagman, Morton (2003) Lost Stars, McDonald and Woodward, Blacksburg, Virginia, p.494. ISBN 0-939923-78-5.
  5. ↑ Samus, General Catalogue of Variable Stars, Vol. I-III (version 2008-Dec) - database entry: V* CK Vul.
  6. ↑ D. Hoffleit and W. H. Warren, Jr., The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version) - database entry: HR 7405.
  7. ↑ a b In Flamsteed's star catalogue and atlases.
    Map of constellations Lyra, Cygnus, Lacerta, Vulpec, Anser, and Sagitta. - Flamsteed, John. 1729. Atlas coelestis Archived 2011-07-27 at the Wayback Machine.: Linda Hall Library.
  8. ↑ a b N.N. Samus, et al., General Catalogue of Variable Stars (Samus+ 2007-2009), 2009yCat....102025S
  9. ↑ http://articles.adsabs.harvard.edu//full/1985IBVS.2681....1K/0000014.000.html?high=4c1e33745313663
  10. ↑ a b http://articles.adsabs.harvard.edu//full/1997IBVS.4471....1K/0000016.000.html?high=4c565f05dc10973
  11. ↑ "Archive copy". Diarsip saka sing asli ing 2010-06-12. Dibukak ing 2013-02-10.{{cite web}}: CS1 maint: archived copy as title (link)
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