Xi Draconis: Perbedaan antara revisi

Xi Draconis
Data pengamatan; Epos J2000 Ekuinoks J2000
Rasi bintang	Draco
Asensio rekta	17j 53m 31.72962d
Deklinasi	+56° 52′ 21.5143″
Magnitudo tampak (V)	3.75
Ciri-ciri
Kelas spektrum	K2 III
Indeks warna U−B	+1.21
Indeks warna B−V	+1.18
Astrometri
Kecepatan radial (Rv)	-26.38 ± 0.20 km/s
Gerak diri (μ)	RA: 93.82 ± 0.14 mdb/thn ; Dek.: 78.50 ± 0.12 mdb/thn
Paralaks (π)	28,98±0,12 mdb
Jarak	112,5 ± 0,5 tc ; (34,5 ± 0,1 pc)
Magnitudo mutlak (MV)	+1.06
Detail
Massa	1.45 ± 0.17 M☉
Radius	12 R☉
Luminositas	49 ± 4 L☉
Gravitasi permukaan (log g)	2.3
Suhu	4,445 K
Metalisitas [Fe/H]	–0.09
Kecepatan rotasi (v sin i)	2.3 km/s
Penamaan lain
	32 Dra, BD+56 2033, FK5 671, HD 163588, HIP 87585, HR 6688, SAO 30631, WDS 17535+5652.
Referensi basis data
SIMBAD	data

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Revisi terkini sejak 18 Desember 2022 12.28

Xi Draconis (ξ Dra / ξ Draconis) adalah salah satu bintang di rasi Draco. Xi Draconis memiliki magnitudo 3.75 dan termasuk pada kelas K2-III. Bintang ini berada pada 111 tahun cahaya dari Bumi.

Etimologi

Bintang ini kadang-kadang disebut juga Grumium yang berarti "rahang sang naga" dalam bahasa Latin dan Nodus Primus yang berarti "ikatan pertama" dalam bahasa Latin. Nama lainnya untuk bintang ini adalah:

nama lain	asal bahasa	arti
天棓一 / Tiānbàngyī	China	bintang pertama pada rasi Alat Pemukul Padi di Langit^[8]

Selain rasi Draco, bintang ini juga merupakan anggota dari berbagai rasi atau asterisma berikut:

nama rasi / asterisma	asal	arti	anggota lainnya
天棓 / Tiānbàng	China	Alat Pemukul Padi di Langit	γ Dra, ν Dra, β Dra, ι Her
Lozenge^[9]		belah ketupat	γ Dra, ν Dra, β Dra
Alwaid	Arab	induk unta	γ Dra, ν Dra, β Dra, μ Dra^[10]^[11]
Al Ṣalīb al Wākiʽ^[10]	Arab	salib yang terbalik	γ Dra, ν Dra, β Dra, μ Dra

Referensi

^ ^a ^b ^c ^d ^e van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752 , Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.
^ ^a ^b ^c Jennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants.", Monthly Notices of the Royal Astronomical Society, 172: 667–679, Bibcode:1975MNRAS.172..667J, doi:10.1093/mnras/172.3.667.
^ Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics, 11: 29–50, Bibcode:1973ARA&A..11...29M, doi:10.1146/annurev.aa.11.090173.000333.
^ Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics, 430 (1): 165–186, arXiv:astro-ph/0409579 , Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272.
^ Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars", Astronomy and Astrophysics, 430: 303–311, arXiv:astro-ph/0409683 , Bibcode:2005A&A...430..303C, doi:10.1051/0004-6361:20041440.
^ ^a ^b ^c Stello, D.; et al. (2008), "Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses", The Astrophysical Journal Letters, 674 (1): L53–L56, arXiv:0801.2155 , Bibcode:2008ApJ...674L..53S, doi:10.1086/528936.
^ ^a ^b ^c ^d Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209.
^ salah satu rasi bintang menurut bangsa Cina
^ "Salinan arsip". Diarsipkan dari versi asli tanggal 1999-02-02. Diakses tanggal 2009-08-14.
^ ^a ^b http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html
^ asterisma ini disebut juga Quinque Dromedarii

Artikel bertopik bintang ini adalah sebuah rintisan. Anda dapat membantu Wikipedia dengan mengembangkannya.

[aaa474_2_653-1] van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, arXiv:0708.1752 , Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357.

[mnras172_667-2] Jennens, P. A.; Helfer, H. L. (September 1975), "A new photometric metal abundance and luminosity calibration for field G and K giants.", Monthly Notices of the Royal Astronomical Society, 172: 667–679, Bibcode:1975MNRAS.172..667J, doi:10.1093/mnras/172.3.667.

[araa11_29-3] Morgan, W. W.; Keenan, P. C. (1973), "Spectral Classification", Annual Review of Astronomy and Astrophysics, 11: 29–50, Bibcode:1973ARA&A..11...29M, doi:10.1146/annurev.aa.11.090173.000333.

[aaa430_165-4] Famaey, B.; et al. (January 2005), "Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters", Astronomy and Astrophysics, 430 (1): 165–186, arXiv:astro-ph/0409579 , Bibcode:2005A&A...430..165F, doi:10.1051/0004-6361:20041272.

[Cardini2005-5] Cardini, D. (January 2005), "Mg II chromospheric radiative loss rates in cool active and quiet stars", Astronomy and Astrophysics, 430: 303–311, arXiv:astro-ph/0409683 , Bibcode:2005A&A...430..303C, doi:10.1051/0004-6361:20041440.

[apjl674_1_L53-6] Stello, D.; et al. (2008), "Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses", The Astrophysical Journal Letters, 674 (1): L53–L56, arXiv:0801.2155 , Bibcode:2008ApJ...674L..53S, doi:10.1086/528936.

[aj135_1_209-7] Massarotti, Alessandro; et al. (January 2008), "Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity", The Astronomical Journal, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209.

[sb0-8] salah satu rasi bintang menurut bangsa Cina

[9] "Salinan arsip". Diarsipkan dari versi asli tanggal 1999-02-02. Diakses tanggal 2009-08-14.

[penelope.uchicago.edu-10] ttp://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html

[11] sterisma ini disebut juga Quinque Dromedarii

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

@@ Baris 1: / Baris 1: @@
+{{Starbox begin
+| name = Xi Draconis
+}}
+{{Starbox observe
+| epoch        = J2000
+| constell     = [[Draco (constellation)|Draco]]
+| ra           = {{RA|17|53|31.72962}}<ref name=aaa474_2_653/>
+| dec          = {{DEC|+56|52|21.5143}}<ref name=aaa474_2_653/>
+| appmag_v     = 3.75<ref name=mnras172_667/>
+}}
+{{Starbox character
+| class        = K2&nbsp;III<ref name=araa11_29/>
+| b-v          = +1.18<ref name=mnras172_667/>
+| u-b          = +1.21<ref name=mnras172_667/>
+| variable     =
+}}
+{{Starbox astrometry
+ | radial_v    = -26.38 ± 0.20<ref name=aaa430_165/>
+ | prop_mo_ra  = {{nowrap|93.82 ± 0.14}}<ref name=aaa474_2_653/>
+ | prop_mo_dec = {{nowrap|78.50 ± 0.12}}<ref name=aaa474_2_653/>
+ | parallax    = 28.98
+ | p_error     = 0.12
+ | parallax_footnote = <ref name=aaa474_2_653/>
+ | absmag_v    = +1.06<ref name=Cardini2005/>
+}}
+{{Starbox detail
+ | mass        = 1.45 ± 0.17<ref name=apjl674_1_L53/>
+ | radius      = 12<ref name=aj135_1_209/>
+ | luminosity  = 49 ± 4<ref name=apjl674_1_L53/>
+ | temperature = 4,445<ref name=apjl674_1_L53/>
+ | gravity     = 2.3<ref name=aj135_1_209/>
+ | metal_fe    = –0.09<ref name=aj135_1_209/>
+ | rotational_velocity = 2.3<ref name=aj135_1_209/>
+}}
+{{Starbox catalog
+| names = 32&nbsp;Dra, BD+56&nbsp;2033, [[FK5]]&nbsp;671, [[Henry Draper catalogue|HD]]&nbsp;163588, [[Hipparcos catalogue|HIP]]&nbsp;87585, [[Star catalogue#BS, BSC, HR|HR]]&nbsp;6688, [[Star catalogue#SAO|SAO]]&nbsp;30631, [[Washington Double Star Catalog|WDS]] 17535+5652.
+}}
+{{Starbox reference
+|Simbad=ksi+Dra
+}}
+{{Starbox end}}
 '''Xi Draconis (ξ Dra / ξ Draconis)''' adalah salah satu bintang di rasi [[Draco (constellation)|Draco]]. Xi Draconis memiliki magnitudo 3.75 dan termasuk pada kelas K2-III. Bintang ini berada pada 111 [[tahun cahaya]] dari [[Bumi]].
 == Etimologi ==
-Bintang ini kadang-kadang disebut juga '''Grumium''' yang berarti "rahang sang naga" dalam bahasa [[Latin]] dan '''Nodus Primus''' yang berarti "ikatan pertama" dalam bahasa [[Latin]]. Nama lainnya untuk bintang ini adalah :
+Bintang ini kadang-kadang disebut juga '''Grumium''' yang berarti "rahang sang naga" dalam [[bahasa Latin]] dan '''Nodus Primus''' yang berarti "ikatan pertama" dalam [[bahasa Latin]]. Nama lainnya untuk bintang ini adalah:
 {| class="wikitable"
@@ Baris 13: / Baris 54: @@
 |天棓一 / Tiānbàngyī||[[China]] ||bintang pertama pada rasi [[Daftar asterisme di Batasan Ungu yang Terlarang#Alat Pemukul Padi di Langit|Alat Pemukul Padi di Langit]]<ref name=sb0>salah satu rasi bintang menurut bangsa Cina</ref>
 |}
-Selain [[rasi]] [[Draco]], bintang ini juga merupakan anggota dari berbagai rasi atau asterisma berikut :
+Selain [[rasi]] [[Draco]], bintang ini juga merupakan anggota dari berbagai rasi atau asterisma berikut:
 {| class="wikitable"
@@ Baris 24: / Baris 65: @@
 | 天棓 / Tiānbàng || [[China]] || [[Daftar asterisme di Batasan Ungu yang Terlarang#Alat Pemukul Padi di Langit|Alat Pemukul Padi di Langit]]||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]], [[Iota Herculis|ι Her]]
 |-
-| Lozenge<ref>http://seds.org/Maps/Const/asterism.html</ref>||  ||belah ketupat||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]]
+| Lozenge<ref>{{Cite web |url=http://seds.org/Maps/Const/asterism.html |title=Salinan arsip |access-date=2009-08-14 |archive-date=1999-02-02 |archive-url=https://web.archive.org/web/19990202143049/http://seds.org/Maps/Const/asterism.html |dead-url=no }}</ref>||  ||belah ketupat||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]]
 |-
-| Alwaid|| [[Arab]] ||induk unta||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]], [[Mu Draconis|μ Dra A]]<ref>http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html</ref><ref>asterisma ini disebut juga ''Quinque Dromedarii''</ref>
+| Alwaid|| [[Bahasa Arab|Arab]] ||induk unta||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]], [[Mu Draconis|μ Dra]]<ref name="penelope.uchicago.edu">http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html</ref><ref>asterisma ini disebut juga ''Quinque Dromedarii''</ref>
 |-
-| Al Ṣalīb al Wākiʽ<ref>http://penelope.uchicago.edu/Thayer/E/Gazetteer/Topics/astronomy/_Texts/secondary/ALLSTA/Draco*.html</ref>|| [[Arab]] ||salib yang terbalik||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]], [[Mu Draconis|μ Dra A]]
+| Al Ṣalīb al Wākiʽ<ref name="penelope.uchicago.edu"/>|| [[Bahasa Arab|Arab]] ||salib yang terbalik||[[Gamma Draconis|γ Dra]], [[Nu Draconis|ν Dra]], [[Beta Draconis|β Dra]], [[Mu Draconis|μ Dra]]
 |}
 == Referensi ==
-{{reflist}}
+{{reflist|refs=
+<ref name=aaa474_2_653>{{citation | first=F. | last=van Leeuwen |date=November 2007 | title=Validation of the new Hipparcos reduction | journal=Astronomy and Astrophysics | volume=474 | issue=2 | pages=653–664 | bibcode=2007A&A...474..653V | doi=10.1051/0004-6361:20078357 | postscript=. |arxiv = 0708.1752 }}</ref>
-{{astronomi-stub}}
+<ref name=Cardini2005>{{citation
+ | title=Mg II chromospheric radiative loss rates in cool active and quiet stars
+ | last1=Cardini | first1=D. | postscript=.
+ | journal=Astronomy and Astrophysics
+ | volume=430 | pages=303-311 | date=January 2005
+ | doi=10.1051/0004-6361:20041440 | bibcode=2005A&A...430..303C |arxiv = astro-ph/0409683 }}</ref>
+<ref name=apjl674_1_L53>{{citation | display-authors=1 | last1=Stello | first1=D. | last2=Bruntt | first2=H. | last3=Preston | first3=H. | last4=Buzasi | first4=D. | title=Oscillating K Giants with the WIRE Satellite: Determination of Their Asteroseismic Masses | journal=The [[Astrophysical Journal]] Letters | volume=674 | issue=1 | year=2008 | pages=L53–L56 | doi=10.1086/528936 | bibcode=2008ApJ...674L..53S | postscript=. |arxiv = 0801.2155 }}</ref>
+<ref name=aj135_1_209>{{citation | display-authors=1 | last1=Massarotti | first1=Alessandro | last2=Latham | first2=David W. | last3=Stefanik | first3=Robert P. | last4=Fogel | first4=Jeffrey | title=Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity | journal=The Astronomical Journal | volume=135 | issue=1 | pages=209–231 |date=January 2008 | doi=10.1088/0004-6256/135/1/209 | bibcode=2008AJ....135..209M | postscript=. }}</ref>
+<ref name=aaa430_165>{{citation | display-authors=1 | last1=Famaey | first1=B. | last2=Jorissen | first2=A. | last3=Luri | first3=X. | last4=Mayor | first4=M. | last5=Udry | first5=S. | last6=Dejonghe | first6=H. | last7=Turon | first7=C. | title=Local kinematics of K and M giants from CORAVEL/Hipparcos/Tycho-2 data. Revisiting the concept of superclusters | journal=Astronomy and Astrophysics | volume=430 | issue=1 | pages=165–186 |date=January 2005 | doi=10.1051/0004-6361:20041272 | bibcode=2005A&A...430..165F |arxiv = astro-ph/0409579 | postscript=. }}</ref>
+<ref name=mnras172_667>{{citation | last1=Jennens | first1=P. A. | last2=Helfer | first2=H. L. | title=A new photometric metal abundance and luminosity calibration for field G and K giants. | journal=[[Monthly Notices of the Royal Astronomical Society]] | volume=172 | pages=667–679 |date=September 1975 | bibcode=1975MNRAS.172..667J | postscript=. | doi=10.1093/mnras/172.3.667}}</ref>
+<ref name=araa11_29>{{citation | last1=Morgan | first1=W. W. | last2=Keenan | first2=P. C. | title=Spectral Classification | journal=Annual Review of Astronomy and Astrophysics | volume=11 | pages=29–50 | year=1973 | doi=10.1146/annurev.aa.11.090173.000333 | bibcode=1973ARA&A..11...29M | postscript=. }}</ref>
+}}
 [[Kategori:Rasi bintang Draco]]
-[[de:Grumium]]
+{{bintang-stub}}
-[[en:Xi Draconis]]
-[[es:Grumium]]
-[[fr:Xi Draconis]]
-[[lb:Grumium (Stär)]]
-[[nl:Grumium]]
-[[pt:Xi Draconis]]
-[[sk:Grumium]]

Data pengamatan Epos J2000 Ekuinoks J2000
Rasi bintang	Draco
Asensio rekta	17^j 53^m 31.72962^d^[1]
Deklinasi	+56° 52′ 21.5143″^[1]
Magnitudo tampak (V)	3.75^[2]
Ciri-ciri
Kelas spektrum	K2 III^[3]
Indeks warna U−B	+1.21^[2]
Indeks warna B−V	+1.18^[2]
Astrometri

Kecepatan radial (R_v)	-26.38 ± 0.20^[4] km/s
Gerak diri (μ)	RA: 93.82 ± 0.14^[1] mdb/thn Dek.: 78.50 ± 0.12^[1] mdb/thn
Paralaks (π)	28,98±0,12^[1] mdb
Jarak	112,5 ± 0,5 tc (34,5 ± 0,1 pc)
Magnitudo mutlak (M_V)	+1.06^[5]

Detail

Massa	1.45 ± 0.17^[6] M_☉
Radius	12^[7] R_☉
Luminositas	49 ± 4^[6] L_☉
Gravitasi permukaan (log g)	2.3^[7]
Suhu	4,445^[6] K
Metalisitas [Fe/H]	–0.09^[7]
Kecepatan rotasi (v sin i)	2.3^[7] km/s

Penamaan lain
32 Dra, BD+56 2033, FK5 671, HD 163588, HIP 87585, HR 6688, SAO 30631, WDS 17535+5652.
Referensi basis data
SIMBAD	data