99 Aquarii: Difference between revisions

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{{Starbox begin
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| name = 15 Arietis
}}
{{Starbox observe
| epoch      = J2000
| ra          = {{RA|02|10|37.59642}}<ref name=aaa474_2_653/>
| dec        = {{DEC|+19|30|01.2099}}<ref name=aaa474_2_653/>
| appmag_v    = 5.74<ref name=mnras389_2_869/>
| constell    = [[Aries (constellation)|Aries]]
}}
{{Starbox character
| class      = M3&nbsp;III<ref name=mnras400_4_1945/>
| r-i        =
| v-r        =
| b-v        = +1.64<ref name=SIMBAD/>
| u-b        = +1.91<ref name=SIMBAD/>
| variable    = Pulsating
}}
{{Starbox astrometry
| radial_v    = {{nowrap|+62.04 ± 0.22}}<ref name=aaa430_165/>
| prop_mo_ra  = +87.88<ref name=aaa474_2_653/>
| prop_mo_dec = -27.82<ref name=aaa474_2_653/>
| parallax    = 5.84
| p_error    = 0.49
| parallax_footnote = <ref name=aaa474_2_653/>
| absmag_v    =
}}
{{Starbox detail
| mass        =
| radius      = 67<ref name=lang2006/>
| luminosity  =
| temperature =
| metal_fe    =
| rotational_velocity =
| age_myr    =
}}
{{Starbox catalog
| names = AV Arietis, [[Durchmusterung|BD]]+18 277, [[FK5]] 1056, [[Henry Draper Catalogue|HD]] 13325, [[Hipparcos Catalogue|HIP]] 10155, [[Bright Star Catalogue|HR]] 631, [[Smithsonian Astrophysical Observatory Star Catalog|SAO]] 92822.<ref name=SIMBAD/>
}}
{{Starbox end}}
 
'''15 Arietis''' is the [[Flamsteed designation]] for a single<ref name=mnras389_2_869/> [[star]] in the northern [[constellation]] of [[Aries (constellation)|Aries]]. It has an [[apparent visual magnitude]] of 5.74,<ref name=mnras389_2_869/> which is just bright enough to be visible to the naked eye from [[Bortle Dark-Sky Scale|dark suburban skies]]. An annual [[parallax]] shift of 5.84&nbsp;[[milliarcsecond|mas]]<ref name=aaa474_2_653/> corresponds to a physical distance of approximately {{Convert|560|ly|pc|abbr=off|lk=on}} from Earth. At that distance, the star's brightness is reduced by 0.33<ref name=aaa430_165/> in magnitude because of [[extinction (astronomy)|extinction]] from [[interstellar medium|interstellar gas and dust]].
 
This is a [[red giant]] star with a [[stellar classification]] of M3&nbsp;III.<ref name=mnras400_4_1945/> The measured [[angular diameter]] of this star is {{nowrap|3.67 ± 0.11 mas}}.<ref name=aaa431_773/> At the estimated distance of Delta Ophiuchi,<ref name=aaa474_2_653/> this yields a physical size of about 67 times the [[Solar radius|radius of the Sun]].<ref name=lang2006/> It is a [[pulsating variable]] star with the [[variable star designation]] AV Arietis. The first pulsation period is 18.1 days with an amplitude of 0.028 magnitudes, while the second is 21.9 days and 0.030 in magnitude.<ref name=mnras400_4_1945/>
 
==References==
{{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 | arxiv=0708.1752 | 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=mnras400_4_1945>{{citation | display-authors=1 | last1=Tabur | first1=V. | last2=Bedding | first2=T. R. | last3=Kiss | first3=L. L. | last4=Moon | first4=T. T. | last5=Szeidl | first5=B. | last6=Kjeldsen | first6=H. | title=Long-term photometry and periods for 261 nearby pulsating M giants | journal=Monthly Notices of the Royal Astronomical Society | volume=400 | issue=4 | pages=1945–1961  | doi=10.1111/j.1365-2966.2009.15588.x | bibcode=2009MNRAS.400.1945T | postscript=. |arxiv = 0908.3228  |date=December  2009}}</ref>
 
<ref name=mnras389_2_869>{{citation | last1=Eggleton | first1=P. P. | last2=Tokovinin | first2=A. A. | title=A catalogue of multiplicity among bright stellar systems | journal=Monthly Notices of the Royal Astronomical Society | volume=389 | issue=2 | pages=869–879  | doi=10.1111/j.1365-2966.2008.13596.x | bibcode=2008MNRAS.389..869E | arxiv=0806.2878 | postscript=.  |date=September  2008}}</ref>
 
<ref name=aaa431_773>{{citation | last1=Richichi | pages=A. | last2=Percheron | first2=I. | last3=Khristoforova | first3=M. | title=CHARM2: An updated Catalog of High Angular Resolution Measurements | journal=Astronomy and Astrophysics | volume=431 | pages=773–777  | doi=10.1051/0004-6361:20042039 | bibcode=2005A&A...431..773R | postscript=.  |date=February  2005}}</ref>
 
<ref name=lang2006>{{citation | first1=Kenneth R. | last1=Lang | title=Astrophysical formulae | volume=1 | series=Astronomy and astrophysics library | edition=3 | publisher=Birkhäuser | year=2006 | isbn=3-540-29692-1 | url=http://books.google.com/books?id=OvTjLcQ4MCQC&pg=PA41 | postscript=. }}. The radius (R<sub>*</sub>) is given by:
:<math>\begin{align} 2\cdot R_*
& = \frac{(170\cdot 3.67\cdot 10^{-3})\ \text{AU}}{0.0046491\ \text{AU}/R_{\bigodot}} \\
& \approx 134\cdot R_{\bigodot}
\end{align}</math></ref>
 
<ref name=SIMBAD>{{citation | title=AV Ari -- Semi-regular pulsating Star | work=SIMBAD Astronomical Database | publisher=Centre de Données astronomiques de Strasbourg | url=http://simbad.u-strasbg.fr/simbad/sim-id?Ident=15+Arietis | accessdate=2012-07-18 | postscript=. }}</ref>
 
}}
 
==External links==
* [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%20631 HR 631]
* [http://aladin.u-strasbg.fr/AladinPreview?-c=02+10+37.6%2B19+30+01&ident=V*+AV+Ari&submit=Aladin+previewer Image 15 Arietis]
 
{{Stars of Aries}}
 
[[Category:Henry Draper Catalogue objects|13325]]
[[Category:Hipparcos objects|010155]]
[[Category:Flamsteed objects|Arietis, 15]]
[[Category:Aries (constellation)]]
[[Category:M-type main-sequence stars]]

Latest revision as of 15:53, 23 December 2014

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