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{{about-distinguish|e Aquilae|epsilon Aquilae{{!}}ε Aquilae}}{{Starbox begin | name = 36 Aquilae }}{{Starbox image | image = | caption = Location of 36 Aquarii (circled) }}{{Starbox observe | epoch = J2000 | ra = {{RA|19|30|39.83606}} | dec = {{DEC|–02|47|19.9944}} | appmag_v = 5.02[3] | constell = Aquila }}{{Starbox character | class = M1 III[4] | r-i = | v-r = | b-v = +1.75[3] | u-b = +2.03[3] | variable = }}{{Starbox astrometry | radial_v = {{nowrap|–10.38 ± 0.55}}[7] | prop_mo_ra = +20.64 | prop_mo_dec = –10.63 | parallax = 6.17 | p_error = 0.30 | parallax_footnote = | absmag_v = }}{{Starbox detail | mass = | radius = 54[11] | luminosity = | temperature = | metal_fe = | rotational_velocity = | age_myr = }}{{Starbox catalog | names = BD–03° 4612, FK5 1509, HD 183630, HIP 95937, HR 7414, SAO 143482.[4] }}{{Starbox reference |Simbad=36+Aql }}{{Starbox end}}36 Aquilae (abbreviated 36 Aql) is a star in the equatorial constellation of Aquila. 36 Aquilae is its Flamsteed designation though it also bears the Bayer designation e Aquilae. With an apparent visual magnitude of 5.02,[3] this star is faintly visible to the naked eye. It has an annual parallax shift of 6.17 mas, indicating a physical distance of {{Convert|530|ly|pc|abbr=off|lk=on}} with a 30 light-year margin of error.The spectrum of this star matches a stellar classification of M1 III.[4] It is a red giant star with 54[11] times the radius of the Sun that is currently on the asymptotic giant branch.[17] This means the star is generating energy by the fusion of hydrogen along an outer shell and helium along a concentric inner shell, surrounding an inert core of carbon and oxygen. 36 Aquilae undergoes small, periodic variations in luminosity, changing by 0.0063 magnitudes about 11.5 times per day, or once every 2 hours and 5.2 minutes.[18] References1. ^1 {{citation | display-authors=1 | last1=Famaey | first1=B. | last2=Pourbaix | first2=D. | last3=Frankowski | first3=A. | last4=van Eck | first4=S. | last5=Mayor | first5=M. | last6=Udry | first6=S. | last7=Jorissen | first7=A. | title=Spectroscopic binaries among Hipparcos M giants. I. Data, orbits, and intrinsic variations | journal=Astronomy and Astrophysics | volume=498 | issue=2 | pages=627–640 | doi=10.1051/0004-6361/200810698 | bibcode=2009A&A...498..627F | postscript=. |arxiv = 0901.0934 |date=May 2009}} 2. ^1 2 3 4 {{citation | last1=Cousins | first1=A. W. J. | title=Photometric Data for Stars in the Equatorial Zone (Seventh List) | journal=Monthly Notes of the Astronomical Society of Southern Africa | volume=23 | page=175 | year=1964 | bibcode=1964MNSSA..23..175C | postscript=. }} 3. ^1 {{citation | last1=Koen | first1=Chris | last2=Eyer | first2=Laurent | title=New periodic variables from the Hipparcos epoch photometry | journal=Monthly Notices of the Royal Astronomical Society | volume=331 | issue=1 | pages=45–59 | doi=10.1046/j.1365-8711.2002.05150.x | bibcode=2002MNRAS.331...45K | arxiv=astro-ph/0112194 | postscript=. |date=March 2002}} 4. ^1 2 {{citation | display-authors=1 | last1=Pasinetti Fracassini | first1=L. E. | last2=Pastori | first2=L. | last3=Covino | first3=S. | last4=Pozzi | first4=A. | title=Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS) - Third edition - Comments and statistics | journal=Astronomy and Astrophysics | volume=367 | issue=2 | pages=521–524 | doi=10.1051/0004-6361:20000451 | bibcode=2001A&A...367..521P | arxiv=astro-ph/0012289 | postscript=. |date=February 2001}} 5. ^1 {{citation | last1=Eggen | first1=Olin J. | title=Asymptotic giant branch stars near the sun | journal=Astronomical Journal | volume=104 | issue=1 | pages=275–313 | doi=10.1086/116239 | bibcode=1992AJ....104..275E | postscript=. |date=July 1992}} 6. ^1 2 3 {{cite simbad | title=* e Aql | accessdate=2012-07-22 | postscript=. }}
[1][2][3][4][5][6] }}External links{{Stars of Aquila}} 9 : Bayer objects|Flamsteed objects|Henry Draper Catalogue objects|Aquila (constellation)|Hipparcos objects|M-type giants|HR objects|Durchmusterung objects|Suspected variables |