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词条 53 Aquarii
释义

  1. References

{{Starbox begin
| name = 53 Aquarii
}}{{Starbox image
| image =

| caption = Location of 53 Aquarii (circled)
}}{{Starbox observe
| epoch = J2000
| ra = {{RA|22|26|34.2753}}
| dec = {{DEC|–16|44|31.697}}
| appmag_v = 5.56[3] (6.35/6.57)[4]
| constell = Aquarius
}}{{Starbox character
| class = {{nowrap|G1 V + G5 V Fe–0.8 CH–1}}[5]
| b-v = +0.61[3]
| u-b = +0.09[3]
| variable =
}}{{Starbox astrometry
| radial_v = +2.1[8]
| prop_mo_ra = +200.59
| prop_mo_dec = +14.51
| parallax = 49.50
| p_error = 1.23
| parallax_footnote =
| absmag_v = 4.05[8] (4.94/4.87)[4]
}}{{Starbox orbit
| reference = [1]
| primary = 53 Aqr A
| name = 53 Aqr B
| period = 3500
| axis = 14.88
| eccentricity = 0.90
| inclination = 44.13
| node = 294.55
| periastron = B 2023
| periarg = 151.40
}}{{Starbox detail
| component1 = 53 Aqr A
| mass = 1.01[2]
| radius = 1.11[16]
| luminosity = 1.39[16]
| temperature = 5,922[4]
| metal_fe = –0.10[4]
| gravity = 4.46[4]
| rotational_velocity = 8[21]
| age_gyr = 0.18–0.37[22]
| component2 = 53 Aqr B
| mass2 =0.99[2]
| temperature2= 5,811[4]
| metal2_fe = –0.19[4]
| gravity2 = 4.44[4]
| rotational_velocity2 = 9[21]
}}{{Starbox catalog
| names = GJ 859, HIP 110778.[28]
| component1 = 53 Aqr A
| names1 = BD–17 6521, HD 212698, HR 8545, LTT 9026, SAO 165078.
| component2 = 53 Aqr B
| names2 = BD–17 6520, HD 212697, HR 8544, LTT 9025, SAO 165077.
}}{{Starbox reference
| Simbad = 53+Aqr | sn=53 Aqr
| Simbad2 = 53+Aqr+A | sn2=53 Aqr A
| Simbad3 = 53+Aqr+B | sn3=53 Aqr B
}}{{Starbox end}}53 Aquarii (abbreviated 53 Aqr) is a binary star[29] system in the equatorial constellation of Aquarius. 53 Aquarii is its Flamsteed designation though the star also bears the Bayer designation of f Aquarii. The combined apparent visual magnitude of the pair is a 5.56,[3] making it just visible to the naked eye in dark suburban skies. Based upon an annual parallax shift of 49.50 milliarcseconds for the first component, this system is located at a distance of approximately {{Convert|65|ly|pc|abbr=off|lk=on}} from Earth.

This is a wide binary star system with a projected separation of 100 astronomical units; indicating that the two stars are at least this distance apart.[16] The primary component is a solar-type main sequence star with a stellar classification of G1 V.[5] It has about 99% of the Sun's mass, 111% of the Sun's radius, and shines with 139% of the luminosity of the Sun.[16] This energy is being emitted from an outer envelope at an effective temperature of 5,922 K,[4] giving it the golden hue of a G-type star.[36] An examination of the primary component with the Spitzer space telescope failed to detect any infrared excess that might otherwise be an indication of a circumstellar debris disk.[16]

The companion is a slightly cooler star with an effective temperature of 5,811 K.[4] It has a stellar classification of G5 V Fe–0.8 CH–1,[5] indicating it is a chemically peculiar G-type main sequence star showing an under-abundance of iron and the molecule CH in its spectrum. As of 2008, it has an angular separation of 1.325 arcseconds along a position angle of 30.9° from the primary.[40]

This system is coeval with the Castor Moving Group of stars that share a common motion through space; hence it is a candidate member of that association. This suggests that the system is young; its estimated age is in the range of 180 to 370 million years, based upon the spectrum and X-ray luminosity, respectively.[22]

References

1. ^{{cite web|url=http://www.usno.navy.mil/USNO/astrometry/optical-IR-prod/wds/orb6|title=Sixth Catalog of Orbits of Visual Binary Stars|publisher=United States Naval Observatory|accessdate=3 June 2017}}
2. ^{{cite journal|author1=Cvetkovic, Z. |author2=Ninkovic, S. |date=2010|title=On the Component Masses of Visual Binaries|journal=Serbian Astronomical Journal|volume=180|pages=71–80|doi=10.2298/SAJ1080071C | bibcode =2010SerAJ.180...71C}}
3. ^10 {{citation | last1=Pasquini | first1=L. | last2=Liu | first2=Q. | last3=Pallavicini | first3=R. | title=Lithium abundances of nearby solar-like stars | journal=Astronomy and Astrophysics | volume=287 | issue=1 | pages=191–205 | bibcode=1994A&A...287..191P | postscript=. |date=July 1994}}
4. ^{{citation | display-authors=1 | last1=Gray | first1=R. O. | first2=C. J. | last2=Corbally | first3=R. F. | last3=Garrison | first4=M. T. | last4=McFadden | first5=P. E. | last5=Robinson | title=Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I | journal=The Astronomical Journal | volume=132 | issue=1 | pages=161–170 |date=July 2006 | doi=10.1086/504637 | bibcode=2006AJ....132..161G | arxiv=astro-ph/0603770 | postscript=. }}
5. ^{{citation | title=The Geneva-Copenhagen survey of the Solar neighbourhood. Ages, metallicities, and kinematic properties of ˜14 000 F and G dwarfs | display-authors=1 | last1=Nordström | first1=B. | last2=Mayor | first2=M. | last3=Andersen | first3=J. | last4=Holmberg | first4=J. | last5=Pont | first5=F. | last6=Jørgensen | first6=B. R. | last7=Olsen | first7=E. H. | last8=Udry | first8=S. | last9=Mowlavi | first9=N. | journal=Astronomy and Astrophysics | volume=418 | pages=989–1019 | doi=10.1051/0004-6361:20035959 | bibcode=2004A&A...418..989N | arxiv=astro-ph/0405198 | postscript=. |date=May 2004}}
6. ^{{citation | last1=Nicolet | first1=B. | year=1978 | title=Photoelectric photometric Catalogue of homogeneous measurements in the UBV System | journal=Astronomy and Astrophysics Supplement Series | volume=34 | pages=1–49 | bibcode=1978A&AS...34....1N | postscript=. }}
7. ^{{citation | display-authors=1 | last1=Torres | first1=C. A. O. | last2=Quast | first2=G. R. | last3=da Silva | first3=L. | last4=de La Reza | first4=R. | last5=Melo | first5=C. H. F. | last6=Sterzik | first6=M. | title=Search for associations containing young stars (SACY). I. Sample and searching method | journal=Astronomy and Astrophysics | volume=460 | issue=3 | pages=695–708 | doi=10.1051/0004-6361:20065602 | bibcode=2006A&A...460..695T | arxiv=astro-ph/0609258 | postscript=. |date=December 2006}}
8. ^{{cite journal | 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 | postscript=. |arxiv = 0806.2878 |date=September 2008}}
9. ^{{citation | display-authors=1 | last1=Maldonado | first1=J. | last2=Martínez-Arnáiz | first2=R. M. | last3=Eiroa | first3=C. | last4=Montes | first4=D. | last5=Montesinos | first5=B. | title=A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups | journal=Astronomy and Astrophysics | volume=521 | page=A12 | doi=10.1051/0004-6361/201014948 | bibcode=2010A&A...521A..12M | postscript=. |arxiv = 1007.1132 |date=October 2010}}
10. ^{{citation | display-authors=1 | last1=Plavchan | first1=Peter | last2=Werner | first2=M. W. | last3=Chen | first3=C. H. | last4=Stapelfeldt | first4=K. R. | last5=Su | first5=K. Y. L. | last6=Stauffer | first6=J. R. | last7=Song | first7=I. | title=New Debris Disks Around Young, Low-Mass Stars Discovered with the Spitzer Space Telescope | journal=The Astrophysical Journal | volume=698 | issue=2 | pages=1068–1094 |date=June 2009 | doi=10.1088/0004-637X/698/2/1068 | bibcode=2009ApJ...698.1068P | postscript=. |arxiv = 0904.0819 }}
11. ^{{cite simbad | title=53 Aqr | accessdate=2012-07-14 | postscript=. }} See also the children entries.
12. ^{{citation|title=The Colour of Stars |date=December 21, 2004 |work=Australia Telescope, Outreach and Education |publisher=Commonwealth Scientific and Industrial Research Organisation |url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html |accessdate=2012-01-16 |postscript=. |deadurl=yes |archiveurl=https://www.webcitation.org/6630AbtJZ?url=http://outreach.atnf.csiro.au/education/senior/astrophysics/photometry_colour.html |archivedate=March 10, 2012 }}
13. ^{{citation | last1=Tokovinin | first1=A. | last2=Cantarutti | first2=R. | title=First Speckle Interferometry at SOAR Telescope with Electron-Multiplication CCD | journal=Publications of the Astronomical Society of the Pacific | volume=120 | issue=864 | pages=170–177 | doi=10.1086/528809 | bibcode=2008PASP..120..170T | postscript=. |date=February 2008}}
[3][4][5][6][7][8][9][10][11][12][13]
}}{{Stars of Aquarius}}

10 : Aquarius (constellation)|Bayer objects|Flamsteed objects|G-type main-sequence stars|Hipparcos objects|Henry Draper Catalogue objects|HR objects|Durchmusterung objects|Gliese and GJ objects|Binary stars

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