Pi Piscis Austrini

{{Short description|Star in the constellation Piscis Austrinus}}

{{Starbox begin}}

{{Starbox image

| image =

{{Location mark

|image=Piscis_Austrinus_IAU.svg|alt=|float=center|width=280

|label=|position=right

|mark=Red circle.svg|mark_width=12|mark_link=π PsA

|x%=26.4|y%=60.5

}}

| caption = Location of π Piscis Austrini (circled)

}}

{{Starbox observe

| constell = Piscis Austrinus

| epoch = J2000

| ra = {{RA|23|03|29.81653}}

| dec = {{DEC|−34|44|57.8827}}

| appmag_v = 5.12

}}

{{Starbox character

| type =

| class = {{nowrap|F1 V Fe-0.8}} + F3 V

| b-v = +0.29

| u-b = +0.00

| variable =

}}

{{Starbox astrometry

| radial_v = {{Val|−6.0|4.2}}

| prop_mo_ra = +72.789

| prop_mo_dec = +83.569

| parallax = 35.3691

| p_error = 0.2124

| parallax_footnote =

| absmag_v = +2.78

}}

{{Starbox orbit

| reference =

| period_unitless = {{Val|178.3177|0.0038|u=days}}

| axis_unitless = ≥ {{Convert|44.3e6|km|AU|disp=out|lk=on}}

| periastron = {{Val|2435319.73|0.25|fmt=commas}}

| eccentricity = {{Val|0.5286|0.0041}}

| periarg = {{Val|2.62|0.81}}

| k1 = {{Val|21.28|0.16}}

}}

{{Starbox detail

| component1 = A

| mass = 1.51

| radius = {{Val|1.64|0.11|0.08}}

| metal_fe = +0.12

| gravity = {{Val|4.30|0.14}}

| age_myr = 474

| luminosity = {{Val|5.85|0.04}}

| temperature = {{Val|7003|195|216|fmt=commas}}

| rotational_velocity =

}}

{{Starbox catalog

| names = {{odlist | B=π PsA | CD=−35°15630 | GJ=886.2 | GJ2=9807 | HD=217792 | HIP=113860 | HR=8767 | SAO=214275 | GC=32122 }}

}}

{{Starbox reference

| Simbad = pi+PsA

}}

{{Starbox end}}

Pi Piscis Austrini, Latinized from π Piscis Austrini, is binary star system in the southern constellation of Piscis Austrinus, near the eastern constellation border with Sculptor. It has a yellow-white hue and is visible to the naked eye as a dim point of light with an apparent visual magnitude of 5.12. The system is located at a distance of 92 light-years from the Sun based on parallax. Its radial velocity is poorly constrained, but it appears to be drifting closer at a rate of around −6 km/s. Pi Piscis Austrini is moving through the galaxy at a velocity of 16.3 km/s relative to the Sun. Its projected galactic orbit carries it between 24,000 and 37,500 light-years from the center of the galaxy.

This is a single-lined spectroscopic binary system with an orbital period of 178.3 days and an eccentricity of 0.53. The primary component is an F-type main-sequence star with a stellar classification of {{nowrap|F1 V Fe-0.8}}.

File:PiPsALightCurve.png for Pi Piscis Austrini, plotted from Hipparcos data]]

As of 2023, there appears to be no consensus in the astronomical literature about whether or not Pi Piscis Austrini is a variable star, and if it is variable, what type of variable star it is. In 1965 it was designated a classical Cepheid variable star with a visual (V) band brightness that varied by 0.3 magnitudes over a period of 7.975 days. The AAVSO's International Variable Star index lists it as a Gamma Doradus variable, with a V band magnitude range of 5.10 to 5.12. Axel Thomas, writing in the AAVSO's Journal, reports that the star appears to be a semiregular variable star, varying by 0.7 magnitudes in V band over a period of 8.625 days. Koen and Eyer examined the Hipparcos data for the star, and report it to be a microvariable with a period of 1.06039 days. On the other hand, the General Catalog of Variable Stars reports the star's brightness as constant, and in separate studies Michel Petit and E. Janot-Pacheco could not detect any change in brightness.

Pi Piscis Austrini displays an infrared excess, suggesting a circumstellar disk is orbiting at a radius of {{Val|23|u=AU}} with a mean temperature of 90 K. The cooler secondary companion has a class of F3 V. The system appears to be a source of X-ray emission.

References

{{reflist|refs=

{{cite simbad|title=* pi. PsA|accessdate=7 January 2017}}

{{cite DR2|6554537293934842496}}

{{cite web

| title=pi PsA | url=https://www.aavso.org/vsx/index.php?view=detail.top&oid=26602

| website=The International Variable Star Index | publisher=AAVSO

| access-date=1 January 2023}}

{{cite web

| url=https://cdsarc.cds.unistra.fr/viz-bin/ftp-index?/ftp/cats/more/HIP/cdroms/cats

| website=Centre de Données astronomiques de Strasbourg | title=/ftp/cats/more/HIP/cdroms/cats

| publisher=Strasbourg astronomical Data Center | access-date=15 October 2022}}

{{cite web

| title=pi. PsA | url=http://www.sai.msu.su/gcvs/cgi-bin/search2.cgi?search=pi.+PsA

| website=General Catalog of Variable Stars

| publisher=Sternberg Astronomical Institute, Moscow University | access-date=1 January 2023}}

{{cite journal

| last1=Petit | first1=Michel | title=Pi PsA | bibcode=1972IBVS..695....2P

| journal=Information Bulletin on Variable Stars |date=July 1972 |volume=695 |issue=2

| page=2 | url=https://ibvs.konkoly.hu/pub/ibvs/0601/0695.pdf | access-date=1 January 2023}}

{{cite journal

| last1=Thomas | first1=Axel | title=Π PsA - Who Are You?

| journal=The Journal of the American Association of Variable Star Observers

| date=June 1991 | volume=20 | issue=1 | pages=23–24 | bibcode=1991JAVSO..20...23T

| url=https://articles.adsabs.harvard.edu/pdf/1991JAVSO..20...23T | access-date=1 January 2023}}

{{cite journal

| 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

| date=March 2002 | volume=331 | issue=1 | pages=45–59

| doi=10.1046/j.1365-8711.2002.05150.x | doi-access=free | arxiv=astro-ph/0112194 | bibcode=2002MNRAS.331...45K

| s2cid=10505995 }}

{{cite journal

| title=A Comprehensive Census of Nearby Infrared Excess Stars

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| journal=The Astrophysical Journal Supplement Series

| volume=225 | issue=1 | id=15 | pages=24 | date=July 2016

| bibcode=2016ApJS..225...15C | arxiv=1606.01134

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| title=A catalogue of multiplicity among bright stellar systems

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| bibcode=2008MNRAS.389..869E | arxiv=0806.2878

| doi=10.1111/j.1365-2966.2008.13596.x | doi-access=free | s2cid=14878976 }}

{{cite journal

| title=On the cepheid nature of pi PsA

| last=Janot-Pacheco | first=E.

| journal=Astronomy and Astrophysics

| volume=34 | pages=325–326 | date=August 1974

| bibcode=1974A&A....34..325J }}

{{citation

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| doi=10.1134/S1063772917010085 | bibcode=2017ARep...61...80S | s2cid=125853869 | postscript=. }}

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| title=Contributions to the Nearby Stars (NStars) Project: spectroscopy of stars earlier than M0 within 40 pc-The Southern Sample

| display-authors=1 | 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 | s2cid=119476992 }}

{{cite journal

| title=Orbital elements of six spectroscopic binary stars

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| volume=147 | pages=355–366 | date=1970 | issue=4 | display-authors=1

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{{cite journal

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| arxiv=0910.3229 | s2cid=119267456 }}

{{cite journal

| title=UBV Photometry of Some Southern Stars (Second List)

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| volume=32 | page=11 | date=1973

| bibcode=1973MNSSA..32...11C | last1=Cousins

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{{cite journal

| title=XHIP: An extended hipparcos compilation

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| volume=38 | issue=5 | pages=331 | year=2012

| bibcode=2012AstL...38..331A | arxiv=1108.4971

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}}