PSR B0329+54

{{Short description|Pulsar in the constellation Camelopardalis}}

{{Starbox short

| name = PSR B0329+54

| epoch = J2000

| constell = Camelopardalis

| ra = {{RA|03|32|59.368}}

| dec = {{DEC|+54|34|43.57}}

| appmag_v =

| absmag_v =

| dist_ly = 3,460

| dist_pc = 1,060

| spectral = Pulsar

| names = NVSS J033259+543444, PSR B0329+54, PSR J0332+5434, TXS 0329+544, PULS CP 0329, 2MASS J03325936+5434448

| Simbad = PSR+B0329%2B54

}}

PSR B0329+54 is a pulsar approximately 3,460 light-years away in the constellation of Camelopardalis. It completes one rotation every 0.71452 seconds and is approximately 5 million years old.

The emissions of this pulsar and the Vela Pulsar were converted into audible sound by the French composer Gérard Grisey, and used as such in the piece Le noir de l'étoile (1989–90).Re, Giuseppe del. 2000. Cosmic Dance, pp. 24–25. Templeton Foundation Press, {{ISBN|9781890151256}}Luminet, Jean-Pierre. 2011. Illuminations: Cosmos et esthétique, pp. 419–420. Odile Jacob, {{ISBN|9782738185938}}{{IRCAM work|id=8960|title=Gérard Grisey: Le Noir de l'étoile}}

Planetary system

In 1999, two exoplanets were announced to be orbiting the pulsar (being classified as pulsar planets). Later observations did not support this conclusion. More recently, a 2017 analysis indicates that a different long-period pulsar planet remains a possibility, but this was subsequently challenged as well.

{{OrbitboxPlanet begin

| table_ref =

| period_unit = year

}}

{{OrbitboxPlanet hypothetical

| exoplanet = b

| mass_earth = 1.97 ± 0.19

| period = 27.76 ± 0.03

| semimajor = 10.26 ± 0.07

| eccentricity = 0.236 ± 0.011

| status = disputed

}}

{{Orbitbox end}}

See also

References

{{Reflist|refs=

{{citation

| display-authors=1

| last1=Cutri | first1=R. M. | last2=Skrutskie | first2=M. F.

| last3=van Dyk | first3=S. | last4=Beichman | first4=C. A.

| last5=Carpenter | first5=J. M. | last6=Chester | first6=T.

| last7=Cambresy | first7=L. | last8=Evans | first8=T.

| last9=Fowler | first9=J. | last10=Gizis | first10=J.

| last11=Howard | first11=E. | last12=Huchra | first12=J.

| last13=Jarrett | first13=T. | last14=Kopan | first14=E. L.

| last15=Kirkpatrick | first15=J. D. | last16=Light | first16=R. M.

| last17=Marsh | first17=K. A. | last18=McCallon | first18=H.

| last19=Schneider | first19=S. | last20=Stiening | first20=R.

| last21=Sykes | first21=M. | last22=Weinberg | first22=M.

| last23=Wheaton | first23=W. A. | last24=Wheelock | first24=S.

| last25=Zacarias | first25=N.

|date=June 2003 | publisher=NASA/IPAC

| title=2MASS All Sky Catalog of point sources

| bibcode=2003tmc..book.....C

| postscript=.

}}

{{citation

| last1=Hobbs | first1=G.

| last2=Lyne | first2=A. G.

| last3=Kramer | first3=M.

| title=An analysis of the timing irregularities for 366 pulsars

| journal=Monthly Notices of the Royal Astronomical Society

| volume=402 | issue=2 | pages=1027–1048

| date=February 2010

| doi=10.1111/j.1365-2966.2009.15938.x

| doi-access=free

| bibcode=2010MNRAS.402.1027H

| postscript=.

|arxiv = 0912.4537 | s2cid=119269505

}}

{{citation

| display-authors=1 | last1=Konacki | first1=Maciej

| last2=Lewandowski | first2=Wojciech | last3=Wolszczan | first3=Alex

| last4=Doroshenko | first4=Oleg | last5=Kramer | first5=Michael

| title=Are There Planets around the Pulsar PSR B0329+54?

| journal=The Astrophysical Journal

| volume=519 | issue=1 | pages=L81–L84 | date=July 1999

| bibcode = 1999ApJ...519L..81K

| doi = 10.1086/312089

| postscript=.

| doi-access=free }}

{{citation

| display-authors=1

| last1=Shabanova | first1=T. V.

| last2=Pugachev | first2=V. D.

| last3=Lapaev | first3=K. A.

| title=Timing Observations of 27 Pulsars at the Pushchino Observatory from 1978 to 2012

| journal=The Astrophysical Journal

| volume=775 | issue=1 | id=2 | pages=24 | date=September 2013

| doi=10.1088/0004-637X/775/1/2

| bibcode=2013ApJ...775....2S | arxiv=1307.0297

| s2cid=119110237 | postscript=.

}}

{{Cite journal|arxiv = 1710.01153|doi = 10.1134/S1063772917110063|title = On the existence of planets around the pulsar PSR B0329+54|year = 2017|last1 = Starovoit|first1 = E. D.|last2 = Rodin|first2 = A. E.|journal = Astronomy Reports|volume = 61|issue = 11|pages = 948–953|bibcode = 2017ARep...61..948S|s2cid = 119460916 |mode=cs2}}

{{cite journal |last1=Potapov |first1=V. A. |last2=Andrianov |first2=S. A. |date=November 2023 |title=Testing the Hypothesis about the Existence of a Planet Orbiting the Pulsar B0329+54 (J0332+5434) |journal=Astronomy Letters |volume=49 |issue=10 |pages=547–552 |doi=10.1134/S1063773723100067 |bibcode=2023AstL...49..547P}}

}}

{{Stars of Camelopardalis}}

{{DEFAULTSORT:PSR B0329+54}}

Category:Pulsars

Category:Camelopardalis

Category:Hypothetical planetary systems

J03325936+5434448

{{var-star-stub}}