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Coordinates: Sky map 20h 06m 15.457s, +44° 27′ 24.61″
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===Follow-up studies===
===Follow-up studies===
On 19 October 2015, the [[SETI Institute]] announced that it had begun using the [[Allen Telescope Array]] to look for [[radio frequency|radio emissions]] from possible intelligent extraterrestrial life in the vicinity of the star.<ref name="SP-20151019-mw">{{cite news |url=http://www.space.com/30855-alien-life-search-kepler-megastructure.html |title=Search For Intelligent Aliens Near Bizarre Dimming Star Has Begun |work=[[Space.com]] |last=Wall |first=Mike |date=19 October 2015 |accessdate=20 October 2015}}</ref><ref>{{cite news |url=http://www.businessinsider.com/search-for-aliens-at-kic-8462852-2015-10 |title=Scientists are days from finding out if that mysterious star could actually harbor aliens |work=Business Insider |first=Jessica |last=Orwig |date=23 October 2015}}</ref> After an initial two-week survey, the SETI Institute reported in November 2015 that it found no evidence of technology-related radio signals from the star system KIC 8462852.<ref name="SETI-20151105" /><ref name="SR-20151105" /><ref name="ARX-20151105" /><ref name="AXV-20151208" />
On 19 October 2015, the [[SETI Institute]] announced that it had begun using the [[Allen Telescope Array]] to look for [[radio frequency|radio emissions]] from possible intelligent extraterrestrial life in the vicinity of the star.<ref name="SP-20151019-mw">{{cite news |url=http://www.space.com/30855-alien-life-search-kepler-megastructure.html |title=Search For Intelligent Aliens Near Bizarre Dimming Star Has Begun |work=[[Space.com]] |last=Wall |first=Mike |date=19 October 2015 |accessdate=20 October 2015}}</ref><ref>{{cite news |url=http://www.businessinsider.com/search-for-aliens-at-kic-8462852-2015-10 |title=Scientists are days from finding out if that mysterious star could actually harbor aliens |work=Business Insider |first=Jessica |last=Orwig |date=23 October 2015}}</ref> After an initial two-week survey, the SETI Institute reported in November 2015 that it found no evidence of technology-related radio signals from the star system KIC 8462852.<ref name="SETI-20151105" /><ref name="SR-20151105" /><ref name="ARX-20151105" /><ref name="AXV-20151208" /> More recently, in February 2016, another SETI related study, using archival [[VERITAS|VERITAS gamma ray observatory]] observations from 2009 to 2015, did not find any evidence of [[Optical communication|pulsed optical beacons]] associated with KIC 8462852.<ref name="AXV-20160203">{{cite arxiv |author=Abeysekara, A.U. et al. |title=A Search for Brief Optical Flashes Associated with the SETI Target KIC 8462852 |date=3 February 2016 |eprint=1602.00987 |class=astro-ph.IM }}</ref>


A study of past infrared data from NASA's [[Spitzer Space Telescope]] and [[Wide-field Infrared Survey Explorer]] found no evidence for an excess of infrared emission from the star, which would have been an indicator of warm dust grains that could have come from catastrophic collisions of meteors or planets in the system. This absence of emission supports the hypothesis that a swarm of cold comets on an unusually eccentric orbit could be responsible for the star's unique light curve, but more studies are needed.<ref name="NASA-20151124"/><ref name="Marengo2015">{{cite journal |title=KIC 8462852: The Infrared Flux |journal=The Astrophysical Journal Letters |first1=Massimo |last1=Marengo |first2=Alan |last2=Hulsebus |first3=Sarah |last3=Willis |volume=814 |issue=1 |at=L15 |date=November 2015 |doi=10.1088/2041-8205/814/1/L15 |arxiv=1511.07908 |bibcode=2015ApJ...814L..15M}}</ref> A follow up 0.8–4.2 [[micron]] spectroscopic study of the system using the [[NASA Infrared Telescope Facility]] found no evidence for hot close-in dust, circumstellar matter from an evaporating or exploding planet, or long-lived large orbiting structure within a few [[astronomical unit]]s of the mature central star, but instead found similarities to another Gigayear-old system, [[Eta Corvi]], undergoing a [[Late Heavy Bombardment]].<ref name="NASA-20151124"/><ref name="Lisse2015">{{cite journal |title=IRTF/SPeX Observations of the Unusual Kepler Light Curve System KIC8462852 |journal=The Astrophysical Journal Letters |first1=Carey |last1=Lisse |first2=Michael |last2=Sitko |first3=Massimo |last3=Marengo |volume=815 |issue=2 |at=L27 |date=December 2015 |doi=10.1088/2041-8205/815/2/L27 |bibcode=2015ApJ...815L..27L |arxiv=1512.00121}}</ref> Submillimetre wavelength observations searching for farther-out cold dust in the system's Kuiper Belt suggest that a distant "catastrophic" planetary disruption explanation is unlikely; the possibility of a disrupted Kuiper Belt scattering comets into the inner system is still to be determined.<ref name="AXV-20151214">{{cite arXiv |title=Constraints on the circumstellar dust around KIC 8462852 |eprint=1512.03693 |class=astro-ph.SR |last1=Thompson |first1=M. A. |last2=Scicluna |first2=P. |last3=Kemper |first3=F. |last4=Geach |first4=J. E. |last5=Dunham |first5=M. M. |last6=Morata |first6=O. |last7=Ertel |first7=S. |last8=Ho |first8=P. T. P. |last9=Dempsey |first9=J. |last10=Coulson |first10=I. |last11=Petitpas |first11=G. |last12=Kirstensen |first12=L. E. |date=14 December 2015}} Submitted to [[Monthly Notices of the Royal Astronomical Society]].</ref>
A study of past infrared data from NASA's [[Spitzer Space Telescope]] and [[Wide-field Infrared Survey Explorer]] found no evidence for an excess of infrared emission from the star, which would have been an indicator of warm dust grains that could have come from catastrophic collisions of meteors or planets in the system. This absence of emission supports the hypothesis that a swarm of cold comets on an unusually eccentric orbit could be responsible for the star's unique light curve, but more studies are needed.<ref name="NASA-20151124"/><ref name="Marengo2015">{{cite journal |title=KIC 8462852: The Infrared Flux |journal=The Astrophysical Journal Letters |first1=Massimo |last1=Marengo |first2=Alan |last2=Hulsebus |first3=Sarah |last3=Willis |volume=814 |issue=1 |at=L15 |date=November 2015 |doi=10.1088/2041-8205/814/1/L15 |arxiv=1511.07908 |bibcode=2015ApJ...814L..15M}}</ref> A follow up 0.8–4.2 [[micron]] spectroscopic study of the system using the [[NASA Infrared Telescope Facility]] found no evidence for hot close-in dust, circumstellar matter from an evaporating or exploding planet, or long-lived large orbiting structure within a few [[astronomical unit]]s of the mature central star, but instead found similarities to another Gigayear-old system, [[Eta Corvi]], undergoing a [[Late Heavy Bombardment]].<ref name="NASA-20151124"/><ref name="Lisse2015">{{cite journal |title=IRTF/SPeX Observations of the Unusual Kepler Light Curve System KIC8462852 |journal=The Astrophysical Journal Letters |first1=Carey |last1=Lisse |first2=Michael |last2=Sitko |first3=Massimo |last3=Marengo |volume=815 |issue=2 |at=L27 |date=December 2015 |doi=10.1088/2041-8205/815/2/L27 |bibcode=2015ApJ...815L..27L |arxiv=1512.00121}}</ref> Submillimetre wavelength observations searching for farther-out cold dust in the system's Kuiper Belt suggest that a distant "catastrophic" planetary disruption explanation is unlikely; the possibility of a disrupted Kuiper Belt scattering comets into the inner system is still to be determined.<ref name="AXV-20151214">{{cite arXiv |title=Constraints on the circumstellar dust around KIC 8462852 |eprint=1512.03693 |class=astro-ph.SR |last1=Thompson |first1=M. A. |last2=Scicluna |first2=P. |last3=Kemper |first3=F. |last4=Geach |first4=J. E. |last5=Dunham |first5=M. M. |last6=Morata |first6=O. |last7=Ertel |first7=S. |last8=Ho |first8=P. T. P. |last9=Dempsey |first9=J. |last10=Coulson |first10=I. |last11=Petitpas |first11=G. |last12=Kirstensen |first12=L. E. |date=14 December 2015}} Submitted to [[Monthly Notices of the Royal Astronomical Society]].</ref>

Revision as of 21:58, 4 February 2016

KIC 8462852

KIC 8462852 in infrared and ultraviolet
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cygnus
Right ascension 20h 06m 15.457s
Declination +44° 27′ 24.61″
Apparent magnitude (V) +11.705±0.017
Characteristics
Evolutionary stage Main sequence[1]
Spectral type F3 V/IV
B−V color index 0.557
V−R color index 0.349
R−I color index 0.305
J−H color index 0.212
J−K color index 0.264
Astrometry
Distance1480 ly
(454 pc)
Absolute magnitude (MV)3.08[1][2]
Details
Mass1.43 M☉
Radius1.58 R☉
Luminosity (bolometric)4.7 L☉
Luminosity (visual, LV)5 L☉
Surface gravity (log g)4.0±0.2 cgs
Temperature6750±120 K
Metallicity0.0±0.1
Rotation0.8797±0.0001 days[1]
Rotational velocity (v sin i)84±4 km/s
Other designations
TYC 3162-665-1,[1] 2MASS J20061546+4427248[1]
Database references
SIMBADdata
KICdata

KIC 8462852[1] – eponymously Tabby's Star[3] (after lead author Tabetha S. Boyajian) or WTF Star (formally for "Where's The Flux?",[4][5][6][7] but also a reference to an expression of disbelief[8]) – is an F-type main-sequence star located in the constellation Cygnus approximately 454 parsecs (1,480 ly) from Earth. Unusual light fluctuations of the star were discovered by citizen scientists as part of the Planet Hunters project, and in September 2015 astronomers and citizen scientists associated with the project posted a preprint of a paper on arXiv describing the data and possible interpretations.[1] The discovery was made from data collected by the Kepler space telescope,[1][9] which observes changes in the brightness of distant stars in order to detect exoplanets.[10]

Several hypotheses have been proposed to explain the star's large irregular changes in brightness as measured by its unusual light curve. The leading hypothesis, based on a lack of observed infrared light, is that of a swarm of cold, dusty comet fragments in a highly eccentric orbit.[11][12][13] Many small masses in "tight formation" orbiting the star have also been proposed.[9] The changes in brightness could be signs of activity associated with intelligent extraterrestrial life building a Dyson swarm.[9][14][15][16] The SETI Institute's initial radio reconnaissance of KIC 8462852, however, found no evidence of technology-related radio signals from the star.[17][18][19][20]

Apparent location

Map showing location of NGC 6866. KIC 8462852 is northeast between NGC 6866 and ο¹ Cygni.

KIC 8462852 in Cygnus[21] is located roughly halfway between the major visually apparent bright stars Deneb (α Cyg, α Cygni, Alpha Cygni) and Rukh (δ Cyg, δ Cygni, Delta Cygni) to the eye as part of the Northern Cross.[22] KIC 8462852 is situated south of Omicron¹ Cygni (ο¹ Cygni, 31 Cygni), and northeast of the star cluster NGC 6866.[22] While only a few arcminutes away from the cluster, it is unrelated and closer to the Sun than it is to the star cluster. With an apparent magnitude of 11.7, the star cannot be seen by the naked eye, but is visible with a 5-inch (130 mm) telescope[23] in a dark sky with little light pollution.

Luminosity

Observations of the luminosity of the star by the Kepler space telescope show small, frequent, non-periodic dips in brightness, along with two large recorded dips in brightness appearing to occur roughly 750 days apart. The amplitude of the changes in the star's brightness, and the aperiodicity of the changes, mean that this star is of particular interest for astronomers.[16] The star's changes in brightness are consistent with many small masses orbiting the star in "tight formation".[9]

The first major dip, on 5 March 2011, obscured the star's brightness by up to 15%, and the other (on 28 February 2013) by up to 22%. In comparison, a planet the size of Jupiter would only obscure a star of this size by 1%, indicating that whatever is blocking light during the star's major dips is not a planet, but rather something covering up to half the width of the star.[16] Due to the failure of two of Kepler's reaction wheels, the star's predicted 750-day dip around April 2015 was not recorded;[1][15] further observations are planned for May 2017.[15]

A later study, published on 13 January 2016, and which may (or may not) be related to the within-day dimmings, indicates the star has gradually faded from 1890 to 1989 by about 20%, which is unprecedented for any F-type main sequence star.[24][25] However, a study published on 27 January 2016 concluded that the possible century-long dimming was likely a data artifact, and not a real astrophysical event.[3] The notion, that the findings of the century-long dimming is a data artifact, has been questioned.[26]

Hypotheses

Based on the star's spectral and star type, the star's changes in brightness could not be attributed to intrinsic variability,[1] so a few hypotheses have been proposed involving material orbiting the star and blocking its light, but none of these fully explain the observed data.

One proposed explanation for the star's odd reduction in light is that it is due to a cloud of disintegrating comets orbiting the star elliptically.[1][11][13][27] Under this scenario, gravity from a nearby star may have caused comets from the star's Oort cloud to fall in toward the star. Evidence supporting this hypothesis includes a red dwarf within 132 billion kilometers (885 AU) of KIC 8462852. However, the notion that disturbed Oort cloud comets orbiting elliptically close to the star could exist in high enough numbers to obscure 22% of the star's observed luminosity has been doubted.[16] Astronomer Bradley Schaefer studied photographic plates of the star from Harvard University, and, after averaging the data, found that the star had gradually dimmed by 20% between 1890 and 1989. He believes that it is extremely unlikely that one star would suffer two different mechanisms unique to that star and that only manifest in dimming the starlight by up to 20%; for this reason Schaefer thinks that the comets hypothesis is invalidated since dimming caused by comets over one century and within days is unrealistic.[24][25] A separate study concluded that the possible century-long dimming is more likely a data artifact than a real astrophysical event.[3] However, this study, suggesting that the century-long dimming is a data artifact, has been questioned.[26] As of February 2016, none of the related studies have been peer reviewed.

Artist's impression of an orbiting swarm of dusty comet fragments, which are a possible explanation for the unusual light signal of KIC 8462852.[11]

Nonetheless, other proposed explanations involve instrument or data artifacts, variable B(e) star, interstellar dust, a series of giant planets with very large ring structures,[28][29] and a recently captured asteroid field.[1]

High-resolution spectroscopy and imaging observations have also been made, as well as spectral energy distribution analyses using the Nordic Optical Telescope in Spain.[1][28] A massive collision scenario would create warm dust that glows in infrared wavelengths, but there is no observed excess infrared energy, ruling out massive planetary collision debris.[16] Other researchers think the planetary debris field explanation is unlikely, given the very low probability that Kepler would ever witness such an event due to the rarity of collisions of such size.[1]

Astronomer Jason Wright (who was consulted by Boyajian)[7][30] and others who have studied KIC 8462852, have suggested in a follow-up paper that if the star is younger than its position and speed would suggest, then it may still have coalescing material around it.[4] In addition, they hypothesized that the objects eclipsing the star could be parts of a megastructure made by an alien civilization, such as a Dyson swarm,[4][9][27][31][32][33] a hypothetical structure that an advanced civilization might build around a star to intercept some of its light for their energy needs.[34][35][36] Due to extensive media coverage on this matter, KIC 8462852 has been compared by Kepler's Steve Howell with KIC 4110611, another star with an odd light curve (which proved, after years of research, to be a part of a five-star system).[37] Regarding the current light curve data of KIC 8462852, Wright has emphasized the importance of upcoming spectral studies.[38] According to Wright, the likelihood of extraterrestrial intelligence being the cause of the dimming is very low; however, the star is an outstanding SETI target because natural explanations have yet to fully explain the dimming phenomenon.[4][31]

Follow-up studies

On 19 October 2015, the SETI Institute announced that it had begun using the Allen Telescope Array to look for radio emissions from possible intelligent extraterrestrial life in the vicinity of the star.[39][40] After an initial two-week survey, the SETI Institute reported in November 2015 that it found no evidence of technology-related radio signals from the star system KIC 8462852.[17][18][19][20] More recently, in February 2016, another SETI related study, using archival VERITAS gamma ray observatory observations from 2009 to 2015, did not find any evidence of pulsed optical beacons associated with KIC 8462852.[41]

A study of past infrared data from NASA's Spitzer Space Telescope and Wide-field Infrared Survey Explorer found no evidence for an excess of infrared emission from the star, which would have been an indicator of warm dust grains that could have come from catastrophic collisions of meteors or planets in the system. This absence of emission supports the hypothesis that a swarm of cold comets on an unusually eccentric orbit could be responsible for the star's unique light curve, but more studies are needed.[11][42] A follow up 0.8–4.2 micron spectroscopic study of the system using the NASA Infrared Telescope Facility found no evidence for hot close-in dust, circumstellar matter from an evaporating or exploding planet, or long-lived large orbiting structure within a few astronomical units of the mature central star, but instead found similarities to another Gigayear-old system, Eta Corvi, undergoing a Late Heavy Bombardment.[11][43] Submillimetre wavelength observations searching for farther-out cold dust in the system's Kuiper Belt suggest that a distant "catastrophic" planetary disruption explanation is unlikely; the possibility of a disrupted Kuiper Belt scattering comets into the inner system is still to be determined.[44]

Many optical telescopes are monitoring KIC 8462852 in anticipation of another multi-day dimming event, with planned follow-up observations of a dimming event using large telescopes equipped with spectrographs to determine if the eclipsing mass is a solid object, or is composed of dust or gas.[45] Additional follow-up observations may involve the ground-based Green Bank Telescope, the Very Large Array Radio Telescope,[28][46] and future orbital telescopes dedicated to exoplanetology such as WFIRST, TESS, and PLATO.[31][36]

See also

References

  1. ^ a b c d e f g h i j k l m n Boyajian, T. S.; LaCourse, D. M.; Rappaport, S. A.; Fabrycky, D.; Fischer, D. A.; et al. (11 September 2015). "Planet Hunters X. KIC 8462852 – Where's the Flux?". arXiv:1509.03622 [astro-ph.SR]. Submitted to Monthly Notices of the Royal Astronomical Society.
  2. ^ Pecaut, Mark J.; Mamajek, Eric E. (September 2013). "Intrinsic Colors, Temperatures, and Bolometric Corrections of Pre-main-sequence Stars". The Astrophysical Journal Supplement. 208 (1). 9. arXiv:1307.2657. Bibcode:2013ApJS..208....9P. doi:10.1088/0067-0049/208/1/9.
  3. ^ a b c Hippke, Michael; Angerhausen, Daniel (27 January 2016). "KIC 8462852 did likely not fade during the last 100 years". arXiv:1601.07314 [astro-ph.EP].
  4. ^ a b c d Wright, Jason (15 October 2015). "KIC 8462852: Where's the Flux?". AstroWright. Pennsylvania State University. Retrieved 16 October 2015.
  5. ^ Newsome, John (16 October 2015). "Space anomaly gets extraterrestrial intelligence experts' attention". CNN News. Retrieved 16 October 2015.
  6. ^ "Discovery of a strange star could mean alien life". Fox News. 15 October 2015. Retrieved 16 October 2015.
  7. ^ a b King, Bob (16 October 2015). "What's Orbiting KIC 8462852 – Shattered Comet or Alien Megastructure?". Universe Today. Retrieved 16 October 2015.
  8. ^ Strom, Marcus (15 October 2015), It's either aliens or a swarm of comets: scientists baffled by WTF 001, our galaxy's strangest star, The Sydney Morning Herald, retrieved 16 October 2015
  9. ^ a b c d e Andersen, Ross (13 October 2015). "The Most Mysterious Star in Our Galaxy". The Atlantic. Retrieved 13 October 2015.
  10. ^ Grush, Loren (16 October 2015). "Why it's so hard for astronomers to discuss the possibility of alien life". The Verge. Retrieved 17 October 2015.
  11. ^ a b c d e Clavin, Whitney; Johnson, Michele (24 November 2015). "Strange Star Likely Swarmed by Comets". NASA. Retrieved 24 November 2015.
  12. ^ Griffin, Andrew (25 November 2015). "Star that could have 'alien megastructure' around it is almost certainly covered by a swarm of comets, Nasa says". The Independent. Retrieved 26 November 2015.
  13. ^ a b Bodman, Eva H. L.; Quillen, Alice (27 November 2015). "KIC 8462852: Transit of a Large Comet Family". arXiv:1511.08821 [astro-ph.EP].
  14. ^ Kaplan, Sarah (15 October 2015). "The strange star that has serious scientists talking about an alien megastructure". The Washington Post. Retrieved 15 October 2015.
  15. ^ a b c Aron, Jacob (18 September 2015). "Citizen scientists catch cloud of comets orbiting distant star". New Scientist. Retrieved 15 October 2015.
  16. ^ a b c d e Plait, Phil (14 October 2015). "Did Astronomers Find Evidence of an Alien Civilization? (Probably Not. But Still Cool.)". Slate. Retrieved 15 October 2015.
  17. ^ a b "Looking For Deliberate Radio Signals From KIC 8462852". 5 November 2015. Retrieved 5 November 2015.
  18. ^ a b "Looking for Deliberate Radio Signals from KIC 8462852" (Press release). The SETI Institute. 5 November 2015. Retrieved 8 November 2015.
  19. ^ a b Harp, G. R.; Richards, Jon; Shostak, Seth; Tarter, J. C.; Vakoch, Douglas A.; et al. (5 November 2015). "Radio SETI Observations of the Anomalous Star KIC 8462852". arXiv:1511.01606 [astro-ph.EP].
  20. ^ a b Schuetz, Marlin; Vakoch, Douglas A.; Shostak, Seth; Richards, Jon (8 December 2015). "Optical SETI Observations of the Anomalous Star KIC 8462852". arXiv:1512.02388 [astro-ph.EP]. Submitted to The Astrophysical Journal Letters.
  21. ^ "KIC10 Search Results". Space Telescope Science Institute. Retrieved 16 October 2015.
  22. ^ a b Sinnott, Roger W. (2010). Sky & Telescope's Pocket Sky Atlas (3rd ed.). Cambridge, Massachusetts: Sky Publishing. ISBN 978-1-931559-31-7.
  23. ^ Masi, Gianluca (16 October 2015). "KIC 8462852: A star and its secrets". The Virtual Telescope Project 2.0. Retrieved 22 October 2015.
  24. ^ a b Aron, Jacob (15 January 2016). "Comets can't explain weird 'alien megastructure' star after all". New Scientist. Retrieved 16 January 2016.
  25. ^ a b Schaefer, Bradley E. (13 January 2016). "KIC 8462852 Faded at an Average Rate of 0.165+-0.013 Magnitudes Per Century From 1890 To 1989". arXiv:1601.03256 [astro-ph.SR].
  26. ^ a b Gilter, Paul (28 January 2016). "Bradley Schaefer: A Response to Michael Hippke". centauri-dreams.org. Retrieved 3 February 2016.
  27. ^ a b Fecht, Sarah (13 October 2015). "Have We Detected Megastructures Built By Aliens Around A Distant Star? Or Just A Cloud Of Comets? Scientists Want To Investigate Further". Popular Science. Retrieved 14 October 2015.
  28. ^ a b c Rzetelny, Xaq (16 October 2015). "Something—we're not sure what—is radically dimming a star's light". Ars Technica. Retrieved 17 October 2015.
  29. ^ Siegel, Ethan (16 October 2015). "No, Astronomers Probably Haven't Found 'Alien Megastructures'". Forbes. Retrieved 17 October 2015.
  30. ^ Laker, Chris (16 October 2015). "'Alien megastructure' may explain light patterns from 'bizarre' star, say scientists". BT.com. Retrieved 17 October 2015.
  31. ^ a b c Wright, Jason T.; Cartier, Kimberly M. S.; Zhao, Ming; Jontof-Hutter, Daniel; Ford, Eric B. (15 October 2015). "The Ĝ Search for Extraterrestrial Civilizations with Large Energy Supplies. IV. The Signatures and Information Content of Transiting Megastructures". arXiv:1510.04606 [astro-ph.EP]. Submitted to The Astrophysical Journal.
  32. ^ "Good night, sleep tight: Advanced alien civilisations rare or absent in the local Universe" (Press release). ASTRON. 15 September 2015. Retrieved 15 October 2015.
  33. ^ Williams, Lee (15 October 2015). "Astronomers may have found giant alien 'megastructures' orbiting star near the Milky Way". The Independent. Retrieved 15 October 2015.
  34. ^ Jones, Morris (November–December 2015). "Reconsidering macro-artefacts in SETI searches". Acta Astronautica. 116: 161–165. doi:10.1016/j.actaastro.2015.07.011.
  35. ^ O'Neill, Ian (14 October 2015). "Has Kepler Discovered an Alien Megastructure?". Discovery.com. Retrieved 17 October 2015.
  36. ^ a b Siemion, Andrew (29 September 2015). "Prepared Statement by Andrew Siemion – Hearing on Astrobiology". House Committee on Science, Space, and Technology. SpaceRef.com. Retrieved 19 October 2015.
  37. ^ "Mysterious star stirs controversy in astronomy world". The Express Tribune. Agence France-Presse. 20 October 2015.
  38. ^ Orwig, Jessica (15 October 2015). "We spoke with some of the astronomers who discovered the 'alien' megastructure to find out if it's fact or fiction". Business Insider.
  39. ^ Wall, Mike (19 October 2015). "Search For Intelligent Aliens Near Bizarre Dimming Star Has Begun". Space.com. Retrieved 20 October 2015.
  40. ^ Orwig, Jessica (23 October 2015). "Scientists are days from finding out if that mysterious star could actually harbor aliens". Business Insider.
  41. ^ Abeysekara, A.U.; et al. (3 February 2016). "A Search for Brief Optical Flashes Associated with the SETI Target KIC 8462852". arXiv:1602.00987 [astro-ph.IM]. {{cite arXiv}}: Explicit use of et al. in: |author= (help)
  42. ^ Marengo, Massimo; Hulsebus, Alan; Willis, Sarah (November 2015). "KIC 8462852: The Infrared Flux". The Astrophysical Journal Letters. 814 (1). L15. arXiv:1511.07908. Bibcode:2015ApJ...814L..15M. doi:10.1088/2041-8205/814/1/L15.
  43. ^ Lisse, Carey; Sitko, Michael; Marengo, Massimo (December 2015). "IRTF/SPeX Observations of the Unusual Kepler Light Curve System KIC8462852". The Astrophysical Journal Letters. 815 (2). L27. arXiv:1512.00121. Bibcode:2015ApJ...815L..27L. doi:10.1088/2041-8205/815/2/L27.
  44. ^ Thompson, M. A.; Scicluna, P.; Kemper, F.; Geach, J. E.; Dunham, M. M.; Morata, O.; Ertel, S.; Ho, P. T. P.; Dempsey, J.; Coulson, I.; Petitpas, G.; Kirstensen, L. E. (14 December 2015). "Constraints on the circumstellar dust around KIC 8462852". arXiv:1512.03693 [astro-ph.SR]. Submitted to Monthly Notices of the Royal Astronomical Society.
  45. ^ Wall, Mike (28 October 2015). "'Alien Megastructure' Mystery May Soon Be Solved". Space.com. Retrieved 28 October 2015.
  46. ^ Mack, Eric (17 October 2015). "The story behind 'alien megastructures' scientists may have found (but probably didn't)". CNET. Retrieved 19 October 2015.

External links

Retrieved from "https://en.wikipedia.org/w/index.php?title=Tabby%27s_Star&oldid=703333680"