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词条 DQ Herculis
释义

  1. In popular culture

  2. References

  3. External links

{{dablink|This article refers to Nova Herculis 1934. Information on the star DQ Herculis is also here. For the type of cataclysmic variable star known as DQ Herculis variables, see intermediate polars}}{{refimprove|date=March 2016}}{{Starbox begin |{{Starbox image
| image =
| caption = DQ Herculis
}}{{Starbox observe |
  epoch=J2000 |  ra=18h 07m 30.25s |  dec=+45° 51′ 32.6″ |  appmag_v=15.16 |  constell=Hercules }}
{{Starbox character |
  class=DBe+M2V|  b-v= |  u-b= |  variable=DQ Herculis }}
{{Starbox astrometry
| radial_v = -4
| prop_mo_ra =
| prop_mo_dec =
| parallax =
| p_error =
| absmag_v = 12.99
| dist_ly = {{convert|386|pc|ly|disp=output number only}}{{±|{{convert|33|pc|ly|disp=output number only}}|{{convert|29|pc|ly|disp=output number only}}}}
| dist_pc = {{val|386|33|29}}
}}{{Starbox detail
| mass = 0.7/0.4
| radius = 0.012/0.44
| luminosity = 0.0064/0.03
| temperature = 14,500/3,500
}}{{Starbox orbit
| period = 0.0002
| axis_unitless = 0.003 AU
| inclination = 81.7
}}{{Starbox catalog |{{Starbox reference |{{Starbox end}}DQ Herculis (or Nova Herculis 1934) was a slow, bright nova occurring in Hercules in December 1934. The nova was discovered on 13 December 1934 by J. P. M. Prentice from Stowmarket, Suffolk.[1] It reached peak brightness on 22 December 1934 with an apparent magnitude of 1.5.[2]

The nova remained visible to the naked eye for several months.[3]

DQ Herculis is the prototype for a category of cataclysmic variable stars called intermediate polars. The system shows orbital period variation, possibly due to the presence of a third body.[4]

In popular culture

The nova was one of the brightest objects observable in the night sky. In addition to scientific articles, and received significant coverage in popular news publications.[5][6] Brad Ricca, an English professor at Case Western Reserve University, has suggested that Nova Herculis may have influenced the development of the origin story of the comic book superhero Superman.[7]

References

1. ^{{Cite web|url=http://www.britastro.org/vss/00191a.html|title=DQ Her|website=www.britastro.org|access-date=2017-08-09}}
2. ^{{cite journal|author=Wright, W. H.| journal=Publications of the Astronomical Society of the Pacific| volume=47|number=275 |pages=47–49| year=1935|jstor=40670634|title=Comments on Nova Herculis 1934|bibcode = 1935PASP...47...47. |doi = 10.1086/124534 }}
3. ^{{cite web|url=http://www.thecrimson.com/article/1935/12/7/nova-herculis-discovered-in-december-1934/|title=Nova Herculis, Discovered in December 1934, Varies From First to Thirteenth Magnitudes--Now Fading, About Sixth|date=1935-12-07|accessdate=2013-08-08}}
4. ^{{cite journal| doi=10.1051/0004-6361/200810909| author=Dai & Qian| last2=Qian| first2=S. B.| title=Plausible explanations for the variations of orbital period in the old nova DQ Herculis| journal=Astronomy and Astrophysics| volume=503|issue=3 |pages=883–888| year=2009| bibcode=2009A&A...503..883D}}
5. ^{{cite news|url=https://select.nytimes.com/gst/abstract.html?res=9E02E6D6103EE53ABC4B51DFB467838F629EDE&n=Top%2fClassifieds%2fReal%20Estate%2fColumns%2fLiving%20In|title=The Week In Science: STAR OF BETHLEHEM A NOVA?; Recent Brilliant Outburst Recalls the Orb the Magi Followed|author=Waldemar Kaempffert|date=1934-12-23|accessdate=2013-08-08|work=The New York Times}}
6. ^{{cite news|url=http://www.time.com/time/magazine/article/0,9171,754501,00.html|title=Science: Nova Herculis; Swaseya|date=1934-12-31|accessdate=2013-08-08|work=Time}}
7. ^{{cite web|url=http://www.space.com/21949-superman-origin-star-explosion.html|title=Superman's Origins Possibly Born from Star Explosion|date=2013-07-12|accessdate=2013-08-07}}

}}

External links

  • http://www.daviddarling.info/encyclopedia/N/Nova_Herculis_1934.html
{{Stars of Hercules}}{{Novae}}

9 : Novae|Nova remnants|Hercules (constellation)|Intermediate polars|Hypothetical planetary systems|1934 in science|Objects with variable star designations|M-type main-sequence stars|Astronomical objects discovered in 1934

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