SN 1572

Supernova
name = Supernova SN 1572


caption = X-ray image of the SN 1572 remnant as seen by Chandra
epoch = ?
type = Type Ia
SNRtype = Nebula
host = Milky Way
constellation = Cassiopeia
ra = 0^h 25.3^m
dec = +64° 09′
gal = G.120.1+1.4
discovery = November 1572
iauc =
mag_v = -4
distance = convert|7500|ly|kpc|abbr=off|lk=on
progenitor = Unknown
progenitor_type = Unknown
b-v = Unknown
notes =

SN 1572 ("Tycho's Supernova", "Tycho's Nova"), "B Cassiopeiae" (B Cas), or "3C 10" was a supernova of Type Ia in the constellation Cassiopeia, one of about eight supernovae visible to the naked eye inhistorical records. It burst forth in early November 1572 and was independently discovered by many individuals.

Historic Description

The appearance of the Milky Way supernova of 1572 was perhaps one of the two or three most important events in the history of astronomy. The "new star" helped to shatter stale, ancient models of the heavens and to inaugurate a tremendous revolution in astronomy that began with the realized need to produce better astrometric star catalogues (and thus the need for more precise astronomical observing instruments). The supernova of 1572 is often called "Tycho's supernova", because of the extensive work that Tycho Brahe (1573, 1602, 1610)clarifyme|date=October 208 did in both observing the new star and in analyzing his own observations and those of many other observers. But Tycho was not even close to being the first to observe the 1572 supernova, although he was apparently the most accurate observer of the object (though not by much over some of his European colleagues like Wolfgang Schuler, Thomas Digges, John Dee and Francesco Maurolico).

The more reliable contemporary reports state that the new star itself burst forth sometime between 1572 November 2 and 6, when it rivalled Venus in brightness. The supernova remained visible to the naked eye into 1574, gradually fading until it disappeared from view.

The Supernova Remnant of SN 1572

Radiological Detection

The search for a supernova remnant was negative until a half-century ago, when Hanbury Brown and Hazard (1952) reported a radio detection at 158.5 MHz. [cite journal |last=Hanbury-Brown |first=R. |authorlink= |coauthors=Hazard, C. |year=1952 |month= |title=Radio-Frequency Radiation from Tycho Brahe's Supernova (A.D. 1572) |journal=Nature |volume=170 |issue=4322 |pages=364–365 |doi=10.1038/170364a0 |url= |accessdate= |quote= ] This was confirmed at wavelength 1.9 m by Baldwin and Edge (1957), [cite journal |last=Baldwin |first=J. E. |authorlink= |coauthors=Edge, D. O. |year=1957 |month= |title=Radio emission from the remnants of the supernovae of 1572 and 1604 |journal=The Observatory |volume=77 |issue= |pages=139–143 |bibcode=1957Obs....77..139B |url= |accessdate= |quote= ] and the remnant was also identified tentatively in the second Cambridge radio-source catalogue as object "2C 34" and identified more firmly as "3C 10" in the third Cambridge list (Edge et al. 1959). There is no dispute that 3C 10 is the remnant of the supernova observed in 1572-1573. Following a review article by Minkowski (1964), [cite journal |last=Minkowski |first=R. |authorlink= |coauthors= |year=1964 |month= |title=Supernovae and Supernova Remnants |journal=Annual Review of Astronomy and Astrophysics |volume=2 |issue= |pages=247–266 |doi=10.1146/annurev.aa.02.090164.001335 |url= |accessdate= |quote= ] the designation 3C 10 appears to be that most commonly used in the literature when referring to the radio remnant of B Cas (though some authors use the tabulated Galactic designation G120.7+2.1 of Green 1984, and many authors commonly refer to it as "Tycho's supernova remnant"—somewhat of a misnomer, as Tycho saw the pointlike supernova, not the expansive radio remnant). Because the radio remnant was reported before the optical supernova-remnant wisps were discovered, the designation 3C 10 is used by some to signify the remnant at all wavelengths.

SN 1572 is associated with the radio source G.120·1+1·4. It has an apparent diameter of 7.4 arc minutes, and is located approximately convert|7500|ly|kpc|abbr=off|lk=on from our Solar system.

Optical Detection

The supernova remnant of B Cas was discovered in the 1960s by scientists with a Palomar Mountain telescope as a very faint nebula. It was later photographed by a telescope on the international ROSAT spacecraft. The supernova was probably of Type Ia, in which a white dwarf star has accreted matter from a companion until it reaches the Chandrasekhar limit and explodes. This type of supernova does not typically create the spectacular nebula more typical of Type II supernovas, such as SN 1054 which created the Crab Nebula. A shell of gas is still expanding from its center at about 9,000 km/s.

Discovery of the Companion Star

In October 2004, a letter in "Nature" reported the discovery of a G2 star, similar in type to our own Sun. [cite journal |last=Ruiz-Lapuente |first=Pilar |authorlink= |coauthors="et al." |year=2004 |month= |title=The binary progenitor of Tycho Brahe's 1572 supernova |journal=Nature |volume=431 |issue=7012 |pages=1069–1072 |doi=10.1038/nature03006 |url= |accessdate= |quote= ] It is thought to be the companion star that contributed mass to the white dwarf that ultimately resulted in the supernova. A subsequent study, published in March 2005, revealed further details about this star: labeled Tycho G, it was likely a main sequence star or subgiant prior to the explosion, but had some of its mass stripped away and its outer layers shock-heated from the effects of the supernova. Tycho G's current velocity is perhaps the strongest evidence that it was the companion star to the white dwarf, as it is traveling at a rate of 136 km/s, which is more than forty times faster than the mean velocity of other stars in its stellar neighbourhood.

ee also

* List of supernova remnants

References

External links

* [http://www.seds.org/~spider/spider/Vars/sn1572.html SN 1572, Tycho's Supernova]
* [http://www.ing.iac.es/PR/newsletter/news9/science7.html The Search for the Companion Star of Tycho Brahe's 1572 Supernova]