Supernova X-rays: too little too soon.
Supernova X-rays: Too little too soon
It was a brilliant burst of light near the object 30 Doradus in the Large Magellanic Cloud Noun 1. Large Magellanic Cloud - the larger of the two Magellanic Clouds visible from the southern hemisphere
Magellanic Cloud - either of two small galaxies orbiting the Milky Way; visible near the south celestial pole last February that first called attention to the explosion of the nearest supernova in almost 400 years. Seeing the light first is natural for human beings. But as astronomers rush to observe this supernova 1987A, one of the main things they expect to record is radiation in the invisible portions of the electromagnetic spectrum electromagnetic spectrum
Total range of frequencies or wavelengths of electromagnetic radiation. The spectrum ranges from waves of long wavelength (low frequency) to those of short wavelength (high frequency); it comprises, in order of increasing frequency (or decreasing .
All this radiation is physically the same as ordinary light, but visible light occupies only a short range of wavelengths in the middle of the total spectrum. As the expanding front of the supernova explosion becomes transparent to more and more wavelengths, new sections of the spectrum keep coming in. The latest are X-rays, recorded simultaneously and separately by a Japanese X-ray satellite and a German experiment attached to a Soviet space station.
The Japanese satellite Ginga and a West German X-ray telescope called Hexe, attached to the Soviet Mir space station, have found X-rays that appear to come from the supernova. Juergen Truemper of the Max Planck Institute for Extraterrestrial Physics The Max Planck Institute for Extraterrestrial Physics is a Max Planck Institute, located in Garching, near Munich, Germany. In 1991 the Max Planck Institute for Physics and Astrophysics (MPIFEP) in Garching, West Germany, and Yasuo Tanaka of the Institute of Space and Astronautical Science in Tokyo reported their groups' findings last week at the Fourth George Mason University Named after American revolutionary, patriot and founding father George Mason, the university was founded as a branch of the University of Virginia in 1957 and became an independent institution in 1972. Workshop on Astrophysics astrophysics, application of the theories and methods of physics to the study of stellar structure, stellar evolution, the origin of the solar system, and related problems of cosmology. , held in Fairfax, Va.
Both groups agree that the supernova emits X-rays in the so-called hard X-ray range from 15 to 350 kilo-electron-volts (keV) energy. However, Ginga found an X-ray spectrum that extends beyond 15 keV down at least to 5 keV, into what observers call the "soft X-ray' range. Hexe, which belongs to the MPIFEP and the University of Tubingen, is not sensitive to these low-energy X-rays. However, another experiment on the Mir station, TTM TTM
Trailing 12 months. Often used with Earnings Per Share. , belonging to the University of Birmingham Due to Birmingham's role as a centre of light engineering, the university traditionally had a special focus on science, engineering and commerce, as well as coal mining. It now teaches a full range of academic subjects and has five-star rating for teaching and research in several (England) and the Space Research Laboratory in Utrecht, the Netherlands, should have been sensitive to these soft X-rays but didn't find them. Gerry Skinner of the University of Birmingham reported that TTM recorded no soft X-ray flux and was able to say only that the intensity of supernova soft X-rays, if any, had to be lower than the instrument's threshold.
Tanaka tried to minimize what he called a "difference' rather than a "discrepancy' between the two reports and expressed confidence that it would be resolved. Others at the meeting were taking it more seriously. Robert P. Kirshner of the Harvard-Smithsonian Center for Astrophysics The Harvard-Smithsonian Center for Astrophysics (CfA) is located in Cambridge, Massachusetts. It consists of the Harvard College Observatory and the Smithsonian Astrophysical Observatory. The Center is located at 60 Garden Street. in Cambridge, Mass., who has been following the supernova in ultraviolet since it exploded, remarked, "Come on, fellows, we can't both be right.'
Astrophysicists eagerly await each addition to the range of the supernova's emissions because different ranges of the spectrum are evidence of different physical processes they believe occur in the supernova. The hard X-rays hard x-rays
x-rays of shorter wavelength.
hard x-rays Radiation physics Short wavelength, high-frequency and highly penetrating megavolt range–eg, produced by 60Cobalt–X-rays used in RT or generated by nuclear 'incidents'. Cf Soft X-rays. found in these discoveries are supposed to come ultimately from processes of nuclear fusion and nuclear decay that between them make the heavier chemical elements. These processes in supernovas are particularly important to astrophysicists and nuclear physicists, because supernovas appear to be the only place in nature where the heaviest elements can be made.
The nuclear processes actually produce gamma rays Gamma rays
Electromagnetic radiation emitted from excited atomic nuclei as an integral part of the process whereby the nucleus rearranges itself into a state of lower excitation (that is, energy content). , a form of electromagnetic radiation electromagnetic radiation, energy radiated in the form of a wave as a result of the motion of electric charges. A moving charge gives rise to a magnetic field, and if the motion is changing (accelerated), then the magnetic field varies and in turn produces an that is harder (more energetic and of higher frequency) than X-rays. However, according to the theoretical models, at the time of the reported observations (July through September) the matter in the expanding supernova shock front should still have been opaque to gamma rays. As they move around inside the supernova, the gamma rays collide with electrons in a process called Compton scattering, by which their energies and frequencies are diminished until they fall into the X-ray range. Then they can get out.
However, the spectrum of hard X-rays found by the observers is, as Tanaka said, "unusual for any kind of X-ray source.' The intensity of the hard X-rays rose during July and August, but not as fast as theoretical models of supernovas predict. It dropped off in September, and so it may also be peaking earlier than the models expect. Theoretical suggestions thrown off the cuff to meet this situation include the idea that there may be less matter in the supernova than theorists have thought, or that it may not be uniform but patchy, so that there are gaps or rare spots in it. Either way, X-rays could get out sooner than expected.
The soft X-rays are even more of a question. Theorists tend to agree that the supernova front is still dense enough to be opaque to them. So some propose that the soft X-rays are coming from interstellar in·ter·stel·lar
Between or among the stars: interstellar gases.
between or among stars
Adj. 1. material just outside the supernova front, which is being struck and disturbed by the expanding front.