But now, an international scientific team has performed an impressive work of celestial archaeology: they have used the interstellar dust as a look-back mirror that allowed them to receive news from the past.
Some light from that explosion was reflected by dust clouds placed at some distance from the dying star, and this reflection has been detected and analysed. This way, modern astronomy witnesses the cataclysmic display that our ancestors did not study, for some reason, in the 17th century. Calar Alto staff, telescopes and instruments have contributed to this finding.Supernovae in our Galaxy
Throughout the history of mankind Galactic supernovae (i.e., those that have exploded inside our Galaxy) have been among the most spectacular astronomical events witnessed. These flashes have been seen and written down starting in China more than two thousand years ago. No doubt, the most famous example is the explosion observed in year 1054, certainly seen by different cultures all across the Earth, but accurately registered only in the far East. This supernova led to the Crab nebula (in constellation Taurus). More recent supernovae were detected in 1572 (Tycho's supernova) and 1604 (Kepler's supernova). In both cases extremely bright, "new" stars were seen shining during several weeks at places where no previous object had been located before.
The celestial object known as Cassiopeia A (or, also, 3C 461) was the first astronomical source of radio waves detected in constellation Cassiopeia, around year 1940. It was identified soon as a supernova remnant, the remains of one of these giant explosive processes. The astronomical community was very puzzled, because the expansion rate of the gas inside Cassiopeia A indicates that the explosion had to be very recent (around 1680), but it seemed that the burst had never been observed.
Knowing the approximate outburst date from the gas motion inside Cassiopeia A, a search was started looking for observational records from 17th century, and finally a possible observation was found, done by the English astronomer John Flamsteed. The identification was not absolutely sure but, if true, it would imply that the Cassiopeia A supernova showed very faint in the Earth skies.
But the paths of science are often surprising and a team of researchers have now found the way to retake a part of the light that went straight past Earth more than three centuries ago, clarifying the nature and circumstances of the Cassiopeia A supernova. The key lays in the process known as light echoing.Light echoing
The light echo effect allows today to study in detail what happened 300 years ago: this process offers an action replay of the supernova which created the most spectacular supernova remnant on sky, and which has at most been witnessed by Flamsteed as a faint star in a time when the first telescopes had just been invented.
So, we are placed in front of this surprising paradox: interstellar dust, the main reason that prevented the study of the explosion in the 17th century, makes it possible to recover part of the lost light, but several centuries later, when human kind has developed much more powerful telescopes, instruments and theories, what allows a better understanding of this event.The research
The analysis of the light echo showed the signatures of the atoms present when Cassiopeia A exploded. The resulting spectrum of light revealed hydrogen and helium -- telltale signs that Cassiopeia A was once a huge red supergiant star whose core collapsed in a rare supernova referred to as "type IIb." Previously, it was not clear the supernova class to which Cassiopeia A belonged. The result contributes to expalain why the explosion went unnoticed in 1680. Beside the absorbing effect of interstellar dust, now it is necessary to add the specific behaviour of this kind of explosions: "Type IIb supernovae fade quickly," says co-author George Rieke (University of Arizona, United States of America). "This, plus a few cloudy nights, might explain the historical enigma around Cassiopeia A," explains Rieke, referring to the reason why it was not recorded by more observers.
Part of the observations leading to this discovery were performed at Calar Alto observatory in October 2007, with the 2.2 m telescope. Key observations were done, too, at Hawaii with the ground-based Subaru telescope, and with the orbiting Spitzer Space Telescope. But, as in any scientific pursue, all this work could be just the beginning. Oliver Krause announces: "We are already excited about future results from the echo research. Beside a detailed study of the Cassiopeia A supernova based on additional Calar Alto and Subaru observations this summer, we are also thinking about a variety of questions about the interstellar medium which can be addressed by the unique light echo experiment Nature has provided us with Cassiopeia A."
David Galadi-Enriquez | alfa
Water without windows: Capturing water vapor inside an electron microscope
13.12.2017 | Okinawa Institute of Science and Technology (OIST) Graduate University
Columbia engineers create artificial graphene in a nanofabricated semiconductor structure
13.12.2017 | Columbia University School of Engineering and Applied Science
MPQ scientists achieve long storage times for photonic quantum bits which break the lower bound for direct teleportation in a global quantum network.
Concerning the development of quantum memories for the realization of global quantum networks, scientists of the Quantum Dynamics Division led by Professor...
Researchers have developed a water cloaking concept based on electromagnetic forces that could eliminate an object's wake, greatly reducing its drag while...
Tiny pores at a cell's entryway act as miniature bouncers, letting in some electrically charged atoms--ions--but blocking others. Operating as exquisitely sensitive filters, these "ion channels" play a critical role in biological functions such as muscle contraction and the firing of brain cells.
To rapidly transport the right ions through the cell membrane, the tiny channels rely on a complex interplay between the ions and surrounding molecules,...
The miniaturization of the current technology of storage media is hindered by fundamental limits of quantum mechanics. A new approach consists in using so-called spin-crossover molecules as the smallest possible storage unit. Similar to normal hard drives, these special molecules can save information via their magnetic state. A research team from Kiel University has now managed to successfully place a new class of spin-crossover molecules onto a surface and to improve the molecule’s storage capacity. The storage density of conventional hard drives could therefore theoretically be increased by more than one hundred fold. The study has been published in the scientific journal Nano Letters.
Over the past few years, the building blocks of storage media have gotten ever smaller. But further miniaturization of the current technology is hindered by...
With innovative experiments, researchers at the Helmholtz-Zentrums Geesthacht and the Technical University Hamburg unravel why tiny metallic structures are extremely strong
Light-weight and simultaneously strong – porous metallic nanomaterials promise interesting applications as, for instance, for future aeroplanes with enhanced...
11.12.2017 | Event News
08.12.2017 | Event News
07.12.2017 | Event News
13.12.2017 | Health and Medicine
13.12.2017 | Physics and Astronomy
13.12.2017 | Life Sciences