Aug. 30, 2013 — An international team of researchers presents fresh evidence that confirms the existence of the superheavy chemical element 115. The experiment was conducted at the GSI Helmholtz Center for Heavy Ion Research, an accelerator laboratory located in Darmstadt. Under the lead of physicists from Lund University in Sweden, the group, which included researchers from Johannes Gutenberg University Mainz (JGU) and the Helmholtz Institute Mainz (HIM), was able to present a way to directly identify new superheavy elements.Share This:Elements beyond atomic number 104 are referred to as superheavy elements. They are produced at accelerator laboratories and generally decay after a short time. Initial reports about the discovery of an element with atomic number 115 were released from a research center in Russia in 2004. The then presented indirect evidence for the new element, however, was insufficient for an official discovery.For the new experiment, scientists at the Institute of Nuclear Chemistry at Mainz University took a sample of the exotic element americium. They deposited an americium layer on a thin foil, which was subsequently bombarded with calcium ions at the GSI facility. For the first time, the exploitation of a new detector system allowed registering photons along with the alpha-decay of the new element and its daughter products. Measured photon energies correspond to those expected for X-rays from these products and thus serve as the element’s fingerprint.”This can be regarded as one of the most important experiments in the field in recent years, because at last it is clear that even the heaviest elements’ fingerprints can be taken”, agreed Professor Dirk Rudolph from Lund University in Sweden and Professor Christoph Düllmann, professor at Mainz University and leading scientist at GSI Darmstadt and HIM. …Read more
June 4, 2013 — Women are perceived as being more willing to lead if they show that they are proud of their personal performance. If, however, they give a cheerful impression, they are judged to have less willingness to leadership roles than men who display similar emotions. This is one of the initial findings of a long-term project in which economic researchers at Technische Universität München (TUM) are investigating the selection and assessment of leaders. They found that women themselves still expect more leadership qualities from men. In the next stage of their project, the TUM researchers want to develop gender-neutral HR management training programs.To increase their share of leadership positions, women are expected to tick a range of boxes — usually demonstrating improved negotiation skills, networking strengths and the ability to develop a strategic career ladder. “But even these skills are not enough,” maintains Professor Isabell Welpe of TUM’s Chair for Strategy and Organization. “They ignore the fact that there are stereotypes that on a subconscious level play a decisive role in the assessment of high achievers. Leaders should be assertive, dominant and hard-lined; women are seen as mediators, friendly, social.”Economic researchers from TUM decided to investigate the mechanisms behind the selection and assessment of leaders in business and academia and ways to challenge stereotypes. They presented their initial findings at a symposium yesterday.In a number of studies, researchers presented a variety of scenarios with (potential) leaders and their employees to randomly selected individuals. They then asked the study participants about their perceptions and expectations.It emerged that the same behavior exhibited by women and men in leadership positions is assessed in different ways. …Read more
May 30, 2013 — Detailed analysis and review have borne out researchers’ initial interpretation of pebble-containing slabs that NASA’s Mars rover Curiosity investigated last year: They are part of an ancient streambed.
The rocks are the first ever found on Mars that contain streambed gravels. The sizes and shapes of the gravels embedded in these conglomerate rocks — from the size of sand particles to the size of golf balls — enabled researchers to calculate the depth and speed of the water that once flowed at this location.
“We completed more rigorous quantification of the outcrops to characterize the size distribution and roundness of the pebbles and sand that make up these conglomerates,” said Rebecca Williams of the Planetary Science Institute, Tucson, Ariz., lead author of a report about them in the journal Science this week. “We ended up with a calculation in the same range as our initial estimate last fall. At a minimum, the stream was flowing at a speed equivalent to a walking pace — a meter, or three feet, per second — and it was ankle-deep to hip-deep.”
Three pavement-like rocks examined with the telephoto capability of Curiosity’s Mast Camera (Mastcam) during the rover’s first 40 days on Mars are the basis for the new report. One, “Goulburn,” is immediately adjacent to the rover’s “Bradbury Landing” touchdown site. The other two, “Link” and “Hottah,” are about 165 and 330 feet (50 and 100 meters) to the southeast. Researchers also used the rover’s laser-shooting Chemistry and Camera (ChemCam) instrument to investigate the Link rock.
“These conglomerates look amazingly like streambed deposits on Earth,” Williams said. “Most people are familiar with rounded river pebbles. Maybe you’ve picked up a smoothed, round rock to skip across the water. Seeing something so familiar on another world is exciting and also gratifying.”
The larger pebbles are not distributed evenly in the conglomerate rocks. In Hottah, researchers detected alternating pebble-rich layers and sand layers. This is common in streambed deposits on Earth and provides additional evidence for stream flow on Mars. In addition, many of the pebbles are touching each other, a sign that they rolled along the bed of a stream.
“Our analysis of the amount of rounding of the pebbles provided further information,” said Sanjeev Gupta of Imperial College, London, a co-author of the new report. “The rounding indicates sustained flow. It occurs as pebbles hit each other multiple times. This wasn’t a one-off flow. It was sustained, certainly more than weeks or months, though we can’t say exactly how long.”
The stream carried the gravels at least a few miles, or kilometers, the researchers estimated.
The atmosphere of modern Mars is too thin to make a sustained stream flow of water possible, though the planet holds large quantities of water ice. Several types of evidence have indicated that ancient Mars had diverse environments with liquid water. However, none but these rocks found by Curiosity could provide the type of stream flow information published this week. Curiosity’s images of conglomerate rocks indicate that atmospheric conditions at Gale Crater once enabled the flow of liquid water on the Martian surface.
During a two-year prime mission, researchers are using Curiosity’s 10 science instruments to assess the environmental history in Gale Crater on Mars, where the rover has found evidence of ancient environmental conditions favorable for microbial life.Read more