Astronomers use Subaru Telescope data to chart the expansion history of the universe with supernovae

An international research team analyzed a database of more than 1000 supernova explosions and found that models for the expansion of the Universe best match the data when a new time-dependent variation is introduced. If proven correct with future, higher-quality data from the Subaru Telescope and other observatories, these results could indicate still unknown physics working on the cosmic scale.

Edwin Hubble's observations over 90 years ago showing the expansion of the Universe remain a cornerstone of modern astrophysics. But when you get into the details of calculating how fast the Universe was expanding at different times in its history, scientists have difficulty getting theoretical models to match observations. Schematical representation of the expansion of the Universe over the course of its history.  CREDIT NAOJ

To solve this problem, a team led by Maria Dainotti (Assistant Professor at the National Astronomical Observatory of Japan and the Graduate University for Advanced Studies, SOKENDAI in Japan and an affiliated scientist at the Space Science Institute in the U.S.A.) analyzed a catalog of 1048 supernovae which exploded at different times in the history of the Universe. The team found that the theoretical models can be made to match the observations if one of the constants used in the equations, appropriately called the Hubble constant, is allowed to vary with time.

There are several possible explanations for this apparent change in the Hubble constant. A likely but boring possibility is that observational biases exist in the data sample. To help correct for potential biases, astronomers are using Hyper Suprime-Cam on the Subaru Telescope to observe fainter supernovae over a wide area. Data from this instrument will increase the sample of observed supernovae in the early Universe and reduce the uncertainty in the data.

But if the current results hold up under further investigation, if the Hubble constant is in fact changing, that opens the question of what is driving the change. Answering that question could require a new, or at least modified, version of astrophysics.

These results will appear as M.G. Dainotti et al. "On the Hubble Constant Tension in the SNe Ia Pantheon Sample" in the Astrophysical Journal on May 17, 2021.

Russian scientists develop method for predicting solar radio flux for two years ahead

Scientists at the Skolkovo Institute of Science and Technology (Skoltech) and their colleagues from the University of Graz & the Kanzelhöhe Observatory (Austria) and the ESA European Space Operations Centre developed a method and software called RESONANCE to predict the solar radio flux activity for 1-24 months ahead. RESONANCE will serve to improve the specification of satellite orbits, re-entry services, modeling of space debris evolution, and collision avoidance maneuvers. The research results were published in the Astrophysical Journal Supplement Series.

Since the launch of Sputnik, the Earth's first artificial satellite, in 1957, more than 41,500 tons of manmade objects have been placed in orbit around the Sun, the Earth, and other planetary bodies. Since that time, the majority of objects, such as rocket bodies and large pieces of space debris, re-entered the Earth's atmosphere in an uncontrolled way, posing a potential hazard to people and infrastructure. Predicting the re-entry date and time is a challenging task, as one needs to specify the density of the upper Earth atmosphere that strongly depends on solar activity which, in turn, is hard to predict. Earth's atmosphere can become very heated due to solar activity which causes it to expand, and a satellite can decay in its orbit and fall back to the Earth due to the effect known as atmospheric drag. In addition, there is a lot of space debris, much of it very small; if a spacecraft unexpectedly changes its orbit and encounters even a small piece of debris, this would be equivalent to hitting a bomb because of the high speed. A piece of a re-entering space object found in Indonesia. The sphere measures about 50 cm in diameter and weighs 7.4 kg.  CREDIT ESA

An international group of scientists led by Skoltech professor Tatiana Podladchikova developed a new method and software called RESONANCE ("Radio Emissions from the Sun: ONline ANalytical Computer-aided Estimator") which provides predictions of the solar radio flux at F10.7 and F30 cm with a lead time of 1 to 24 months. The F10.7 and F30 indices represent the flux density of solar radio emissions at a wavelength of 10.7 and 30 cm averaged over an hour and serve as a solar proxy of the ultraviolet solar emission which heats the Earth's upper atmosphere. The method combines state-of-art physics-based models and advanced data assimilation methods, where the resulting F10.7 and F30 forecasts are used as solar input in the re-entry prediction tool for further estimation of an object re-entry time.

"We systematically evaluated the performance of RESONANCE in providing re-entry predictions on past ESA re-entry campaigns for 602 payloads and rocket bodies as well as 2,344 objects of space debris that re-entered from 2006 to 2019 over the full 11-year solar cycle. The test results demonstrated that the predictions obtained by RESONANCE in general also lead to improvements in the forecasts of re-entry epochs and can thus be recommended as a new operational service for re-entry predictions and other space weather applications," says lead author and Skoltech's MSc graduate Elena Petrova who is currently pursuing her Ph.D. studies at the Centre for Mathematical Plasma Astrophysics, Catholic University of Leuven (KU Leuven).

"The number of re-entered objects is closely related to the solar activity level: the majority of objects return during the maximum solar activity phase within the 11-year cycle. Interestingly, the space debris re-entry time closely follows the evolution of the cycle, reacting immediately to changes in solar activity. At the same time, payloads and rocket bodies also show a large number of re-entries during the declining phase of the cycle, which may be related to the time delay between solar activity and re-entry for large objects", says professor Astrid Veronig, a co-author of the study and director of Kanzelhöhe Observatory at the University of Graz.

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"It is very important to monitor and predict solar activity for orbit prediction needs. For example, Skylab which was intended to perform a controlled re-entry in the 1970s dropped on Earth in an uncontrolled way due to inaccurate calculations of the atmospheric drag due to solar activity. Another example is the most recent launch of the Chinese Long March 5B rocket on May 9, 2021: the remnants from its second stage that carried China's first space station module made an uncontrolled re-entry and landed in the Indian Ocean. Thus the development of robust and reliable space weather operational services bringing together the forefront of research with engineering applications is of prime importance for the protection of space and ground-based infrastructures and advancement of space exploration. And whatever storms may rage, we wish everyone good weather in space," says Tatiana Podladchikova, assistant professor at the Skoltech Space Center (SSC) and a research co-author. Frequency of re-entered objects during 11-year solar cycle 24. Top: F10.7 cm radio flux data. Middle: Number of payloads and rocket bodies re-entered. Bottom: Number of objects of space debris re-entered.  CREDIT Petrova et al., 2021

Currently, the team is preparing RESONANCE for operational use as part of a new space weather service for continuous prediction of solar radio flux activity.

CEA, IFP Energies nouvelles renew their collaboration

The CEA and IFP Energies nouvelles (IFPEN) have just signed an agreement extending their collaboration initiated in 2007 on the numerical code framework called Arcane in the field of high-performance computations.

The CEA Military Applications Division launched the Arcane software platform in 2000 within the scope of the Simulation program. It is used to optimize the performance of large parallel-processing supercomputers and to manage complex data for 3D unstructured meshes. Thanks to its sophisticated object-oriented design, Arcane is both flexible and modular in its construction of simulation software, offering different levels of reading. It also gives players involved in the development process (physicists, numerical analysts, and computer scientists) the opportunity to focus on their core activities. This approach simplifies the development of innovative scientific tools in shorter time frames. vignettearcane 2 02b9a

Since 2007, the CEA and IFPEN have been working together to further develop the Arcane platform, sharing technical breakthroughs along the way. IFPEN Ressources Energétiques Carnot Institute has recently been exploiting this platform to develop a new-generation simulator for its research in geosciences.

Since the end of nuclear testing in 1996, the Simulation program has ensured the safety and reliability of nuclear weapons for France. It is based on the modeling of physical phenomena that describe how nuclear weapons work, resolving equations using supercomputers, and experimental validation in large test facilities.

  • Interactive development environments (IDE), with improvements to end-user support, from writing algorithms to debugging in a parallel configuration
  • Performance of computer codes, with adaptations to the platform to accept new architectures combining processors and accelerators
  • Software engineering, including steps to modularise the platform
  • Open-source distribution of the Arcane platform.

The open-source licensing of Arcane represents a key milestone in the platform’s development, enabling its promotion within the scientific community, fast-tracking collaboration with other research organizations and universities (internships, PhDs, and post-doctoral research), simplifying contributions to public-funded projects (ANR, future investments program, etc.), and encouraging the submission of articles in journals and for conferences.