Press Releases and Media Appearances
Long-period oscillations of the Sun discovered
Ten years of data from NASA’s Solar Dynamics Observatory combined with numerical models reveal the deep low musical notes of the Sun.
July 20, 2021
A team of solar physicists led by Laurent Gizon of the Max Planck Institute for Solar System Research (MPS) and the University of Göttingen in Germany has reported the discovery of global oscillations of the Sun with very long periods, comparable to the 27-day solar rotation period. The oscillations manifest themselves at the solar surface as swirling motions with speeds on the order of 5 kilometers per hour. These motions were measured by analyzing 10 years of observations from NASA’s Solar Dynamics Observatory (SDO). Using computer models, the scientists have shown that the newly discovered oscillations are resonant modes and owe their existence to the Sun’s differential rotation. The oscillations will help establish novel ways to probe the Sun’s interior and obtain information about our star’s inner structure and dynamics. The scientists describe their findings in a letter to appear today in the journal Astronomy & Astrophysics. [read full press-release article] |
Media Appearances:
- "Huge Waves in the Sun Discovered with NASA Mission" NASA (in English)
- "Scientists discovered global oscillations of the Sun with very long periods" Tech Explorist (in English)
- "Max-Planck-Institut für Sonnensystemforschung: Team entdeckt neue Schwingungen der Sonne" Göttinger Tageblatt (in German)
- "„Tiefe“ Schwingungen der Sonne entdeckt" Wissenschaft.de (in German)
Solar cycle 25 has begun
Since December 2019, solar activity has been on the up. This is consistent with predictions, to which MPS researchers contributed.
September 15, 2020
In the past one and a half years, the Sun has been rather dull: hardly a sunspot covered its surface, hardly a solar flare hurled radiation and particles into space. As observational data now show, for the last nine months solar activity has been slowly picking up again. Already in December 2019, our star passed its activity minimum, an event which occurs approximately every eleven years. This confirms predictions made by the Solar Cycle 25 Prediction Panel, an international panel of experts organized by NASA and NOAA (National Oceanic and Atmospheric Administration), in March last year. The panel, whose members include Dr. Robert Cameron from the Max Planck Institute for Solar System Research (MPS) in Germany, expects the Sun to be as tame in the now beginning solar cycle 25 as it has been in the previous eleven years.
[read full press-release article]
Media appearances:
- Welt (In German)
- Hessischen/Niedersächsischen Allgemeine (HNA) (in German)
- Reduktionsnetzwerk Deutschland (RND) (in German)
Gigantic, red and full of spots
About eight percent of red giants are covered by sunspot-like, dark areas. These stars rotate faster than others of their kind.
Starspots are more common among red giant stars than previously thought. In the journal Astronomy & Astrophysics, researchers led by the Max Planck Institute for Solar System Research (MPS) in Germany report that approximately eight percent of red giants exhibit such spots. They are the expression of strong magnetic fields at the stellar surface. These magnetic fields are created deep inside the star in a process that requires, among other things, convection and a fast rotation of the star. Although red giants are generally regarded as slowly rotating stars, those with starspots are apparently an exception. The new publication offers a comprehensive analysis of the reasons for their short rotation periods ranging from forced synchronization with another, closely neighboring star, to the swallowing of a star or planet, to a fast initial rotation speed in an early phase of development. [read full press-release article] |
Media appearances:
- Göttinger Tageblatt (in German)
Mystery of solar cycle illuminated
In the convection zone of the star, the plasma currents make a huge turnover that lasts about 22 year.
Solar activity fluctuates in a rhythm of about eleven years, which is reflected among other things in the frequency of sunspots. A complete magnetic period lasts 22 years. Scientists have long been puzzling over what causes this cycle. It must be related to the conditions beneath the "skin" of our star: A layer of hot plasma - electrically-conductive gas - extends from the surface to 200,000 kilometers below. The plasma within this convection zone is constantly in motion. A team of scientists from the Max Planck Institute for Solar System Research, the University of Göttingen and New York University Abu Dhabi has now succeeded in drawing the most comprehensive picture of the plasma flows in nort-south-direction to date. The researchers have found a remarkably simple flow geometry: the plasma describes a single turnover in each solar hemisphere, which lasts for about 22 years. In addition, the flow in the direction of the equator at the bottom of the convection zone causes spots to form closer and closer to the equator during the solar cycle. [read full press-release article] |
Media appearances:
A faint resemblance of Sun and Earth
The star Kepler-160 and its companion KOI-456.04 are more reminiscent of the Sun-Earth system than any previously known exoplanet-star pair
The star Kepler-160 is probably orbited by a planet less than twice the size of the Earth with a star-planet distance that could permit planetary surface temperatures conducive to life. The newly discovered exoplanet, which was found by a team of scientists led by the Max Planck Institute for Solar System Research (MPS) in Göttingen is more than just another potentially habitable world. One of the key properties making it resemble the Sun-Earth system more than any other previously known world, is its Sun-like host star. Most of the Earth-like exoplanets known so far are in orbit around a faint red dwarf star emitting their energy mostly as infrared radiation rather than as visible light. The light shed on KOI-456.04 by its Sun-like host star, however, is very much like the daylight seen on our home planet. Moreover, the orbital period of KOI-456.04 around its Sun-like star is almost identical to an Earth year.
[read full press-release article]
Media appearances:
- CNN (Englisch)
- RND (in German)
- Münsterland Zeitung (in German)
- Deutschlandfunk (radio, mp3, in German)
Older Press Releases
- 18 Earth-sized exoplanets discovered, May 2019 [Media: National Geographic article, EarthSky, Frankfurter Rundschau(in German), Spiegel (in German), HNA (in German) ]
- ERC synergy grant for solar physics at the MPS, October 2018 [Media: HNA (in German)]
- New External Scientific Member at the MPS, September 2018
- A new twist on stellar rotation, September 2018 [Media: Astronomy Now ]
- Giant swirls on the Sun, May 2018 [Media: The Daily Galaxy, Göttinger Tageblatt (in German)]
- Otto Hahn Medal for Jan Langfellner, June 2017
- Finding new Earths: PLATO spacecraft to be built, June 2017
- New Max Planck Fellow appointed at the MPS, April 2017
- Full Braking at Alpha-Centauri, February 2017
- Distant star is roundest object ever observed in nature, November 2016
- Slow appearance of sunspots challenges theory, July 2016
- Eavesdropping on Aliens, March 2016
- Giant hurricanes on the Sun, August 2014
- Stellar inventory: Searching for other Earths, February 2014
- Interior rotation of a distant star revealed, July 2013
- Unexpectedly slow motions below the Sun's surface, July 2012
Selected Old Research Highlights
Giant swirls on the Sun
May 7, 2018
A team of scientists led by the Max Planck Institute for Solar System Research (MPS) and the University of Göttingen has discovered new waves of vorticity on the Sun. As described in today’s issue of Nature Astronomy, these Rossby waves propagate in the direction opposite to rotation, have lifetimes of several months, and maximum amplitudes at the Sun’s equator. For forty years scientists had speculated about the existence of such waves on the Sun, which should be present in every rotating fluid system. Now, they have been unambiguously detected and characterized for the first time. The solar Rossby waves are close relatives of the Rossby waves known to occur in the Earth’s atmosphere and oceans.
A new twist on stellar rotation
September 20, 2018
The research project called WHOLESUN aims at understanding the origin of solar magnetic activity by studying the Sun in its entirety. It is funded through a prestigious Synergy Grant from the European Research Council (ERC), awarded to a team of four European Principal Investigators from the Max Planck Institute for Solar System Research (MPS) in Germany, the University of St Andrews in the UK, the CEA research centre in France, and the University of Oslo in Norway. The researchers will pool their expertise in solar physics over the next six years to determine how the magnetic field is generated in the solar interior to create sunspots on the solar surface and eruptions in the solar atmosphere. To this end, the team will attempt to model the Sun as a whole using supercomputers and incorporating observational knowledge from space missions.
ERC Synergy Grant for solar physics at the MPS
October 23, 2018
The research project called WHOLESUN aims at understanding the origin of solar magnetic activity by studying the Sun in its entirety. It is funded through a prestigious Synergy Grant from the European Research Council (ERC), awarded to a team of four European Principal Investigators from the Max Planck Institute for Solar System Research (MPS) in Germany, the University of St Andrews in the UK, the CEA research centre in France, and the University of Oslo in Norway. The researchers will pool their expertise in solar physics over the next six years to determine how the magnetic field is generated in the solar interior to create sunspots on the solar surface and eruptions in the solar atmosphere. To this end, the team will attempt to model the Sun as a whole using supercomputers and incorporating observational knowledge from space missions.
Slow appearance of sunspots challenges theory
Scientists find that sunspots rise to the surface much more slowly than predicted
July 13, 2016
Solar active regions consist of strongly magnetic sunspots and surrounding regions of more diffuse magnetic field. These regions are the origin of solar activity which controls space weather and causes beautiful phenomena such as aurora but in some cases also damage to satellites or power grids. Solar active regions are thought to be the result of magnetic flux concentrations - bundles of magnetic field lines - rising from deep in the solar interior and penetrating the surface. A team consisting of researchers from the Max Planck Institute for Solar System Research (MPS), The University of Göttingen, NorthWest Research Associates, and the High Altitude Observatory of the National Center for Atmospheric Research has now shown that these magnetic flux concentrations move upward through the solar interior at speeds of not more than about 150 m/s. This is much slower than predicted by the prevailing current model. For their study, which is published today in the journal Science Advances, they compared satellite observations and computer simulations.
Distant star is roundest object ever observed in nature
Scientists measure the shape of a pulsating star with unprecedented precision.
November 16, 2016
Stars are not perfect spheres, several mechanisms can change their shape. One mechanism is rotation: the more quickly a star rotates, the more flat it becomes due to the centrifugal force. Since distant stars appear as points in the sky, measuring their shape is a challenging task. A team of researchers led by Prof. Dr. Laurent Gizon from the Max Planck Institute for Solar System Research (MPS) and the University of Göttingen succeeded in measuring the oblateness of a slowly rotating star. In their study, which is published on 16 November, 2016 in the journal Science Advances, they determine for the first time stellar oblateness with unprecedented precision using asteroseismology – the study of the oscillations of stars. The technique is applied to a star 5000 light years (47,000,000 billion kilometers) away from Earth and reveals that the difference between the equatorial and polar radii of the star is only 3 kilometers – a number that is astonishing small compared to the star’s mean radius of 1.5 million kilometers.
Interior Rotation of a Distant Star Revealed
2013
With the help of asteroseismic data obtained by the CoRoT space telescope, scientists were able to determine the interior rotation of a Sun-like star - and characterise an exoplanet.
A team of scientists led by researchers from the Max Planck Institute for Solar System Research (Germany) and the University of Göttingen (Germany) have unambiguously measured the internal rotation of a Sun-like star and determined the inclination of its rotation axis for the first time. Their calculations show that the star rotates about 2.3 times faster than the Sun, with the axis of rotation inclined at 30 degrees to our line of sight. The star, HD52265, is located more than 90 light years away in the constellation of Monoceros. The results also prove that the body known to accompany the star is indeed an exoplanet and not - as previously argued - a small companion star called a brown dwarf. This is the first time that asteroseismology, the study of a star's internal oscillations, has been used to constrain the mass of an orbiting companion of a Sun-like star. The results were published in the journal "Proceedings of the National Academy of Sciences of the United States of America" (PNAS).
Seismic constraints on rotation of Sun-like star and mass of exoplanet, Gizon et al.,
Proceedings of the National Academy of Sciences of the United States of America (PNAS), Early Edition, 29. Juli 2013
doi:10.1073/pnas.1303291110