The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of a black hole, has revealed a new view of the massive object at the centre of the galaxy Messier 87 (M87): how it looks in polarised light. This is the first time astronomers have been able to measure polarisation, a signature of magnetic fields, this close to the edge of a black hole. The observations are key to explaining how the galaxy, located 55 million light-years away, is able to launch energetic jets from its core.
“We are now seeing the next crucial piece of evidence to understand how magnetic fields behave around black holes, and how activity in this very compact region of space can drive powerful jets that extend far beyond the galaxy,” says Monika Mościbrodzka, Coordinator of the EHT Polarimetry Working Group and Assistant Professor at Radboud University in the Netherlands.
On 10 April 2019, scientists released the first ever image of a black hole, revealing a bright ring-like structure with a dark central region — the black hole’s shadow. Since then, the EHT collaboration has delved deeper into the data on the supermassive object at the heart of the M87 galaxy collected in 2017. They have discovered that a significant fraction of the light around the M87 black hole is polarised.
“This work is a major milestone: the polarisation of light carries information that allows us to better understand the physics behind the image we saw in April 2019, which was not possible before,” explains Iván Martí-Vidal, also Coordinator of the EHT Polarimetry Working Group and GenT Distinguished Researcher at the University of Valencia, Spain. He adds that “unveiling this new polarised-light image required years of work due to the complex techniques involved in obtaining and analysing the data.”
Light becomes polarised when it goes through certain filters, like the lenses of polarised sunglasses, or when it is emitted in hot regions of space where magnetic fields are present. In the same way that polarised sunglasses help us see better by reducing reflections and glare from bright surfaces, astronomers can sharpen their view of the region around the black hole by looking at how the light originating from it is polarised. Specifically, polarisation allows astronomers to map the magnetic field lines present at the inner edge of the black hole.
“The newly published polarised images are key to understanding how the magnetic field allows the black hole to 'eat' matter and launch powerful jets,” says EHT collaboration member Andrew Chael, a NASA Hubble Fellow at the Princeton Center for Theoretical Science and the Princeton Gravity Initiative in the US.
The bright jets of energy and matter that emerge from M87’s core and extend at least 5000 light-years from its centre are one of the galaxy’s most mysterious and energetic features. Most matter lying close to the edge of a black hole falls in. However, some of the surrounding particles escape moments before capture and are blown far out into space in the form of jets.
Astronomers have relied on different models of how matter behaves near the black hole to better understand this process. But they still don’t know exactly how jets larger than the galaxy are launched from its central region, which is comparable in size to the Solar System, nor how exactly matter falls into the black hole. With the new EHT image of the black hole and its shadow in polarised light, astronomers managed for the first time to look into the region just outside the black hole where this interplay between matter flowing in and being ejected out is happening.
The observations provide new information about the structure of the magnetic fields just outside the black hole. The team found that only theoretical models featuring strongly magnetised gas can explain what they are seeing at the event horizon.
“The observations suggest that the magnetic fields at the black hole’s edge are strong enough to push back on the hot gas and help it resist gravity’s pull. Only the gas that slips through the field can spiral inwards to the event horizon,” explains Jason Dexter, Assistant Professor at the University of Colorado Boulder, US, and Coordinator of the EHT Theory Working Group.
To observe the heart of the M87 galaxy, the collaboration linked eight telescopes around the world – including the ALMA (Atacama Large Millimeter/submillimeter Array) and APEX (Atacama Pathfinder EXperiment) in northern Chile – to create a virtual Earth-sized telescope, the EHT. The impressive resolution obtained with the EHT is equivalent to that needed to measure the length of a credit card on the surface of the Moon.
“With ALMA and APEX, which through their southern location enhance the image quality by adding geographical spread to the EHT network, European scientists were able to play a central role in the research,” says Ciska Kemper, European ALMA Programme Scientist at ESO. “With its 66 antennas, ALMA dominates the overall signal collection in polarised light, while APEX has been essential for the calibration of the image.”
"ALMA data were also crucial to calibrate, image and interpret the EHT observations, providing tight constraints on the theoretical models that explain how matter behaves near the black hole event horizon," adds Ciriaco Goddi, a scientist at Radboud University and Leiden Observatory, the Netherlands, who led an accompanying study that relied only on ALMA observations.
The EHT setup allowed the team to directly observe the black hole shadow and the ring of light around it, with the new polarised-light image clearly showing that the ring is magnetised. The results are published today in two separate papers by the EHT collaboration in Astrophysical Journal Letters.
The research involved over 300 researchers from multiple organisations and universities worldwide.
Chalmers scientists Michael Lindqvist and John Conway, both at Onsala Space Observatory and the Department of Space, Earth and Environment, represent Sweden in the EHT collaboration.
"In Onsala we have participated since the 1960s in the development of very long baseline interferometry (VLBI), the technique used in the EHT. Onsala Space Observatory is one of three partners in APEX, one of the telescopes in the EHT network, and we have worked for many years with our partners building up capacity for VLBI at APEX", says Michael Lindqvist.
“The Swedish contribution to this research has been significant", says Iván Martí-Vidal, who worked at Onsala Space Observatory until 2018. “The observatory in Onsala has also been responisble for calibrating ALMA data, and its role as a partner in the APEX telescope has been critical for being able to calculate and correct for the instrumental polarisation in ALMA."
Detailed knowledge of these aspects is of great importance for the conclusions about the supermassive black hole that have now been presented.
This research is presented in two papers by the EHT collaboration published on 24 March 2021 in Astrophysical Journal Letters: "First M87 Event Horizon Telescope Results VII: Polarization of the Ring" (doi: 10.3847/2041-8213/abe71d) and "First M87 Event Horizon Telescope Results VIII: Magnetic Field Structure Near The Event Horizon" (doi: 10.3847/2041-8213/abe4de). Accompanying research is presented in the paper "Polarimetric properties of Event Horizon Telescope targets from ALMA" (doi: 10.3847/2041-8213/abee6a) by Goddi, Martí-Vidal, Messias, and the EHT collaboration, which has been accepted for publication in Astrophysical Journal Letters.
Robert Cumming, communications officer, Onsala Space Observatory, Chalmers, +46 70-493 31 14, email@example.com
Michael Lindqvist, astronomer, Onsala Space Observatory, Chalmers, firstname.lastname@example.org
A (överst) - A view of the M87 supermassive black hole in polarised light. The lines mark the orientation of polarisation, which is related to the magnetic field around the shadow of the black hole.
B - Composite image showing M 87's supermassive black hole and jet, as seen in polarized light. Images from different radio telescopes show the jet's polarisation at different scales. Top: ALMA observations taken at the same time as the EHT observations. In the middle are measurements with the VLBA in the USA. The EHT observations are shown at the bottom of the image.
Bild: EHT Collaboration; ALMA (ESO/NAOJ/NRAO), Goddi et al.; VLBA (NRAO), Kravchenko et al.; J. C. Algaba, I. Martí-Vidal
C: Jetstrålen i M 87 i polariserat ljus uppmätt av ALMA.
Bild: ALMA (ESO/NAOJ/NRAO), Goddi et al.