The Suffering Never Ends

Affirmations i use to study/get things done!

"You've prepared the whole year for this. Don't let it go to waste." "I can and I will." "It doesn't matter how hard it takes to reach my goal." "It doesn't matter if the other person is more talented than you. There's no rule for them to work more harder than you." "You can wake up anyday and decide to change the person that you are." "Who cares if I'm pretty if I fail my finals?" "One day, you'll leave this world behind so live a life that you'll remember." "If it's a million to one. I'm gonna be that one.” "You can't be perfect. No one can. But you can try to be the best." "Failure is a part of success. Use it in the best way possible." "You are more than capable of handling yourself and your textbooks." "Study like you haven't prayed and pray like you haven't studied." "You came this far only to come this far?" "There is no way I'm going to come back with something I don't like." "Study because learning is better than being ignorant." "Grades aren't everything but they do make your life somewhat easier." "I know more than i think I do." “There are no shortcuts to any place worth going.”  "Progress > Perfection." "You're doing this for you. Only you. Don't forget that."

1/100

ugh didn't do that much, or at least not as much as I would have wanted to.

I went to school for the extra maths classes, then came home and solved quite a lot of maths problems, and then went to maths tutoring. I arrived home at 7 pm, it is almost 11 pm and I have been procrastinating since. I will try and study a little for Romanian tonight, cause there are some concepts I really need to understand.

I'll eventually reblog tomorrow with what I managed to do tonight!!!

I want this 🥺

Recoloring old black and white lgbt photos (1/?)

An accurate description of the life of a 1st year astrophysics major:

going to class and your professor talking fondly about the "wonderful feeling after the elevator cable snaps while you're in it"

said professor then proceeding to play a rock song

on most days only expect 2-5 students in class even though we have 13

where did the others go?? nobody knows, maybe they were abducted by aliens

speaking of aliens

your other professor pausing class to talk about what would happen if we met them

and getting mildly upset that an asteroid is no longer headed towards earth

cats

just so many physics department cats

and celebrating their birthdays

nobody in the department sleeps

don't be alarmed when your professor goes to the group chat at 3am to talk about whatever

hating elon musk

somehow other majors don't think astrophysics majors actually attend school until they meet you

there are days where we only talk about why star trek wasn't safe (they never wore seatbelts for a long time!!)

we like frogs

and rocks

rock go brrrr

sometimes finding your professor's face photoshopped onto satellites

working for hours but having 0 progress

your prof. assuring you that this is normal even for professionals

random scifi talks and book recs

cats

everyone in the dept likes greek letters

getting back to your dorm at almost midnight

the hall is eerily quiet but nobody is asleep

crying over the moon is normal

so is crying over the mars rovers

crying in general is normal

your professor saying odd things like

"this is just some weird image of two people about to die- but anyway, spacetime"

the astronomers of the school are also the astrologers

setting up in the lounge reading people's birth charts and astro cards

having to sneak through the back of the building because our id cards never work

sitting in the observatory with the lights off waiting for the professor to get there

planning to bring your hallmates to the planetarium to impress them

did i mention the cats?

meow

why do we have things that glow?

and this????

idk might make a pt. 2 or not

Learning to like Physics

I actually cannot believe how much I used to hate Physics until last year, but then I actually took the time and effort to understand it and?? it’s so cool and fun and easy?? unreal.

It literally seemed impossible for me and I legit thought I wouldn’t be able to graduate because I was never gonna pass Physics (I’m a Math major so we actually have 4 required Physics courses). I don’t know what the point of this is but, don’t be afraid of Physics guys!! (or any other subject!!) yes it’s frustrating as hell and you feel dumb for not having a clue about what is happening or how to work out the problems but I swear once it clicks for you (and it will) it’s gonna be great.

So if anyone needs a step by step (for college/uni), here’s one:

Google is your best friend, the internet has plenty of videos/papers/worked out problems for you to check out. The most important thing to look for is drawings and videos that help you visualize what’s going on. In most of general physics, the key is to see what forces are acting, and from that follows everything else.

Know your core equations. Honestly it’s always the same ones in the end.

For mechanics: you absolutely gotta know Newton’s Laws, Work and its relation to Kinetic/Potential Energy. Momentum is also important.

For thermodynamics: First and Second Law of Thermodynamics; pV = nRT, Boyle/Gay Lussac etc (note that they’re all connected), Carnot’s Cycle.

For electromagnetism: Maxwell’s equations. This is as far as I’ve gotten in my studies.

Understand where the formulas come from, rather than learning them by heart. For me, this was necessary because my memory is absolutely shit so there was no way I could remember every variation. But most of the formulas actually do make sense, and once you’ve drawn out a diagram of what’s happening, you can work them out yourself.

For the previous point, I suggest you watch and rewatch your professor’s explanation until you get the gist. Don’t get discouraged if it’s not immediately crystal clear, seek out other explanations if you need to. Then try to do it yourself.

ASK. FOR. HELP. I cannot stress this enough, do not feel ashamed about asking questions in class or during office hours. There are no stupid questions, and you’re paying thousands every year for people to teach you. Also physics is hard, so you’re pretty much expected to not understand immediately. Moreover, I can guarantee there’s at least one other person in the room with the same question who’s too afraid to ask. I was that person, and I failed the class because of it. Don’t be me.

Practice until you’re able to do most variations of standard problems. Once you’re able to do a certain problem, try to change it and see what happens. You don’t have to crunch the numbers all over again, go with your intuition first. Then you can calculate everything and see if you were correct.

This is all I’ve got at the moment. It applies to General Physics because I’m still pretty shit at Mathematical Physics (Rational Mechanics?) lmao, which is why I don’t talk about Lagrangians and such here.

If anyone has any other tips (for Mathematical Physics as well!) , please feel free to add them. Note that I’m from Italy, and this is what it was like for me. Other countries might have different ways of testing or focus on some formulas that I haven’t included. Do what works for you, obviously.

Good luck STEM students, I know it’s hard, but hopefully worth it in the long run :)

omg,,,,,,their hearts were full of love and blood and whiskey,,,,,,,

Nastya Rasputina Pride Icons

Jonny丨Nastya丨Ashes丨Brian丨Ivy丨TS丨Tim丨Raphaella丨Marius

☆requests☆

What if after Neil died, Todd went and visited Neil's grave every day and one day, a few years after graduation, he went to Neil's grave and set a ring on the head stone asking if Neil would marry him. Neil would have obviously said yes if he were still alive so Todd buries the ring a little under the ground near the headstone and wears his around just to remind him of his first and last love. The ring is engraved with Neil's name and the day he killed himself.

(Thank you for this very sad headcanon @/the.poet.and.the.actor on Instagram.)

a short french lesson: les negatives

the common french negation with ne/pas is used to contradict or deny a statement. today we will learn more ways to express this, using words other than “pas.” 

note : in spoken french, the ne is usually dropped, but i will include it in these examples. 

ne… jamais : never, not ever example: je ne suis pas triste means i am not sad, while je ne suis jamais triste means i am never sad. 

ne… rien : nothing, not anything example: je n’ai pas de livre means i don’t have any books, while je n’ai rien means i don’t have anything.

ne… personne : nobody, no one, not anyone example: je ne parle pas means i don’t speak, while je ne parle à personne means i don’t speak to anyone.

ne… plus : not anymore, no longer example: je ne travaille pas means i am not woking, while je ne travaille plus means i am no longer working.

ne… que : only example: il ne voit pas les lions means he doesn’t see the lions, while il ne voit que les lions means he only sees the lions. 

ne… pas encore : not yet example: il n’est pas arrivé means he has not arrived, while il n'est pas encore arrivé means he has not arrived yet. 

ne… pas du tout : at all example: je n’ai pas faim means i am not hungry, while je n’ai pas du tout faim means i am not hungry at all. 

ne… ni : neither, nor example: il ne voit ni les lions, ni les tigres means he sees neither the lions nor the tigers. 

the odd ones, personne and rien 

ce matin, madeleine ne veut voir personne means this morning, madeleine doesn’t want to see anybody.

il ne veut parler à personne means he does not want to talk to anybody. 

elle ne pense à rien means she is not thinking about anything. 

alright, french lesson over! let me know if i need to change anything or if you have questions. merci d'avoir lu ce texte ☺

Astronomers image magnetic fields at the edge of M87’s black hole

The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of a black hole, has today revealed a new view of the massive object at the centre of the Messier 87 (M87) galaxy: 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 M87 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 northern Chile-based Atacama Large Millimeter/submillimeter Array (ALMA) and the Atacama Pathfinder EXperiment (APEX), in which the European Southern Observatory (ESO) is a partner — 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 in The Astrophysical Journal Letters by the EHT collaboration.

The research involved over 300 researchers from multiple organisations and universities worldwide.

“The EHT is making rapid advancements, with technological upgrades being done to the network and new observatories being added.

We expect future EHT observations to reveal more accurately the magnetic field structure around the black hole and to tell us more about the physics of the hot gas in this region,” concludes EHT collaboration member Jongho Park, an East Asian Core Observatories Association Fellow at the Academia Sinica Institute of Astronomy and Astrophysics in Taipei.

More information

This research was presented in two papers by the EHT collaboration published today in The 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 The Astrophysical Journal Letters.

The EHT collaboration involves more than 300 researchers from Africa, Asia, Europe, North and South America.

The international collaboration is working to capture the most detailed black hole images ever obtained by creating a virtual Earth-sized telescope.

Supported by considerable international investment, the EHT links existing telescopes using novel systems — creating a fundamentally new instrument with the highest angular resolving power that has yet been achieved.

The individual telescopes involved are: ALMA, APEX, the Institut de Radioastronomie Millimetrique (IRAM) 30-meter Telescope, the IRAM NOEMA Observatory, the James Clerk Maxwell Telescope (JCMT), the Large Millimeter Telescope (LMT), the Submillimeter Array (SMA), the Submillimeter Telescope (SMT), the South Pole Telescope (SPT), the Kitt Peak Telescope, and the Greenland Telescope (GLT). The EHT consortium consists of 13 stakeholder institutes: the Academia Sinica Institute of Astronomy and Astrophysics, the University of Arizona, the University of Chicago, the East Asian Observatory, Goethe-Universitaet Frankfurt, Institut de Radioastronomie Millimétrique, Large Millimeter Telescope, Max Planck Institute for Radio Astronomy, MIT Haystack Observatory, National Astronomical Observatory of Japan, Perimeter Institute for Theoretical Physics, Radboud University and the Smithsonian Astrophysical Observatory.

ESO is the foremost intergovernmental astronomy organisation in Europe and the world’s most productive ground-based astronomical observatory by far. It has 16 Member States: Austria, Belgium, the Czech Republic, Denmark, France, Finland, Germany, Ireland, Italy, the Netherlands, Poland, Portugal, Spain, Sweden, Switzerland and the United Kingdom, along with the host state of Chile and with Australia as a Strategic Partner. ESO carries out an ambitious programme focused on the design, construction and operation of powerful ground-based observing facilities enabling astronomers to make important scientific discoveries. ESO also plays a leading role in promoting and organising cooperation in astronomical research. ESO operates three unique world-class observing sites in Chile: La Silla, Paranal and Chajnantor. At Paranal, ESO operates the Very Large Telescope and its world-leading Very Large Telescope Interferometer as well as two survey telescopes, VISTA working in the infrared and the visible-light VLT Survey Telescope. Also at Paranal ESO will host and operate the Cherenkov Telescope Array South, the world’s largest and most sensitive gamma-ray observatory. ESO is also a major partner in two facilities on Chajnantor, APEX and ALMA, the largest astronomical project in existence. And on Cerro Armazones, close to Paranal, ESO is building the 39-metre Extremely Large Telescope, the ELT, which will become “the world’s biggest eye on the sky”.

The Atacama Large Millimeter/submillimeter Array (ALMA), an international astronomy facility, is a partnership of ESO, the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile. ALMA is funded by ESO on behalf of its Member States, by NSF in cooperation with the National Research Council of Canada (NRC) and the Ministry of Science and Technology (MOST) and by NINS in cooperation with the Academia Sinica (AS) in Taiwan and the Korea Astronomy and Space Science Institute (KASI). ALMA construction and operations are led by ESO on behalf of its Member States; by the National Radio Astronomy Observatory (NRAO), managed by Associated Universities, Inc. (AUI), on behalf of North America; and by the National Astronomical Observatory of Japan (NAOJ) on behalf of East Asia. The Joint ALMA Observatory (JAO) provides the unified leadership and management of the construction, commissioning and operation of ALMA.

The BlackHoleCam research group was awarded the European Research Council €14 million Synergy Grant in 2013. The Principal Investigators are Heino Falcke, Luciano Rezzolla and Michael Kramer and the partner institutes are JIVE, IRAM, MPE Garching, IRA/INAF Bologna, SKA and ESO. BlackHoleCam is part of the Event Horizon Telescope collaboration.

IMAGE 1….The Event Horizon Telescope (EHT) collaboration, who produced the first ever image of a black hole released in 2019, has today a new view of the massive object at the centre of the Messier 87 (M87) galaxy: 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. This image shows the polarised view of the black hole in M87. The lines mark the orientation of polarisation, which is related to the magnetic field around the shadow of the black hole. Credit: EHT Collaboration

IMAGE 2….This composite image shows three views of the central region of the Messier 87 (M87) galaxy in polarised light. The galaxy has a supermassive black hole at its centre and is famous for its jets, that extend far beyond the galaxy. One of the polarised-light images, obtained with the Chile-based Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, shows part of the jet in polarised light. This image captures the part of the jet, with a size of 6000 light years, closer to the centre of the galaxy. The other polarised light images zoom in closer to the supermassive black hole: the middle view covers a region about one light year in size and was obtained with the National Radio Astronomy Observatory’s Very Long Baseline Array (VLBA) in the US. The most zoomed-in view was obtained by linking eight telescopes around the world to create a virtual Earth-sized telescope, the Event Horizon Telescope or EHT. This allows astronomers to see very close to the supermassive black hole, into the region where the jets are launched. The lines mark the orientation of polarisation, which is related to the magnetic field in the regions imaged.The ALMA data provides a description of the magnetic field structure along the jet. Therefore the combined information from the EHT and ALMA allows astronomers to investigate the role of magnetic fields from the vicinity of the event horizon (as probed with the EHT on light-day scales) to far beyond the M87 galaxy along its powerful jets (as probed with ALMA on scales of thousand of light-years). The values in GHz refer to the frequencies of light at which the different observations were made. The horizontal lines show the scale (in light years) of each of the individual images. Credit: EHT Collaboration; ALMA (ESO/NAOJ/NRAO), Goddi et al.; VLBA (NRAO), Kravchenko et al.; J. C. Algaba, I. Martí-Vidal

IMAGE 3…. This composite image shows three views of the central region of the Messier 87 (M87) galaxy in polarised light and one view, in the visible wavelength, taken with the Hubble Space Telescope. The galaxy has a supermassive black hole at its centre and is famous for its jets, that extend far beyond the galaxy. The Hubble image at the top captures a part of the jet some 6000 light years in size. One of the polarised-light images, obtained with the Chile-based Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, shows part of the jet in polarised light. This image captures the part of the jet, with a size of 6000 light years, closer to the centre of the galaxy. The other polarised light images zoom in closer to the supermassive black hole: the middle view covers a region about one light year in size and was obtained with the National Radio Astronomy Observatory’s Very Long Baseline Array (VLBA) in the US. The most zoomed-in view was obtained by linking eight telescopes around the world to create a virtual Earth-sized telescope, the Event Horizon Telescope or EHT. This allows astronomers to see very close to the supermassive black hole, into the region where the jets are launched. The lines mark the orientation of polarisation, which is related to the magnetic field in the regions imaged. The ALMA data provides a description of the magnetic field structure along the jet. Therefore the combined information from the EHT and ALMA allows astronomers to investigate the role of magnetic fields from the vicinity of the event horizon (as probed with the EHT on light-day scales) to far beyond the M87 galaxy along its powerful jets (as probed with ALMA on scales of thousand of light-years). The values in GHz refer to the frequencies of light at which the different observations were made. The horizontal lines show the scale (in light years) of each of the individual images. Credit: EHT Collaboration; ALMA (ESO/NAOJ/NRAO), Goddi et al.; NASA, ESA and the Hubble Heritage Team (STScI/AURA); VLBA (NRAO), Kravchenko et al.; J. C. Algaba, I. Martí-Vidal

IMAGE 4….This image shows a view of the jet in the Messier 87 (M87) galaxy in polarised light. The image was obtained with the Chile-based Atacama Large Millimeter/submillimeter Array (ALMA), in which ESO is a partner, and captures the part of the jet, with a size of 6000 light years, closer to the centre of the galaxy. The lines mark the orientation of polarisation, which is related to the magnetic field in the region imaged. This ALMA image therefore indicates what the structure of the magnetic field along the jet looks like. Credit: ALMA (ESO/NAOJ/NRAO), Goddi et al.

IMAGE 5….The Event Horizon Telescope (EHT) — a planet-scale array of eight ground-based radio telescopes forged through international collaboration — was designed to capture images of a black hole. In coordinated press conferences across the globe, EHT researchers revealed that they succeeded, unveiling the first direct visual evidence of the supermassive black hole in the centre of Messier 87 and its shadow. The shadow of a black hole seen here is the closest we can come to an image of the black hole itself, a completely dark object from which light cannot escape. The black hole’s boundary — the event horizon from which the EHT takes its name — is around 2.5 times smaller than the shadow it casts and measures just under 40 billion km across. While this may sound large, this ring is only about 40 microarcseconds across — equivalent to measuring the length of a credit card on the surface of the Moon. Although the telescopes making up the EHT are not physically connected, they are able to synchronize their recorded data with atomic clocks — hydrogen masers — which precisely time their observations. These observations were collected at a wavelength of 1.3 mm during a 2017 global campaign. Each telescope of the EHT produced enormous amounts of data – roughly 350 terabytes per day – which was stored on high-performance helium-filled hard drives. These data were flown to highly specialised supercomputers — known as correlators — at the Max Planck Institute for Radio Astronomy and MIT Haystack Observatory to be combined. They were then painstakingly converted into an image using novel computational tools developed by the collaboration. Credit: EHT Collaboration

IMAGE 6….Messier 87 (M87) is an enormous elliptical galaxy located about 55 million light years from Earth, visible in the constellation Virgo. It was discovered by Charles Messier in 1781, but not identified as a galaxy until 20th Century. At double the mass of our own galaxy, the Milky Way, and containing as many as ten times more stars, it is amongst the largest galaxies in the local universe. Besides its raw size, M87 has some very unique characteristics. For example, it contains an unusually high number of globular clusters: while our Milky Way contains under 200, M87 has about 12,000, which some scientists theorise it collected from its smaller neighbours. Just as with all other large galaxies, M87 has a supermassive black hole at its centre. The mass of the black hole at the centre of a galaxy is related to the mass of the galaxy overall, so it shouldn’t be surprising that M87’s black hole is one of the most massive known. The black hole also may explain one of the galaxy’s most energetic features: a relativistic jet of matter being ejected at nearly the speed of light. The black hole was the object of paradigm-shifting observations by the Event Horizon Telescope. The EHT chose the object as the target of its observations for two reasons. While the EHT’s resolution is incredible, even it has its limits. As more massive black holes are also larger in diameter, M87’s central black hole presented an unusually large target—meaning that it could be imaged more easily than smaller black holes closer by. The other reason for choosing it, however, was decidedly more Earthly. M87 appears fairly close to the celestial equator when viewed from our planet, making it visible in most of the Northern and Southern Hemispheres. This maximised the number of telescopes in the EHT that could observe it, increasing the resolution of the final image. This image was captured by FORS2 on ESO’s Very Large Telescope as part of the Cosmic Gems programme, an outreach initiative that uses ESO telescopes to produce images of interesting, intriguing or visually attractive objects for the purposes of education and public outreach. The programme makes use of telescope time that cannot be used for science observations, and  produces breathtaking images of some of the most striking objects in the night sky. In case the data collected could be useful for future scientific purposes, these observations are saved and made available to astronomers through the ESO Science Archive. Credit: ESO

IMAGE 7….This chart shows the position of giant galaxy Messier 87 in the constellation of Virgo (The Virgin). The map shows most of the stars visible to the unaided eye under good conditions. Credit: ESO, IAU and Sky & Telescope

IMAGE 8….This image shows the contribution of ALMA and APEX to the EHT. The left hand image shows a reconstruction of the black hole image using the full array of the Event Horizon Telescope (including ALMA and APEX); the right-hand image shows what the reconstruction would look like without data from ALMA and APEX. The difference clearly shows the crucial role that ALMA and APEX played in the observations. Credit: EHT Collaboration

IMAGE 9….This artist’s impression depicts the black hole at the heart of the enormous elliptical galaxy Messier 87 (M87). This black hole was chosen as the object of paradigm-shifting observations by the Event Horizon Telescope. The superheated material surrounding the black hole is shown, as is the relativistic jet launched by M87’s black hole. Credit: ESO/M. Kornmesser