These images show evidence for an exhaust vent attached to a chimney releasing hot gas from a region around the supermassive black hole at the center of the Milky Way, as reported in our latest press release. In the main image of this graphic, X-rays from NASA’s Chandra X-ray Observatory (blue) have been combined with radio data from the MeerKAT telescope (red).

Previously, astronomers had identified a “chimney” of hot gas near the Galactic Center using X-ray data from Chandra and ESA’s XMM-Newton. Radio emission detected by MeerKAT shows the effect of magnetic fields enclosing the gas in the chimney.

The evidence for the exhaust vent is highlighted in the inset, which includes only Chandra data. Several X-ray ridges showing brighter X-rays appear in white, roughly perpendicular to the plane of the Galaxy. Researchers think these are the walls of a tunnel, shaped like a cylinder, which helps funnel hot gas as it moves upwards along the chimney and away from the Galactic Center.

We welcome Orsolya Eszter Kovács, a postdoctoral fellow at Masaryk University, Czechia, as our guest blogger. She spent over two years at the Smithsonian Astrophysical Observatory as a pre-doctoral fellow while working on the PhD she obtained from Eötvös Loránd University, Hungary. She is the first author of a recent paper presenting one of the most distant supermassive black holes ever seen.

In the past six months¹ Chandra has unveiled two supermassive black holes remarkably close to their formation epoch, only about 500 million years after the big bang. These findings mark some of the most distant supermassive black holes observed to date.

Supermassive black holes, the largest type of black holes, lurk in the heart of most big galaxies. These cosmic behemoths play a central role in the formation and evolution of their hosting galaxies, exerting influence so significant that they can even suppress star formation.

The origin of these giant black holes is a subject of debate. Do they originate from the collapse of the earliest stellar population, known as Population III stars? Although it seems like an obvious explanation, to reach those immense masses observed in their later stages, these “light black hole seeds” need to be fed with an extreme amount of matter in a relatively brief period (through a process that astronomers call “accretion”). Yet, such a high accretion rate seems improbable as a universal solution, because there are physical limits on how quickly material can fall inwards. The outwards pressure from the intense radiation associated with high accretion can overcome the gravitational forces pulling material inwards, causing the material to be pushed away instead.

New movies of two of the most famous objects in the sky — the Crab Nebula and Cassiopeia A — are being released from NASA’s Chandra X-ray Observatory. Each includes X-ray data collected by Chandra over about two decades. They show dramatic changes in the debris and radiation remaining after the explosion of two massive stars in our galaxy.

The Crab Nebula, the result of a bright supernova explosion seen by Chinese and other astronomers in the year 1054, is 6,500 light-years from Earth. At its center is a neutron star, a super-dense compact object produced by the supernova. As it rotates at about 30 times per second, its beam of radiation passes over the Earth every rotation, like a cosmic lighthouse.

As the young pulsar slows down, large amounts of energy are injected into its surroundings. In particular, a high-speed wind of matter and anti-matter particles plows into the surrounding nebula, creating a shock wave that forms the ring seen in the movie. Jets from the poles of the pulsar spew X-ray emitting matter and antimatter particles in a direction perpendicular to the ring.

The Chandra Source Catalog (CSC) is the definitive catalog of X-ray sources detected by the observatory. The latest version, known as CSC 2.1, was released in early April 2024.

Since the Uhuru satellite in the 1970s, X-ray astrophysics missions have a tradition of publishing detailed catalogs of the X-ray sources detected along with a list of key physical properties.

CSC 2.1. carries this tradition forward. Below is an adapted announcement from members of the team who worked on this important resource for the scientific community:

The Chandra X-ray Center (CXC) is pleased to announce the availability of Release 2.1 of the Chandra Source Catalog (CSC 2.1). This catalog covers roughly 730 square degrees of sky and contains 407,806 unique X-ray sources and over 1.3 million individual source detections identified in more than 15,000 Chandra imaging observations released publicly prior to the end of 2021.

The following press release from Brown University, being released in conjunction with another from the Smithsonian Institution, highlights an exciting new project that brings cosmic objects in 3D to Instagram “experiences.” This project was led by Dr. Kimberly Arcand of the Smithsonian Astrophysical Observatory that runs the Chandra X-ray Center on behalf of NASA. These new Chandra Instagram experiences are the first ever to include sonifications (translations of data into sound) and represent a new way of making astronomical data more accessible.

By using a phone camera and a new set of Instagram augmented reality filters, anyone can dive into the depths of space, encountering nebulae, pulsars and even remnants of exploded stars.

Gaze at the ethereal colors of distant nebulae. Zoom in to the heart of an exploded star. Listen to chimes, bells and electric rhythms representing a celestial object far off in space. Through new Instagram filters, users of the app can now embark on cosmic journeys through their smartphones with space-themed augmented reality experiences.

The filters are fun, for sure — but they’re also grounded in some serious science. The experiences were created by researchers from Brown University, Smithsonian Astrophysical Observatory and NASA to celebrate the 25th anniversary the Chandra spacecraft, NASA’s flagship X-ray telescope. The goals are to engage the public, make images of space more accessible and add new layers of understanding to some of the most well-known and widely studied objects in the sky.

In the year 1181 a rare supernova explosion appeared in the night sky, staying visible for 185 consecutive days. Historical records show that the supernova looked like a temporary ‘star’ in the constellation Cassiopeia shining as bright as Saturn.

Ever since, scientists have tried to find the supernova’s remnant. At first it was thought that this could be the nebula around the pulsar — the dense core of a collapse star — named 3C 58. However closer investigations revealed that the pulsar is older than supernova 1181.

In the last decade, another contender was discovered; Pa 30 is a nearly circular nebula with a central star in the constellation Cassiopeia. It is pictured here combining images from several telescopes. This composite image uses data across the electromagnetic spectrum and shows a spectacular new view of the supernova remnant. This allows us to marvel at the same object that appeared in our ancestors’ night sky more than 800 years ago.

This image shows a quasar, a rapidly growing supermassive black hole, which is not achieving what astronomers would expect from it, as reported in our latest press release. Data from NASA’s Chandra X-ray Observatory (blue) and radio data from the NSF’s Karl G. Jansky’s Very Large Array (red) reveal some of the evidence for this quasar’s disappointing impact on its host galaxy.

Known as H1821+643, this quasar is about 3.4 billion light-years from Earth. Quasars are a rare and extreme class of supermassive black holes that are furiously pulling material inwards, producing intense radiation and sometimes powerful jets. H1821+643 is the closest quasar to Earth in a cluster of galaxies.

Quasars are different than other supermassive black holes in the centers of galaxy clusters in that they are pulling in more material at a higher rate. Astronomers have found that non-quasar black holes growing at moderate rates influence their surroundings by preventing the intergalactic hot gas from cooling down too much. This regulates the growth of stars around the black hole.

Three new sonifications of images from NASA’s Chandra X-ray Observatory and other telescopes have been released. This work is also being featured in a new NASA+ documentary, "Listen to the Universe."

Sonification is the process of translating data into sounds. In the case of Chandra and other telescopes, scientific data are collected from space as digital signals that are commonly turned into visual imagery. The sonification project takes these data through another step of mapping the information into sound.