Tag Archives: Gaia

An artist's impression of a collision between the Milky Way and a smaller dwarf galaxy, such as that which occurred about eight to 10 billion years agoV. Belokurov (Cambridge, UK) based on an image by ESO/Juan Carlos Muñoz)

A dwarf galaxy may have collided with the Milky Way 3 billion years ago

Over twenty years ago astronomers first observed an unusually high density of stars in the vicinity of the Virgo cluster with the Milky Way, but until now the cause of the so-called Virgo Overdensity was unknown. New research suggests that this overdensity was actually caused by a dwarf galaxy plugging into the heart of the Milky Way over 3 billion years ago. But unlike in folklore when a wooden stake plunges through the heart of a vampire, it was this cosmic impaler that was destroyed by the interaction. 

The gravitational influence of the Milky Way ripped the dwarf galaxy apart leaving behind telltale shell-like formations of stars as the only evidence of the violent collision. Evidence that has now been uncovered by astronomers.

Two spiral galaxies (from left) NGC 2207 and IC 2163 colliding with one another. Credit: NASA.

“When we put it together, it was an ‘aha’ moment. This group of stars had a whole bunch of different velocities, which was very strange,” says Heidi Jo Newberg, the Rensselaer Institute professor of physics, applied physics, and astronomy, who led the team that made the discovery. “Now that we see their motion as a whole, we understand why the velocities are different, and why they are moving the way that they are.”

The team’s research is published in the latest edition of The Astrophysical Journal. They detail two shell-like structures in the Virgo Overdensity and a further pair in Hercules Aquila Cloud region. Their findings are based on data provided by the Sloan Digital Sky Survey, the European Space Agency’s Gaia space telescope, and the LAMOST telescope in China.

The Virgo Overdensity: Evidence of a Cosmic Collision

The Virgo Overdensity has, until now, been something of an oddity amongst such clusters. Star surveys have revealed that some of the stars that make up the Virgo Overdensity are moving toward us, whilst others are moving away. This is behaviour that would not normally be seen in a cluster of this kind. In 2019, researchers from the Rensselaer Institute had put forward the idea that this is because the overdensity is a result of a radial — or T-bone — collision.

The shell structures described in this new study — not observed before–seems to confirm this origin for the Virgo Overdensity. These arcs of stars — curved like umbrellas — are believed by the team to be the what remains of the dwarf galaxy after it was pulled apart by the Milky Way’s overpowering gravitational influence. 

an N-body simulation of a radial merger between the Milky Way Galaxy and a dwarf galaxy. Collisions like these create what are known as “shells” in the Galaxy’s halo (Thomas Donlon)

The process caused the dwarf galaxy to ‘bounce’ through the centre of the Milky Way with its stars being gradually incorporated into our galaxy. Each time the dwarf galaxy passed through the Milky Way’s centre the stars would initially move quickly, gradually being slowed by the gravity of our galaxy, until this influence eventually pulls them back. Each time the dwarf galaxy ‘threaded back’ through the centre a new shell was created. 

Counting the number of shells allowed the team to calculate how many cycles the dwarf galaxy has undergone which in turn allows them to estimate how many years it has been since the collision — which they are naming the ‘Virgo Radial Merger’ —  took place. Thus the team dates the first passage of the dwarf galaxy through the centre of the Milky Way at 2.7 billion years ago. 

The Immigrant’s Song

Lead author Newberg believes that the majority of the stars in the Milky Way’s halo — a spherical cloud of stellar bodies that surround our galaxy’s spiral arms — appear to be ‘immigrants’ that formed in smaller galaxies and deposited by collisions different from the radial merger described above. 

The researcher, who specialises in the Milky Way’s stellar halo, says that as dwarf galaxies were absorbed into the Milky Way, ensuing tidal forces pulled their stars into long cords moving in unison through the halo. These are so-called tidal mergers which are both less violent and far more common than radial collisions. 

The fact that radial mergers are uncommon means the team was slightly taken back by the discovery of such evidence in the centre of the Milky Way. It was only as the team began to model the movement of the Virgo Overdensity that the significance of their discovery began to dawn on them. 

The Gaia Sausage–the team’s findings imply this colourfully named cluster of stars was not created in the same event that created the Virgo Overdensity, or that it is much younger than previously believed (ESA/Gaia. this image was prepared by Edmund Serpell, a Gaia Operations Engineer working in the Mission Operations Centre at ESA’s European Space Operations Centre in Darmstadt, Germany. CC by SA 3.0)

“There are other galaxies, typically more spherical galaxies, that have a very pronounced shell structure, so you know that these things happen, but we’ve looked in the Milky Way and hadn’t seen really obvious gigantic shells,” explains Thomas Donlon II, a Rensselaer graduate student and first author of the paper. “And then we realized that it’s the same type of merger that causes these big shells. It just looks different because, for one thing, we’re inside the Milky Way, so we have a different perspective, and also this is a disk galaxy and we don’t have as many examples of shell structures in disk galaxies.”

In addition to pointing towards the radial collision almost 3 billion years ago, the team’s research has potential implications for other stellar phenomena. In particular, the findings indicate that the ‘Gaia Sausage’ — a formation that astronomers believe is the result of a collision with a dwarf galaxy between 8 and 11 billion years ago — was not created by the same event that created the Virgo Overdesity, as scientists had previously believed.

The team’s findings clearly imply that the Virgo Overdensity is much younger than the Gaia Sausage meaning that the two had different origins, or that the colourfully named ‘sausage’ is fresher than previously believed. This would also mean that it could not have caused the thick central disc stars at the centre of the Milky Way.

“There are lots of potential tie-ins to this finding,” concludes Newberg. “The Virgo Radial Merger opens the door to a greater understanding of other phenomena that we see and don’t fully understand, and that could very well have been affected by something having fallen right through the middle of the galaxy less than 3 billion years ago.”

ESA’s Gaia observatory sends back first star chart showing a billion new stars

The team working with the Gaia space telescope has just released the first batch of the data they’ve recorded — and it’s huge. The craft has seen over a billion stars and measured the distance to and sideways motion of two million of them.

Gaia’s first star map.

Gaia is ESA’s space observatory launched in December 2013 — the best craft of its kind humanity has ever constructed. Its mapping efforts are still several years to completion but the data it beamed back is on a scale far greater than anything we’ve had access to before. On Wednesday, ESA released a huge set of data comprising 1.1 billion light sources. Out of these, roughly 400 million are objects never before recorded.

“You’re imaging the whole sky in basically [Hubble] space telescope quality and because you can now resolve all the stars that previously maybe looked as though they were merged as one star at low resolution – now we can see them,” explained Anthony Brown from Leiden University, Netherlands.

“Gaia is going to be a revolution,”  said Gerry Gilmore from Cambridge University, UK, was one of the mission’s proposers. “It’s as if we as astronomers have been bluffing up until now. We’re now going to see the truth.”

The treasure trove of data is so huge that scientists say they won’t to be able to analyze all of it — so they’re appealing to the public to join in and discover the great unknown.  A web page has been created where anyone can play with Gaia data and look for novel phenomena.

Gaia’s goal was to improve on the work of Hipparcos, the first high-precision astrometry satellite, launched in 1989. At the time Hipparcos’ catalogue of the Milky Way became the go-to chart of this corner of the Universe, detailing the precise position, brightness, distance to and proper motion of 100,000 stars. Gaia increased that number twenty-fold — and this is only the first part of the data.

Astrometry is the art of calculating the position and movement of celestial bodies hundreds, thousands, even millions of light years away starting from distances we can measure — the distance between two points on Earth’s orbit, for example. As our planet orbits the Sun, relatively nearby stars seem to move against the seemingly fixed stars farther away. So, we can use the parallax angle to calculate the distance to these target stars.

Because the ratio between the distances we know and those we’re calculating is so huge these angles are tiny — under one arcsecond (1/60 of a degree) for the nearest stars. Parallax measurements are used as references to correct more indirect techniques of measuring these huge distances, so Gaia is programmed to take repeated measurements for each star to reduce errors to under seven micro-arcseconds — an error the size of a one euro coin on a Moon-Earth distance.

The craft carries two sets of optical telescopes, which project their light on a one-billion-pixel camera detector connected to a trio of instruments. This technological fortitude allows Gaia to pick out stars more accurately than anything we’re ever constructed before. It uses all this information to measure details such as the temperature and composition of the stars, which can be used to determine their age.

Getting an accurate reading over such distances is tricky, so repeated viewings of each point are required.

All in all, the mission is expected to take five years to complete but once over it’s estimated Hipparcos’ 100,000-strong catalogue will expand to over one billion objects. But after seeing the data it became apparent that Gaia is picking up many more faint light sources that we’ve anticipated, so that number could climb as high as two to three billion objects.

Not all of these will be actual stars. Quasars, planets, distant galaxies — they’re all here. In particular, by looking at how the stars Gaia picked up “wobble” through the sky, astronomers can predict the existence of worlds orbiting them.

“Gaia is going to be extremely useful for exoplanets, and especially systems that have the Jupiter kind of planets,” said Esa’s Gaia project scientist, Timo Prusti.

“The numbers are going to be impressive; we expect 20,000. The thing is, you need patience because the exoplanets are something where you have to collect five years of data to see the deviation in the movements.”

Another goal of the Gaia mission is to measure the radial velocity of stars — the movement they make towards or away from the craft as they move around the galaxy. Compare this with the stars’ proper motion, and it will give us a glimpse into the dynamics of the Milky Way.

Image credits ESA.

Before the mission’s launch, scientists had hoped to get radial velocity data on about 150 million stars. Soon after the satellite’s launch, however, scientists realized that there was a lot of stray light reaching the camera, which impaired its observation of the faintest stars and their colors. Engineers think this is caused in part by the way sunlight bends past the 10m-diameter shade that Gaia uses to keep its telescopes shaded. They say that the more time the mission runs, the closer Gaia will get to its target.

“Clearly, with the stray light we lost sensitivity. On the other hand, it happens to be that there are more stars than were thought before. So we’re still talking about 100 million radial velocities,” Timo Prusti told BBC News.