Hubble Uncovers Clues to the Formation and Evolution of the Milky Way

In the embers of once vibrant white dwarf stars in the central bulge of the galaxy

NASA's Hubble Space Telescope has detected for the first time a population of white dwarfs embedded in the hub of our Milky Way galaxy. The Hubble images are the deepest, most detailed study of the galaxy's central bulge of stars. The smoldering remnants of once-vibrant stars can yield clues to our galaxy's early construction stages that happened long before Earth and our sun formed. [Left] — This is a ground-based view of the Milky Way’s central bulge, seen in the direction of the constellation Sagittarius. Giant dust clouds block most of the starlight coming from the galactic center. Hubble, however, peered through a region (marked by the arrow) called the Sagittarius Window, which offers a keyhole view into the galaxy's hub. [Upper right] — This is a small section of Hubble's view of the dense collection of stars crammed together in the galactic bulge. The region surveyed is part of the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) field and is located 26,000 light-years away. [Lower right] — Hubble uncovered extremely faint and hot white dwarfs. This is a sample of 4 out of the 70 brightest white dwarfs spied by Hubble in the Milky Way's bulge. Astronomers picked them out based on their faintness, blue-white color, and motion relative to our sun. The numbers in the inset images correspond to the white dwarfs' location in the larger Hubble view. Image: NASA/ESA
NASA’s Hubble Space Telescope has detected for the first time a population of white dwarfs embedded in the hub of our Milky Way galaxy. The Hubble images are the deepest, most detailed study of the galaxy’s central bulge of stars. The smoldering remnants of once-vibrant stars can yield clues to our galaxy’s early construction stages that happened long before Earth and our sun formed.
[Left] — This is a ground-based view of the Milky Way’s central bulge, seen in the direction of the constellation Sagittarius. Giant dust clouds block most of the starlight coming from the galactic center. Hubble, however, peered through a region (marked by the arrow) called the Sagittarius Window, which offers a keyhole view into the galaxy’s hub.
[Upper right] — This is a small section of Hubble’s view of the dense collection of stars crammed together in the galactic bulge. The region surveyed is part of the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) field and is located 26,000 light-years away.
[Lower right] — Hubble uncovered extremely faint and hot white dwarfs. This is a sample of 4 out of the 70 brightest white dwarfs spied by Hubble in the Milky Way’s bulge. Astronomers picked them out based on their faintness, blue-white color, and motion relative to our sun. The numbers in the inset images correspond to the white dwarfs’ location in the larger Hubble view.
Image: NASA/ESA

Space news (December 08, 2015) – Looking through a cosmic keyhole 26,000 light-years away in Sagittarius

Astronomers trying to understand the formation and evolution of the Milky Way by studying the first stars to be born in the galaxy have a problem. The stars within the central bulge of the galaxy formed first according to stellar theory. Unfortunately, the light from these suns is blocked by massive clouds of gas and dust, which makes studying their role in the formation and evolution of the Milky Way difficult. 

In order to view the central bulge of the galaxy, astronomers looked through a small keyhole in the sky, called the Sagittarius Window. Making it possible to study the formation and evolution of the Milky Way and galaxies as a whole by comparison. A view giving us a look into the very heart of the galaxy and the blueprints nature uses to construct these island universes.

Current astronomical theory believes the central bulge of the Milky Way grew first, followed by the relatively quick birth of the stars making up the rest of the galaxy. Peering deep into the heart of the central bulge, astronomers have discovered a family of 70 ancient white dwarf stars, they believe are the smoldering remnants of once-vibrant suns that inhabited the core long ago. Ancient stars scientists are studying to uncover clues to the processes that formed the Milky Way and by relation the family of galaxies in the cosmos. Marking the deepest, most detailed archeological study of the central bulge of the Milky Way and by extension its formation and evolution.

These ancient white dwarf stars hold the keys to opening the door to better understanding the history of the Milky Way. To gaining knowledge and facts concerning 12 billion-year-old suns that existed when the galaxy was young. Knowledge and facts giving astronomers clues to the early years and evolution of the Milky Way and the billions of island universes in the cosmos.

This is a close up of ancient white dwarfs inhabiting the bulge of the Milky Way.
This is a close up of ancient white dwarfs inhabiting the bulge of the Milky Way. Image NASA/ESA

It is important to observe the Milky Way’s bulge because it is the only bulge we can study in detail,” explained Annalisa Calamida of the Space Telescope Science Institute (STScI) in Baltimore, Maryland, the science paper’s lead author. “You can see bulges in distant galaxies, but you cannot resolve the very faint stars, such as the white dwarfs. The Milky Way’s bulge includes almost a quarter of the galaxy’s stellar mass. Characterizing the properties of the bulge stars can then provide important information to understanding the formation of the entire Milky Way galaxy and that of similar, more distant galaxies.”

The Hubble survey also found slightly more low-mass stars in the bulge, compared to those in the galaxy’s disk population. This result suggests that the environment in the bulge may have been different than the one in the disk, resulting in a different star-formation mechanism,” Calamida said.

Astronomers have only looked at about 70 of the hottest white dwarfs Hubble can pick out of at least 70 thousand stars in the small area of the bulge of the Milky Way they looked at. White dwarf stars detected by making extremely precise measurements of the motion of over 240,000 stars they detected over a decade of viewing as part of the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS). Precise measurements astronomers used to determine which stars are disk stars or suns inhabiting the bulge of our galaxy. Stars that inhabit the bulge move at a different rate than suns in the disk of the galaxy as compared to our Sun. Extremely hot white dwarfs are also slightly bluer relative to stars like our own sun and they become fainter and cooler as they age. Facts that allowed Hubble’s Advanced Camera for Surveys to pick out 70 of the brightest white dwarf stars inhabiting the bulge of the Milky Way.

Comparing the positions of the stars from now and 10 years ago we were able to measure accurate motions of the stars,” said Kailash Sahu of STScI, and the study’s leader. “The motions allowed us to tell if they were disk stars, bulge stars, or halo stars.”

These 70 white dwarfs represent the peak of the iceberg,” Sahu said. “We estimate that the total number of white dwarfs is about 100,000 in this tiny Hubble view of the bulge. Future telescopes such as NASA’s James Webb Space Telescope will allow us to count almost all of the stars in the bulge down to the faintest ones, which today’s telescopes, even Hubble, cannot see.”

The team’s going back to work

This team of intrepid astronomers and scientists now plan to increase the sample size of the white dwarfs currently being studied. This will be done by analyzing additional parts of the SWEEPS field of study, which they hope to use to get more precise measurements of the exact age of the bulge of the Milky Way. They’ll also take a look at the possibility the star formation processes used to create the bulge billions of years ago, could be slightly different than current star formation processes at work in the younger disk of the galaxy.

You can learn more about the Hubble Space Telescope here.

Read and learn about white dwarf stars here.

Read about the discoveries of the Space Telescope Science Institute (STScI) here.

Learn more about the formation and evolution of the Milky Way here.

Read about the discoveries of the Sagittarius Window Eclipsing Extrasolar Planet Search (SWEEPS) here.

Read about five Explorer Program missions recently selected by NASA.

Learn more about galactic nurseries where stars are born.

Read about the first Earth-sized exoplanet found orbiting in the habitable zone of its home star.

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The Greater the Mass, the Bigger the Pull

In the battle between celestial masses, greater mass means a bigger pull, and usually survival of the more massive body 

Space scientists looking a possible sources for a new x-ray source detected in globular cluster NGC 6388 are not on the trail of a cosmic mystery.
Space scientists looking a possible sources for a new x-ray source detected in globular cluster NGC 6388 are hot on the trail of a cosmic mystery.

Space news (April 28, 2015)

– A cosmic mystery unfolds 43,000 light years away in globular cluster NGC 6388

NASA space scientists studying the source of x-rays emanating from a globular cluster on the edge of the Milky Way are on the trail of a cosmic mystery.

Evidence seems to indicate x-rays were created as hot gas was drawn into the intermediate-mass black hole space scientists believe resides at the center of globular cluster NGC 6388.

Taking a closer look at data obtained using the European Space Agency’s INTErnational Gamma-Ray Laboratory (INTEGRAL), and NASA’s Chandra X-ray Observatory and Swift Gamma-Ray Burst Explorer revealed the x-rays emanated from a location slightly off to one side of the center of NGC 6388.

Where does this cosmic mystery lead?

Space scientists looking at theoretical simulations and the data obtained observing the x-ray source for 200 days now believe x-rays were created as a planet, one-third the mass of Earth, was ripped apart as it came to close to a white dwarf star roughly the size of our planet.

In the movie
In the movie “When Worlds Collide”, the star Bellus is on a collision course with Earth.

How could a body the size of Earth pull apart a planet estimated to be one-third the mass?

A white dwarf star is the remnant of a medium-mass star, similar to our own Sun. In this case, space scientists estimate the white dwarf star was about 1.4 times the mass of our Sun, which means its surface gravity would be over 10,000 times stronger.

As a body thirty-three percent of the mass of Earth travels near a white dwarf star with a surface gravity of this magnitude, space scientists simulations indicate the difference in gravitational forces between the far and near side of the body creates gravitational tides that are greatly enhanced due to the nearness and magnitude of gravitational forces involved.

Space scientists indicate computer simulations suggest a planet would be first pulled away from its parent star due to the gravitational force created by the dense concentration of stars near the center of globular cluster NGC 6388.

If this planet were to pass near a white dwarf star with a mass close to the one in this news story, computer simulations indicate it could be torn apart by extreme tidal forces created as it passes.

The planetary debris created is then heated and glows in x-rays as it falls into the gravitational field of the white dwarf.

In this case, the observed amount of x-rays is as computer simulations indicate should be detected, so space scientists think they’re at least on the right trail. They’re now going over the data obtained and conducting new experiments to eliminate other possible x-ray sources.

For more information on NASA’s space mission visit here.

Learn more about the Chandra X-ray Observatory here.

Discover more about the mission of the European Space Agency’s INTErnational Gamma-Ray Laboratory (INTEGRAL) here.

For more information concerning the Swift Gamma-Ray Burst Explorer visit here.

Learn more about stars similar to our Sun.

Learn more about the possible evolution of life during the early universe.

Learn more about the human desire to travel to Mars.