Space

June 7, 2013

NASA’s Hubble maps 3-D structure of ejected material around erupting star

nasa-hubble
A flash of light from a stellar outburst has provided a rare look at the 3-D structure of material ejected by an erupting nova.

Astronomers used NASA’s Hubble Space Telescope to observe the light emitted by the close double-star system T Pyxidis, or T Pyx, a recurring nova, during its latest outburst in April 2011.

A nova erupts when a white dwarf, the burned-out core of a sun-like star, has siphoned off enough hydrogen from a companion star to trigger a thermonuclear runaway. As hydrogen builds up on the surface of the white dwarf, it becomes hotter and denser until it detonates like a colossal hydrogen bomb, leading to a 10,000-fold increase in brightness in a little more than one day. Nova explosions are extremely powerful, equal to a blast of one million billion tons of dynamite. T Pyx erupts every 12 to 50 years.

Contrary to some predictions, the astronomers were surprised to find the ejecta from earlier outbursts stayed in the vicinity of the star and formed a disk of debris around the nova. The discovery suggests material continues expanding outward along the system’s orbital plane, but it does not escape the system.

“We fully expected this to be a spherical shell,” says Arlin Crotts of Columbia University, a member of the research team. “This observation shows it is a disk, and it is populated with fast-moving ejecta from previous outbursts.”

Team member Stephen Lawrence of Hofstra University in Hempstead, N.Y., will present the results Tuesday at the American Astronomical Society meeting in Indianapolis.

Team member Jennifer Sokoloski, also of Columbia University and co-investigator on the project, suggests these data indicate the companion star plays an important role in shaping how material is ejected, presumably along the system’s orbital plane, creating the pancake-shaped disk. The disk is tilted about 30 degrees from face-on toward Earth.

Using Hubble’s Wide Field Camera 3, the team took advantage of the blast of light emitted by the erupting nova to trace the light’s path as it lit up the disk and material from previous ejecta. The disk is so vast, about a light-year across, that the nova’s light cannot illuminate all of the material at once. Instead, the light sweeps across the material, sequentially illuminating parts of the disk, a phenomenon called a light echo. The light reveals which parts of the disk are nearer to Earth and which sections are farther away. By tracing the light, the team assembled a 3-D map of the structure around the nova.

“We’ve all seen how light from fireworks shells during the grand finale will light up the smoke and soot from shells earlier in the show,” Lawrence said. “In an analogous way, we’re using light from T Pyx’s latest outburst and its propagation at the speed of light to dissect its fireworks displays from decades past.”

Although astronomers have witnessed light propagating through material surrounding other novae, this is the first time the immediate environment around an erupting star has been studied in three dimensions.

Astronomers have studied light echoes from other novae, but those phenomena illuminated interstellar material around the stars instead of material ejected from them.

The team also used the light echo to refine estimates of the nova’s distance from Earth. The new distance is 15,600 light-years from Earth. Previous estimates were between 6,500 and 16,000 light-years. T Pyx is located in the southern constellation Pyxis, or the Mariner’s Compass.

The team is continuing to analyze the Hubble data to develop an outflow model. T Pyx has a history of outbursts. Besides the 2011 event, other previous known eruptions were seen in 1890, 1902, 1920, 1944 and 1966.

Astronomers call erupting stars novae, Latin for “new,” because they abruptly appear in the sky. A nova quickly begins to fade in several days or weeks as the hydrogen is exhausted and blown into space.

The team also includes Helena Uthas of Columbia University. The team’s results will appear online Wednesday, June 5 and will be published in the June 20 issue of the Astrophysical Journal Letters. Sokoloski is the paper’s lead author.




All of this week's top headlines to your email every Friday.


 
 

 

Northrop Grumman’s AstroMesh reflector successfully deploys for NASA’s SMAP satellite

The NASA Jet Propulsion Laboratory successfully deployed the mesh reflector and boom aboard the Soil Moisture Active Passive spacecraft, a key milestone on its mission to provide global measurements of soil moisture. Launched Jan. 31, SMAP represents the future of Earth Science by helping researchers better understand our planet. SMAP’s unmatched data capabilities are enabled...
 
 
NASA photograph by Brian Tietz

NASA offers space tech grants to early career university faculty

NASA photograph by Brian Tietz Tensegrity research is able to simulate multiple forms of locomotion. In this image, a prototype tensegrity robot reproduces forward crawling motion. NASA’s Space Technology Mission Director...
 
 

NASA releases first global rainfall, snowfall map from new mission

Like a lead violin tuning an orchestra, the GPM Core Observatory – launched one year ago on Feb. 27, 2014, as a collaboration between NASA and the Japan Aerospace Exploration Agency – acts as the standard to unify precipitation measurements from a network of 12 satellites. The result is NASA’s Integrated Multi-satellite Retrievals for GPM...
 

 

New NASA Earth Science Missions expand view of our home planet

Four new NASA Earth-observing missions are collecting data from space with a fifth newly in orbit ñ after the busiest year of NASA Earth science launches in more than a decade. On Feb. 27, 2014, NASA and the Japan Aerospace Exploration Agency launched the Global Precipitation Measurement Core Observatory into space from Japan. Data from...
 
 

NASA, ESA telescopes give shape to furious black hole winds

NASA’s Nuclear Spectroscopic Telescope Array (NuSTAR) and ESA’s (European Space Agency) XMM-Newton telescope are showing that fierce winds from a supermassive black hole blow outward in all directions – a phenomenon that had been suspected, but difficult to prove until now. This discovery has given astronomers their first opportunity to measure the strength of these...
 
 
NASA photograph by Gary Banziger

Jurczyk named head of NASA Space Technology Mission Directorate

NASA photograph by Gary Banziger NASA’s Steve Jurczyck addresses an audience during a manufacturing event in Hampton, Va., last month. NASA Administrator Charles Bolden has named Steve Jurczyk as the agency’s Associ...
 




0 Comments


Be the first to comment!


Leave a Reply

Your email address will not be published. Required fields are marked *

You may use these HTML tags and attributes: <a href="" title=""> <abbr title=""> <acronym title=""> <b> <blockquote cite=""> <cite> <code> <del datetime=""> <em> <i> <q cite=""> <strike> <strong>