Eta Carinae Time-Lapse: 1999, 2003, 2009, 2014, and 2020
Credit: X-ray: NASA/SAO/GSFC/M. Corcoran et al; HST: NASA/ESA/STScI
Image Processing: NASA/CXC/SAO/L. Frattare, J. Major, N. Wolk
Credit: X-ray: NASA/SAO/GSFC/M. Corcoran et al; HST: NASA/ESA/STScI
Image Processing: NASA/CXC/SAO/L. Frattare, J. Major, N. Wolk
A new movie made from over two decades of data from NASA’s Chandra X-ray Observatory shows a famous star system changing with time, as described in our latest press release. Eta Carinae contains two massive stars (one is about 90 times the mass of the Sun and the other is believed to be about 30 times the Sun’s mass).
In the middle of the 19th century, skywatchers observed as Eta Carinae experienced a huge explosion that was dubbed the “Great Eruption.” During this event, Eta Carinae ejected between 10 and 45 times the mass of the Sun. This material became a dense pair of spherical clouds of gas, now called the Homunculus nebula, on opposite sides of the two stars. The Homunculus is clearly seen in a composite image of the Chandra data with optical light from the Hubble Space Telescope (blue, purple, and white).
Eta Carinae (Composite)
Credit: X-ray: NASA/SAO/GSFC/M. Corcoran et al; HST: NASA/ESA/STScI;
Image Processing: NASA/CXC/SAO/L. Frattare, J.Major, N. Wolk
Eta Carinae (Summed)
Credit:NASA/SAO/GSFC/M. Corcoran et al.
Visual Description:
Fast Facts for Eta Carinae (Time-lapse):
Credit: X-ray: NASA/SAO/GSFC/M. Corcoran et al.; Image Processing: L. Frattare, J. Major, N. Wolk (SAO/CXC)
Scale: Image is about 2.2 arcmin (4.8 light-years) across.
Category: Normal Stars & Star Clusters
Coordinates (J2000): RA 10h 45m 04s | Dec -59° 41´ 03"
Constellation: Carina
Observation Dates: 17 observations from Sept 1999 to March 2020
Observation Time: 79 hours 41 minutes (3 days 7 hours 41 minutes)
Obs. ID: 50, 51, 1249, 4455, 9933-9937, 16509, 15731, 15732, 16510, 15733, 16511, 22312, 22313
Instrument: ACIS
References: Corcoran, M. et al, ApJ, 2022, 937, 122. DOI 10.3847/1538-4357/ac8f27
Color Code: X-ray: red, green, and blue
Distance Estimate: About 7,500 light-years
In the middle of the 19th century, skywatchers observed as Eta Carinae experienced a huge explosion that was dubbed the “Great Eruption.” During this event, Eta Carinae ejected between 10 and 45 times the mass of the Sun. This material became a dense pair of spherical clouds of gas, now called the Homunculus nebula, on opposite sides of the two stars. The Homunculus is clearly seen in a composite image of the Chandra data with optical light from the Hubble Space Telescope (blue, purple, and white).
Credit: X-ray: NASA/SAO/GSFC/M. Corcoran et al; HST: NASA/ESA/STScI;
Image Processing: NASA/CXC/SAO/L. Frattare, J.Major, N. Wolk
A new time-lapse sequence contains frames
of Eta Carinae taken with Chandra from 1999, 2003, 2009, 2014, and
2020. Astronomers used the Chandra observations along with data from
ESA’s XMM-Newton to watch as the stellar eruption from about 180 years
ago continues to expand into space at speeds up to 4.5 million miles per
hour. The two massive stars produce the blue, relatively high energy X-ray source in the center of the ring. They are too close to each other to be seen individually.
A bright ring of X-rays (orange) around the Homunculus nebula was discovered about 50 years ago and studied in previous Chandra work. The new movie of Chandra, plus a deep, summed image generated by adding the data together, reveal important hints about Eta Carinae’s volatile history. This includes the rapid expansion of the ring, and a previously-unknown faint shell of X-rays outside it.
This faint X-ray shell is highlighted in an additional graphic showing the summed image. The image on the left emphasizes the bright X-ray ring, and the image on the right shows the same data but emphasizing the faintest X-rays. The shell is located in between the two contour levels, as labeled.
A bright ring of X-rays (orange) around the Homunculus nebula was discovered about 50 years ago and studied in previous Chandra work. The new movie of Chandra, plus a deep, summed image generated by adding the data together, reveal important hints about Eta Carinae’s volatile history. This includes the rapid expansion of the ring, and a previously-unknown faint shell of X-rays outside it.
This faint X-ray shell is highlighted in an additional graphic showing the summed image. The image on the left emphasizes the bright X-ray ring, and the image on the right shows the same data but emphasizing the faintest X-rays. The shell is located in between the two contour levels, as labeled.
Credit:NASA/SAO/GSFC/M. Corcoran et al.
Because the newly discovered outer X-ray shell has a similar shape
and orientation to the Homunculus nebula, researchers concluded both
structures have a common origin.
The idea is that material was blasted away from Eta Carinae well before
the 1843 Great Eruption — sometime between 1200 and 1800, based on the
motion of clumps of gas previously seen in Hubble Space Telescope data.
Later this slower material was lit up in X-rays when the fast blast wave
from the Great Eruption tore through space, colliding with and heating
the material to millions of degrees to create the bright X-ray ring. The
blast wave has now traveled beyond the bright ring.
A paper describing these results appeared in The Astrophysical Journal and is available at https://iopscience.iop.org/article/10.3847/1538-4357/ac8f27
The authors of the paper are Michael Corcoran (NASA’s Goddard Space Flight Center), Kenji Hamaguchi (GSFC), Nathan Smith (University of Arizona), Ian Stevens (University of Birmingham, UK), Anthony Moffat (University of Montreal), Noel Richardson (Embry-Riddle Aeronautical University), Gerd Weigelt (Max Planck Institute for Radio Astronomy), David Espinoza-Galeas (The Catholic University of America), Augusto Damineli (University of Sao Paolo, Brazil), and Christopher Russell (Catholic University).
NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
A paper describing these results appeared in The Astrophysical Journal and is available at https://iopscience.iop.org/article/10.3847/1538-4357/ac8f27
The authors of the paper are Michael Corcoran (NASA’s Goddard Space Flight Center), Kenji Hamaguchi (GSFC), Nathan Smith (University of Arizona), Ian Stevens (University of Birmingham, UK), Anthony Moffat (University of Montreal), Noel Richardson (Embry-Riddle Aeronautical University), Gerd Weigelt (Max Planck Institute for Radio Astronomy), David Espinoza-Galeas (The Catholic University of America), Augusto Damineli (University of Sao Paolo, Brazil), and Christopher Russell (Catholic University).
NASA's Marshall Space Flight Center manages the Chandra program. The Smithsonian Astrophysical Observatory's Chandra X-ray Center controls science operations from Cambridge, Massachusetts, and flight operations from Burlington, Massachusetts.
Source: NASA's Chandra X-Ray Observatory
Visual Description:
This release features composite images and a time-lapse movie of a
cosmic explosion that sky watchers have been observing since the middle
of the 19th century. About 180 years ago, a huge explosion inside the
Eta Carinae star system ejected massive amounts of material in an event
dubbed the "Great Eruption". The resulting gas and debris cloud has been
expanding ever since.
The time lapse sequence of Chandra observations begins with an image from 1999. Here, a hazy, neon blue ball with a brilliant white core is encircled by a patchy, oblong, orange ring. The blue and white ball shows X-rays from two massive stars, 30 and 90 times the mass of our sun. These stars are too close together to be seen individually. The oblong orange gas ring encircling them is tilted, stretching toward our upper right and lower left.
The time lapse movie progresses with four similar images, containing data from 2003, 2009, 2014, and 2020. As the images flit by, one after the other, the neon blue ball expands, but the white core appears stable. The patches forming the orange ring of gas shift and swell, moving away from the stars inside the blue and white ball.
An additional composite image features optical and X-ray observations of the explosion, inside the expanding orange ring of gas. Here, the explosion is shaped like an hourglass, or peanut shell, with bulbous ends and a narrow middle. The shell is a translucent mauve color, streaked with purple veins. Inside, at the narrow middle, a brilliant white light gleams brightly. The peanut shell shape is tilted, with one bulbous end pointing away from us, toward our upper right, and the other pointing toward us, down to our lower left. This is the same orientation as the orange ring of gas. That indicates that both structures have the same origin: the "Great Eruption", observed about 180 years ago.
The time lapse sequence of Chandra observations begins with an image from 1999. Here, a hazy, neon blue ball with a brilliant white core is encircled by a patchy, oblong, orange ring. The blue and white ball shows X-rays from two massive stars, 30 and 90 times the mass of our sun. These stars are too close together to be seen individually. The oblong orange gas ring encircling them is tilted, stretching toward our upper right and lower left.
The time lapse movie progresses with four similar images, containing data from 2003, 2009, 2014, and 2020. As the images flit by, one after the other, the neon blue ball expands, but the white core appears stable. The patches forming the orange ring of gas shift and swell, moving away from the stars inside the blue and white ball.
An additional composite image features optical and X-ray observations of the explosion, inside the expanding orange ring of gas. Here, the explosion is shaped like an hourglass, or peanut shell, with bulbous ends and a narrow middle. The shell is a translucent mauve color, streaked with purple veins. Inside, at the narrow middle, a brilliant white light gleams brightly. The peanut shell shape is tilted, with one bulbous end pointing away from us, toward our upper right, and the other pointing toward us, down to our lower left. This is the same orientation as the orange ring of gas. That indicates that both structures have the same origin: the "Great Eruption", observed about 180 years ago.
Fast Facts for Eta Carinae (Time-lapse):
Credit: X-ray: NASA/SAO/GSFC/M. Corcoran et al.; Image Processing: L. Frattare, J. Major, N. Wolk (SAO/CXC)
Scale: Image is about 2.2 arcmin (4.8 light-years) across.
Category: Normal Stars & Star Clusters
Coordinates (J2000): RA 10h 45m 04s | Dec -59° 41´ 03"
Constellation: Carina
Observation Dates: 17 observations from Sept 1999 to March 2020
Observation Time: 79 hours 41 minutes (3 days 7 hours 41 minutes)
Obs. ID: 50, 51, 1249, 4455, 9933-9937, 16509, 15731, 15732, 16510, 15733, 16511, 22312, 22313
Instrument: ACIS
References: Corcoran, M. et al, ApJ, 2022, 937, 122. DOI 10.3847/1538-4357/ac8f27
Color Code: X-ray: red, green, and blue
Distance Estimate: About 7,500 light-years
