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5 images found for "nustar, xmm-newton"
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This image taken by the ultraviolet-light monitoring camera on the European Space Agency's (ESA's) XMM-Newton telescope shows the beautiful spiral arms of the galaxy NGC1365.
This image taken by the ultraviolet-light monitoring camera on the European Space Agency's (ESA's) XMM-Newton telescope shows the beautiful spiral arms of the galaxy NGC1365.

NuSTAR's Improved View
This image taken by the ultraviolet-light monitoring camera on the European Space Agency's (ESA's) XMM-Newton telescope shows the beautiful spiral arms of the galaxy NGC1365.

Target:
Mission: NuSTAR, XMM-Newton
Spacecraft:
Instrument:
Size: 3000 x 2400
ID#: PIA16699
Added: 2013-02-27

Views: 644

NuSTAR's Improved View

This image taken by the ultraviolet-light monitoring camera on the European Space Agency's (ESA's) XMM-Newton telescope shows the beautiful spiral arms of the galaxy NGC1365.

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NASA's NuSTAR, has helped to show that the spin rates of black holes can be measured conclusively. The solid lines show two theoretical models that explain low-energy X-ray emission seen previously from the spiral galaxy NGC 1365 by XMM-Newton.
NASA's NuSTAR, has helped to show that the spin rates of black holes can be measured conclusively. The solid lines show two theoretical models that explain low-energy X-ray emission seen previously from the spiral galaxy NGC 1365 by XMM-Newton.

Two X-Ray Observatories are Better Than One
NASA's NuSTAR, has helped to show that the spin rates of black holes can be measured conclusively. The solid lines show two theoretical models that explain low-energy X-ray emission seen previously from the spiral galaxy NGC 1365 by XMM-Newton.

Target:
Mission: NuSTAR, XMM-Newton
Spacecraft:
Instrument:
Size: 4266 x 2400
ID#: PIA16870
Added: 2013-02-27

Views: 568

Two X-Ray Observatories are Better Than One

NASA's NuSTAR, has helped to show that the spin rates of black holes can be measured conclusively. The solid lines show two theoretical models that explain low-energy X-ray emission seen previously from the spiral galaxy NGC 1365 by XMM-Newton.

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This chart depicts the electromagnetic spectrum, highlighting the X-ray portion. NASA's NuSTAR and ESA's XMM-Newton telescope complement each other by seeing different colors of X-ray light.
This chart depicts the electromagnetic spectrum, highlighting the X-ray portion. NASA's NuSTAR and ESA's XMM-Newton telescope complement each other by seeing different colors of X-ray light.

Complementary X-Ray Vision
This chart depicts the electromagnetic spectrum, highlighting the X-ray portion. NASA's NuSTAR and ESA's XMM-Newton telescope complement each other by seeing different colors of X-ray light.

Target:
Mission: NuSTAR, XMM-Newton
Spacecraft:
Instrument:
Size: 3000 x 1731
ID#: PIA16698
Added: 2013-02-27

Views: 590

Complementary X-Ray Vision

This chart depicts the electromagnetic spectrum, highlighting the X-ray portion. NASA's NuSTAR and ESA's XMM-Newton telescope complement each other by seeing different colors of X-ray light.

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Scientists measure the spin rates of supermassive black holes by spreading the X-ray light into different colors. The light comes from accretion disks that swirl around black holes, as shown in both of the artist's concepts.
Scientists measure the spin rates of supermassive black holes by spreading the X-ray light into different colors. The light comes from accretion disks that swirl around black holes, as shown in both of the artist's concepts.

Two Models of Black Hole Spin (Artist's Concept)
Scientists measure the spin rates of supermassive black holes by spreading the X-ray light into different colors. The light comes from accretion disks that swirl around black holes, as shown in both of the artist's concepts.

Target:
Mission: NuSTAR, XMM-Newton
Spacecraft:
Instrument:
Size: 3600 x 2400
ID#: PIA16697
Added: 2013-02-27

Views: 773

Two Models of Black Hole Spin (Artist's Concept)

Scientists measure the spin rates of supermassive black holes by spreading the X-ray light into different colors. The light comes from accretion disks that swirl around black holes, as shown in both of the artist's concepts.

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Black holes are tremendous objects whose immense gravity can distort and twist space-time, the fabric that shapes our universe as this chart from NASA's NuSTAR and ESA's XMM-Newton telescope illustrates.
Black holes are tremendous objects whose immense gravity can distort and twist space-time, the fabric that shapes our universe as this chart from NASA's NuSTAR and ESA's XMM-Newton telescope illustrates.

How to Measure the Spin of a Black Hole (Artist's Concept)
Black holes are tremendous objects whose immense gravity can distort and twist space-time, the fabric that shapes our universe as this chart from NASA's NuSTAR and ESA's XMM-Newton telescope illustrates.

Target:
Mission: NuSTAR, XMM-Newton
Spacecraft:
Instrument:
Size: 3600 x 2400
ID#: PIA16696
Added: 2013-02-27

Views: 958

How to Measure the Spin of a Black Hole (Artist's Concept)

Black holes are tremendous objects whose immense gravity can distort and twist space-time, the fabric that shapes our universe as this chart from NASA's NuSTAR and ESA's XMM-Newton telescope illustrates.

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Formats:
Full-Res TIFF: Download, Full-Res JPEG: Download
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Currently displaying images 1-5 of 5
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