This NASA/ESA Hubble Space Telescope image features
the face-on spiral galaxy NGC 4900.
ESA/Hubble & NASA, S. J.
Smartt, C. Kilpatrick
This NASA/ESA Hubble Space Telescope image
features a sparkling spiral galaxy paired with a prominent star, both in the
constellation Virgo. While the galaxy and the star appear to be close to one
another, even overlapping, they’re actually a great distance apart. The star,
marked with four long diffraction spikes, is in our own galaxy. It’s just 7,109
light-years away from Earth. The galaxy, named NGC 4900, lies about 45 million
light-years from Earth.
This image combines data from two of
Hubble’s instruments: the Advanced Camera for Surveys, installed in 2002 and still in operation today, and the older Wide
Field and Planetary Camera 2, which was in use from 1993 to 2009. The data used
here were taken more than 20 years apart for two different observing programs —
a real testament to Hubble’s long scientific lifetime!
Both programs aimed to understand the
demise of massive stars. In one, researchers studied the sites of past
supernovae, aiming to estimate the masses of the stars that exploded and
investigate how supernovae interact with their surroundings. They selected NGC
4900 for the study because it hosted a supernova named SN 1999br.
In the other program, researchers laid the groundwork for studying future supernovae by collecting images of more than 150 nearby galaxies. When researchers detect a supernova in one of these galaxies, they can refer to these images, examining the star at the location of the supernova. Identifying a supernova progenitor star in pre-explosion images gives valuable information about how, when, and why supernovae occur.
By: NASA Hubble Mission Team, Goddard Space Flight Center
No comments:
Post a Comment