JFIFHH=This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). We see it partially edge-on and this perspective showcases the galaxy’s beautiful arms, which swirl like a whirlpool around its bright central region. Even though NGC 7331 is a spiral galaxy like our galactic home, the Milky Way, it is actually quite different from it. NGC 7331 is an unbarred spiral galaxy — in other words, it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way — and its central bulge displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. However, it is similar in size, shape, and mass to our own, has a comparable star formation rate and hosts a similar number of stars, has a central supermassive black hole as the Milky Way does, and has spiral arms that look quite like the Milky Way’s. This twinnish similarity is more than just an interesting fact — it’s actually very useful. It can be difficult for astronomers to study certain aspects of our own galaxy because we live inside it, but by studying similar galaxies we can build a better understanding of our own, and of galactic behaviour and evolution as a whole. This image was captured by Hubble’s Wide Field Camera 3 (WFC3), which is able to observe light spanning the near-infrared, visible, and near-ultraviolet parts of the spectrum.bPhotoshop 3.08BIMZ%GTwins with differencesNGC 7331720180129<060000n ESA/Hubble & NASA/D. Milisavljevs ESA/HubblexThis NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it’s beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble’s Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star — a supernova — which can still be faintly seen as a tiny red dot near the galaxy’s central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich — in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the Milky Way. It also has a comparable star formation rate, hosts a similar number of stars, has a central supermassive black hole and comparable spiral arms. The primary difference between our galaxies is that NGC 7331 is an unbarred spiral galaxy — it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. By studying similar galaxies we hold a scientific mirror up to our own, allowing us to build a better understanding of our galactic environment which we cannot always observe, and of galactic behaviour and evolution as a whole.8BIM 8BIM%_lb Z#CIs!8ExifMM*This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). We see it partially edge-on and this perspective showcases the galaxy’s beautiful arms, which swirl like a whirlpool around its bright central region. Even though NGC 7331 is a spiral galaxy like our galactic home, the Milky Way, it is actually quite different from it. NGC 7331 is an unbarred spiral galaxy — in other words, it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way — and its central bulge displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. However, it is similar in size, shape, and mass to our own, has a comparable star formation rate and hosts a similar number of stars, has a central supermassive black hole as the Milky Way does, and has spiral arms that look quite like the Milky Way’s. This twinnish similarity is more than just an interesting fact — it’s actually very useful. It can be difficult for astronomers to study certain aspects of our own galaxy because we live inside it, but by studying similar galaxies we can build a better understanding of our own, and of galactic behaviour and evolution as a whole. This image was captured by Hubble’s Wide Field Camera 3 (WFC3), which is able to observe light spanning the near-infrared, visible, and near-ultraviolet parts of the spectrum.This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). We see it partially edge-on in a perspective which showcases the galaxy’s beautiful arms, which swirl like a whirlpool around its bright central region. Even though NGC 7331 is a spiral galaxy like our galactic home, the Milky Way, it is actually quite different from it. NGC 7331 is an unbarred spiral galaxy — in other words, it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. However, it is similar in size, shape, and mass to our own galaxy, has a comparable star formation rate and hosts a similar number of stars. Like the Milky Way, it has a central supermassive black hole and spiral arms that look quite like our own. This twinnish similarity is more than just an interesting fact — it’s actually very useful. It can be difficult for astronomers to study certain aspects of our own galaxy because we live inside it, but by studying similar galaxies we almost hold a scientific mirror up to ourselves, allowing us to build a better understanding of our galactic environment, and of galactic behaviour and evolution as a whole. This image was captured by Hubble’s Wide Field Camera 3 (WFC3), which is able to observe light spanning the near-infrared, visible, and near-ultraviolet parts of the spectrum.This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). We see it partially edge-on in a perspective which showcases the galaxy’s beautiful arms, which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble’s Wide Field Camera 3 (WFC3), as they observed an extraordinary exploding star — a supernova — which can still be faintly seen as a tiny red dot near the central yellow core. Named SN2014C, it exhibited a strange life-cycle, rapidly evolving from a supernova containing very little Hydrogen to one that is Hydrogen-rich — in just one year. NGC 7331 is similar in size, shape, and mass to our own galaxy, has a comparable star formation rate and hosts a similar number of stars. Like the Milky Way, it has a central supermassive black hole and spiral arms that look quite like our own. The primary difference between our galaxies is that NGC 7331 is an unbarred spiral galaxy — it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. This twinnish similarity is very useful, as it can be difficult for astronomers to study some aspects of our own galaxy because we live inside it. By studying similar galaxies we hold a scientific mirror up to ourselves, allowing us to build a better understanding of our galactic environment, and of galactic behaviour and evolution as a whole. whole.This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it’s beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble’s Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star — a supernova — which can still be faintly seen as a tiny red dot near the galaxy’s central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich — in just one year. NGC 7331 is similar in size, shape, and mass to the Milky Way, it also has a comparable star formation rate and hosts a similar number of stars. Like our own galaxy, it has a central supermassive black hole and comparable spiral arms. The primary difference between our galaxies is that NGC 7331 is an unbarred spiral galaxy — it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. By studying similar galaxies we hold a scientific mirror up to our own, allowing us to build a better understanding of our galactic environment which we cannot always observe, and of galactic behaviour and evolution as a whole.sc itself. By studying similar galaxies we hold a scientific mirror up to ourselves, allowing us to build a better understanding of our own galactic environment, and of galactic behaviour and evolution as a whole.This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it’s beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble’s Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star — a supernova — which can still be faintly seen as a tiny red dot near the galaxy’s central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich — in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the Milky Way. It also has a comparable star formation rate, hosts a similar number of stars, has a central supermassive black hole and comparable spiral arms. The primary difference between our galaxies is that NGC 7331 is an unbarred spiral galaxy — it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. By studying similar galaxies we hold a scientific mirror up to our own, allowing us to build a better understanding of our galactic environment which we cannot always observe, and of galactic behaviour and evolution as a whole.s a whole. XICC_PROFILE HLinomntrRGB XYZ  1acspMSFTIEC sRGB-HP cprtP3desclwtptbkptrXYZgXYZ,bXYZ@dmndTpdmddvuedLview$lumimeas $tech0 rTRC< gTRC< bTRC< textCopyright (c) 1998 Hewlett-Packard CompanydescsRGB IEC61966-2.1sRGB IEC61966-2.1XYZ QXYZ XYZ o8XYZ bXYZ $descIEC http://www.iec.chIEC http://www.iec.chdesc.IEC 61966-2.1 Default RGB colour space - sRGB.IEC 61966-2.1 Default RGB colour space - sRGBdesc,Reference Viewing Condition in IEC61966-2.1,Reference Viewing Condition in IEC61966-2.1view_. \XYZ L VPWmeassig CRT curv #(-27;@EJOTY^chmrw| %+28>ELRY`gnu| &/8AKT]gqz !-8COZfr~ -;HUcq~ +:IXgw'7HYj{+=Oat 2FZn  % : O d y  ' = T j " 9 Q i  * C \ u & @ Z t .Id %A^z &Ca~1Om&Ed#Cc'Ij4Vx&IlAe@e Ek*Qw;c*R{Gp@j>i  A l !!H!u!!!"'"U"""# #8#f###$$M$|$$% %8%h%%%&'&W&&&''I'z''( (?(q(())8)k))**5*h**++6+i++,,9,n,,- -A-v--..L.../$/Z///050l0011J1112*2c223 3F3334+4e4455M555676r667$7`7788P8899B999:6:t::;-;k;;<' >`>>?!?a??@#@d@@A)AjAAB0BrBBC:C}CDDGDDEEUEEF"FgFFG5G{GHHKHHIIcIIJ7J}JK KSKKL*LrLMMJMMN%NnNOOIOOP'PqPQQPQQR1R|RSS_SSTBTTU(UuUVV\VVWDWWX/X}XYYiYZZVZZ[E[[\5\\]']x]^^l^__a_``W``aOaabIbbcCccd@dde=eef=ffg=ggh?hhiCiijHjjkOkklWlmm`mnnknooxop+ppq:qqrKrss]sttptu(uuv>vvwVwxxnxy*yyzFz{{c{|!||}A}~~b~#G k͂0WGrׇ;iΉ3dʋ0cʍ1fΏ6n֑?zM _ɖ4 uL$h՛BdҞ@iءG&vVǥ8nRĩ7u\ЭD-u`ֲK³8%yhYѹJº;.! zpg_XQKFAǿ=ȼ:ɹ8ʷ6˶5̵5͵6ζ7ϸ9к<Ѿ?DINU\dlvۀ܊ݖޢ)߯6DScs 2F[p(@Xr4Pm8Ww)Kmhttp://ns.adobe.com/xap/1.0/ 814 657 555 438 336 275 WFC3 WFC3 WFC3 WFC3 WFC3 WFC3 Optical Optical Optical Optical Optical Ultraviolet 4061.0 3038.0 C.5.5.2 Red Red Green Cyan Blue Blue I H-Alpha +NIII V B u uv -1.10171197421e-05 1.10171197421e-05 2030.5 1519.0 339.272234733 34.4087283825 Hubble Space Telescope Hubble Space Telescope Hubble Space Telescope Hubble Space Telescope Hubble Space Telescope Hubble Space Telescope Twins with differences This NASA/ESA Hubble Space Telescope image shows a spiral galaxy known as NGC 7331. First spotted by the prolific galaxy hunter William Herschel in 1784, NGC 7331 is located about 45 million light-years away in the constellation of Pegasus (The Winged Horse). Facing us partially edge-on, the galaxy showcases it’s beautiful arms which swirl like a whirlpool around its bright central region. Astronomers took this image using Hubble’s Wide Field Camera 3 (WFC3), as they were observing an extraordinary exploding star — a supernova — which can still be faintly seen as a tiny red dot near the galaxy’s central yellow core. Named SN2014C, it rapidly evolved from a supernova containing very little Hydrogen to one that is Hydrogen-rich — in just one year. This rarely observed metamorphosis was luminous at high energies and provides unique insight into the poorly understood final phases of massive stars. NGC 7331 is similar in size, shape, and mass to the Milky Way. It also has a comparable star formation rate, hosts a similar number of stars, has a central supermassive black hole and comparable spiral arms. The primary difference between our galaxies is that NGC 7331 is an unbarred spiral galaxy — it lacks a “bar” of stars, gas and dust cutting through its nucleus, as we see in the Milky Way. Its central bulge also displays a quirky and unusual rotation pattern, spinning in the opposite direction to the galactic disc itself. By studying similar galaxies we hold a scientific mirror up to our own, allowing us to build a better understanding of our galactic environment which we cannot always observe, and of galactic behaviour and evolution as a whole. 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