These data are crucial to understand galaxies in the young Universe.
The faintest dots you can see are galaxies the light of which took over 13 Billion yrs to reach us. A snapshot of the Universe when it was less than a Billion years old. (3/n)
The Spitzer Infrared data were combined with data in other wavelengths, observed by telescopes on the ground and in Space (#Hubble & many others), all looking at the same parts of the sky - the "CANDELS" fields.
Combined, data from the different telescopes give a comprehensive view of 10s of 1000s of galaxies at different times in the past, over most of the history of the Universe. How this "multi-wavelength astronomy" works is briefly explained here: 👇
The fields for CANDELS (&S-CANDELS) followed the selection of fields we did for an earlier #Spitzer project I was a part of: the Spitzer Extended Deep Survey (SEDS), with a 12-hr exposure depth. They became today's deep survey fields. SEDS is here: cfa.harvard.edu/SEDS/
(6/n)
I love the sense of size and perspective these ultra-deep Spitzer images convey. The angle on the sky is much larger than the #Hubble Deep Fields, and galaxies being unresolved, you aren't distracted by details. You get a sense of size, enormity. The big picture.
(7/n)
You can access S-CANDELS images at the NASA/IPAC IRSA. Choose a field, go to Science Preview, pan, zoom, change color & depth, explore. irsa.ipac.caltech.edu/data/SPITZER/S…
Enjoy.
We are stardust - the conscious stardust that gives the Universe an observer with a sense of joy and awe. (8/8)
A remark: Of course, there are *some* stars in this image - foreground stars in our Milky Way. The bright ones are discernible by having spikes.
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Why do we know #Betelgeuse may go #Supernova within the next few 100000 years, but most likely not soon? And why are we sure the Sun will be a safe star for Billions of years?
First thing to know is: stars are not all alike. They are big, small, bright, dim, have different colors and die different deaths. The quantity at the root of their diversity is their MASS. Stars have masses between roughly 0.1 & 100 times the Sun’s mass. Large ones are rare.2/
Here is the fundamental diagram of stellar evolution. It’s called the Hertzsprung-Russell Diagram (HRD). The further left you go, the hotter stars become. The further up you go, the brighter stars become. 3/
(Pic: ESO)