Miracle. All of it.

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Comet 45P/Honda–Mrkos–Pajdušáková was first discovered 13 orbits ago in 1948 and has returned to the inner Solar System. It is physically ancient. It spends most of its time near the orbit of Jupiter and last neared the Sun in 2011. Over the past few months, Comet 45P’s new sunward plummet has brightened it considerably. The comet is currently visible with binoculars over the western horizon just after sunset, not far from the much brighter planet Venus. Comet 45P was captured last week sporting a long ion tailwith impressive structure. It will pass relatively close to the Earth early next month.”


Notes:

David Bowie

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David Bowie 1947-2016
R.I.P.


Source: this isn’t happiness

Ungraspable

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I’m outside with Zeke.
It’s dark. Still. Quiet.
We’re both calm.
I look up.
He’s sniffing.
Yes, I sense it too.
Something bigger, much bigger here.


In quietness,
the sound of eternity
can at times be heard—
the stars somehow closer and
a sense of the earth’s moving.

~ Michael Boiano


Milky Way Fact Source: Thank you Rob Firchau @ The Hammock Papers

These are mind blowing large numbers

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…Just how many planets are there?…There could be about 23 billion stars in our Milky Way galaxy, each harbouring Earth-sized planets with life-friendly temperatures on their surfaces. Twenty-three billion, give or take a few…Some studies produce numbers of Earth-sized planets closer to 17 billion…Others suggest a figure as low as 6 billion or so, but these are just the planets close to Earth in size. If we extend our reach to slightly larger worlds, the places now known as ‘super-Earths’, we’re back into the tens of billions. No matter how you slice the cosmic cake, you end up with a vast wedge of planets that we’d be happy to go and study, perhaps even land on and cautiously tiptoe about. These are mind-blowingly huge numbers…

So, given the enormity of the number of planets in the galaxy, the question Caleb Scharf tries to answer in his essay is: Are We Alone?


Image Source: theorangeco.  Quote Source: Aeon Magazine

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