A weather and forecast conjunction alignment provided a cloudless sky for the first Kirkstallhenge unveiling, as the last post in the mistYmuse 20/21 encores.
The sunrise was a bit more northern than I thought, rising behind the second building, but that provided a nice shot as our planet span around a bit more, positioning our view of the sun between the buildings.
You’ve been a great crowd, and I’m sure the ancestors would be proud.
Happy mistYmuse ist day, as the m departs with only 3 days to go until mistYmuse Y day; this isn’t a mystery worthy of Scooby; and the greenYgrey world solstice day! This is my contribution to amateur astronomy; the old way; showing how the sunrise (really: our first view of the sun) has started its journey back up the eastern horizon, from its most southerly midwinter point around December 21st (it was cloudy then, so the middle photo is from the 22nd). The top photo is from November 27th, and the bottom yesterday, both 25/26 days either side of the middle one on December 22nd. In the middle midwinter one, the sun rises in the v, to the right of the big tree, while in the other two it rises to the left of the big tree.
To my brain, it still seems strange that the sun goes back up the eastern horizon, even though we’re going around the sun in a circle (now at about 11 o’clock according to an orrery, compared to 1 o’clock in November):
But, thinking about it, that’s because my brain is still thinking of the humanistic sun ‘rise’, rather than the heliocentric our ‘first view of the sun’. ‘Sunrise’ is of course because of our planet’s spin each ‘day’, rather than our orbit around the sun, which gives us our ‘year’ and ‘seasons’.
The sunrise travelling back up the ‘eastern horizon’ is really that we see it earlier in the northern hemisphere as our planet’s stationary axis tilt is pointing more towards the sun for half of the orbit (measured in our calendar as from December to June, with equal half way with the southern hemisphere in March and September).
The orrery shows the norther hemisphere’s six months of more sunlight are when Earth is ‘south’ of the sun, which makes sense when you think about it (not at first for me!), as we are tipped towards the sun then.
Milky Way View
Another way to check this, and get a better idea of how Earth’s 23.4/5 axis tilt and solar orbit directs our view and time, is to look out from the sun, into space. Our planet and solar system is in the west of our Milky Way galaxy.
So, sometimes here on Earth, we have a clear view of most of the Milky Way, and other times we’re on the other side of the sun for the best views (of more of the galaxy). As shown on that website, our best views of the Milky Way are just coming up, from February to October, when we’ll be on the inside of the sun during our solar system (in the above image at about 6/7 o’clock) orbit for closer dark sky views of the centre of our galaxy.
That’s why different constellations are visible at different times of the year, and in different parts of the sky. Ursa Major looked quite low in the northern sky during the summer when I used it to see comet neowise, and now it looks directly above us. That’s because Earth’s position to it has changed, rather than the ‘night sky’ changing. And the same is true of the ‘sunrise’.
Sorry, if the above dragged on a bit, but I’m still working it out myself too!!
Comparing today and Monday’s photos you can see how the sun has moved north on the horizon, as it appears to us, into the centre of the two buildings it was previously to the right of, as we look at them; but apparently it’s because of our Earth’s axis tilt and orbit of the sun allowing us to see it earlier: ten minutes earlier, from 06.51 to 06.41.