09:56 Thu, 08 Dec 2011
I
wrote
previously about blue moons when we last had one in December 2009, and two years
later we are going to have another one on Saturday night.
Even though blue moons are fairly rare, this one will be even more exceptional because
it will be a full lunar eclipse, starting late Saturday night for us in Western
Australia.
Actually, this lunar eclipse is even rarer because it is the second one this year, the
last being in June. You don't often get two eclipses in one year.
This is a full eclipse so it promises to be quite spectacular. I will be out there
enjoying the view.
09:33 Fri, 18 Nov 2011
What would you say is the difference between the lowest and highest point on the Moon?
We know it has low flat plains (the Mares) and it has higher areas where higher
is, umm, I don't know, some sort of hand-waving number. Craters are in there somewhere,
too.
NASA has released this topographic map of the Moon. Look at the range. Lowest is about
−9,000m and highest is +10,000m, a range of roughly 20,000m or 65,000ft! Who'd a
thunk it.

Click for a larger resolution image.
My guess would have been around 5,000ft at the most. I would have been very wrong.
08:14 Thu, 10 Nov 2011
Had a lovely moon
ring last night.
It was about 11pm and I went out to the courtyard and sat down to see how close Jupiter
was going to come to the almost-full Moon. It was a little crisp for late Spring, but
not too bad, still t-shirt and shorts weather, albeit chilly.
Looking up, I was surprised to see a bright, sharp moon ring, enormous in the light sky.
Jupiter was hanging aglow nearby. It really was quite spectacular and unexpected given
I had wandered out for quick look-see at the Moon.
Moon rings are caused by the light refracting from ice crystals in cirrus cloud high up in the
atmosphere. Light from the Moon streaming down to Earth hits the crystals and is
refracted in various directions. An observer will see all the light from crystals where
the angle from the Moon to the cloud to their location is the angle of the internal reflection of
the crystals.
This diagram shows what happens with just two rays of light. Some of the light is
[continued...]
10:08 Sun, 30 Oct 2011
I jumped in the car and headed out last night, ready for an hour or two of astronomy.
As always, am feeling a bit tired this morning.
The thing that sparked me up was an article in yesterday's paper about Venus transits.
The next one is in June 2012, less than a year away, and the one after that is not until
2117. It got me thinking about astronomy in general and particularly around Perth.
The motivation was M31, the
Andromeda galaxy. M31 is about 2.5 million light years and is magnitude 3.4,
visible to the naked eye in a moderately dark sky. Melbourne was too far south to see
it, so I have always wanted to see it once I got to somewhere further north. Now I am
in Perth where M31 gets up to about 20° above the horizon at a certain time of the year, and
right now is that time.
I don't know my way around the dark areas outside Perth, so I figured I would just head
north. North is easy for me, it is basically a freeway to the outskirts and then jump
[continued...]
10:52 Sat, 29 Oct 2011
How to get XEphem and Scrotwm to work together nicely, so that popup dialogs and windows float naturally.
XEphem is a well known astronomy and ephemeris program for unix and Mac (and Windows
on Cygwin or an emulator), and scrotwm
is a dynamic tiling window manager for the same set of operating systems, including
Cygwin/Windows.
Since scrotwm is a tiling window manager, its default behaviour is to open new windows
in a full size tile. XEphem opens quite a few new windows; almost any task opens a
dialog window so you can specify parameters or choose various options. This means that
using XEphem and scrotwm together results in a bunch of open tiles, some of which are
clearly meant to be small dialog windows and others which are meant to be quite large,
such as the view of the sky. We want to change this so that the windows open as they
were designed to open (and which they would if they were on a normal desktop).
Scrotwm lets you override the default behaviour of any window by using its quirks mode.
You specify the window class and name and the behaviour you want. This is clearly
demonstrated in its man page. Unfortunately, you can't use a wildcard, so you can't say
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13:50 Fri, 30 Sep 2011
Wolfram Alpha has a cool
web page that shows satellites overhead, where overhead is defined as visible, i.e.
above the local horizon.
I was very surprised to find I have 1,685 satellites overhead right now. If I
had to guess, I suppose I would have said 3 or 4, not 1,685!
On the other hand, Wolfram Alpha define a satellite as anything, including junk. Even so,
when we restrict it to non-debris satellites it is still a big number, 670 to be exact.
You can click on each satellite and get the orbital elements, range, azimuth and a bunch
of other stuff including a map showing the orbits.
It is pretty cool and worth a visit to play around.
11:18 Fri, 02 Sep 2011
Check out this image of a big coronal mass ejection a few days ago.
Click for full size
Awesome.
The white circle represents the Sun, hidden by the coronagraph's occulting disk.
Eye-balling the image using my Mk-1 thumb, the ejection was 2 or 3 times the Sun's
diameter.
The instrument is part of the SOHO
project, the Solar and Heliographic Observatory, and the actual instrument is the
Large Angle and Spectrometric
Coronagraph Experiment (LASCO).
[continued...]
13:44 Mon, 11 Jul 2011
Today is Neptune's first birthday. It was discovered on 23rd September 1846 and it
takes 164.79 years to complete one orbit, which is today.
Happy birthday, Neptune.
Bob (no, I don't know anything more about him) has a
good in-depth article, and Wikipedia has more.
08:50 Wed, 08 Jun 2011
NASA's Image of the Day shows some stunning photos occasionally, and this is one of them.
Endeavour docked to the ISS, taken from Soyuz (click for bigger)
The pictures are the first taken of a shuttle docked to the station from the
perspective of a Russian Soyuz spacecraft. On May 23, the Soyuz was carrying
Russian cosmonaut Dmitry Kondratyev, NASA astronaut Cady Coleman and European
Space Agency astronaut Paolo Nespoli back to Earth. Once their vehicle was
about 600 feet from the station, Mission Control Moscow, outside the Russian
capital, commanded the orbiting laboratory to rotate 130 degrees. This move
allowed Nespoli to capture digital photographs and high definition video of
shuttle Endeavour docked to the station. Credit: NASA
06:00 Fri, 13 May 2011
Planetary alignment, how and why. With diagrams!
Did you catch the planetary alignment this morning? It was spectacular. I got up early
just before 6am and drove to a nearby hill to get a full view, and it was awesome. The
sky was crisp and sharp and the three brightest planets seemed to hang there glowing
brightly in the low eastern sky. You could easily imagine our early ancestors several
thousand years ago being gobsmacked by such a spectacle and wondering what those lights
were. Heck, even today, when we know what it is. And all this on Friday the 13th!
Marvellous.
Here is the view from the Southern Hemisphere; people in the north probably saw
something similar flipped left-to-right.
top to
bottom: Jupiter, Mercury, Venus and Mars
Venus and Mercury are in the inner Solar System, while Mars and Jupiter are in the
outer. How can we see all four when two of them are "behind" us? The answer is that they
aren't behind us at all. We all are travelling in a glorified circle around the Sun, so
sometimes we can see across the Solar System, past the Sun, all the way across to the
outer Solar System. It's obvious when you see the diagram:
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