Jupiter and the Moon shine through steady skies

Here are a few pictures of the Moon and Jupiter that I captured on Friday night/Saturday morning under some great seeing conditions – in fact the best seeing conditions I’ve seen all year. All of the images were taken with an 8-inch Schmidt-Cassegrain telescope, an Imaging Source DMK21AU618.AS CCD camera and a 2x Barlow lens. To create the colour Jupiter image I also used a set of Astronomik RGB filters and a 3x Barlow lens (I used the 3x Barlow for the Atlas/Hercules shot too).

Jupiter and the Great Red Spot. Credit: Will Gater
Posidonius_01122012The rille network within crater/walled plain Posidonius. Credit: Will Gater
Janssen_01122012The walled plain Janssen and the crater Fabricius (top). Credit: Will Gater
CleomedesLong shadows on the floor of the walled plain Cleomedes. Credit: Will Gater
DorsaGeikieCrater Messier (left) and Dorsa Geikie (centre). Credit: Will Gater
gocleniusCrater Gutenberg (upper left). Credit: Will Gater
VallisRheitaVallis Rheita and crater Rheita. Credit: Will Gater
copernicusCrater Copernicus lit from above. Credit: Will Gater
atlas_herculesCraters Atlas (right) & Hercules (left). Credit: Will Gater
RimaCauchySinus Concordiae & Rima Cauchy. Credit: Will Gater

Two glittering planets meet the Earthshine lit Moon

Venus, Jupiter & the crescent Moon. (Click for full-size version) Credit: Will Gater

Jupiter, Venus and the crescent Moon are putting on a wonderful show in the west after sunset at the moment. The picture above shows the view last night with Jupiter and the Moon separated by roughly 3 degrees. A close-up of the view (below) shows the Moon and Jupiter as well as two of the Galilean satellites – Ganymede and Callisto. Tonight the view is no less spectacular with the brilliant Venus and the crescent Moon a little over 2 degrees apart. Pop out and see them if you can.

While you’re out, look out for the effect known as ‘Earthshine’. This is where sunlight reflected off the Earth’s bright cloud tops lights up the part of the Moon that isn’t directly lit by the Sun; it’s best seen when the Moon is a thin crescent, like it is at the moment. You can see Earthshine clearly illuminating the face of the Moon in the image below.

Jupiter, the crescent Moon & Earthshine. (Click for full-size version) Credit: Will Gater

NASA’s Juno mission to Jupiter

An artist’s impression of the Juno spacecraft at Jupiter. Credit: NASA/JPL-Caltech

Thanks to a tweet from the Guardian’s science correspondent Ian Sample I’ve been exploring this superb, Flash based, website covering NASA’s Juno mission.

After clicking on the ‘begin journey’ tab the site takes you through a series of narrated full screen videos that set the scene for the mission and explain some of key scientific objectives; between each video there’s an excellent interactive page, with further images and videos, allowing you to find out more about each topic. For example, here’s a page that covers the rocket that will launch Juno, while this one focuses on Jupiter’s atmosphere.

As well as the great graphics & engaging narration I particularly liked the ‘cluster’ of stars at the end of the presentation, each one representing an astronomical question.

As for the probe itself, it’s scheduled to be launched on an Atlas V rocket tomorrow (5 August). You’ll be able to watch the lift-off live, and in HD, on the NASA TV page here.

Hiding Ganymede and an extrasolar connection

jupiterhubble1Jupiter & Ganymede. Credit: NASA, ESA, and E. Karkoschka (Univ. of Arizona)

Jupiter might not exactly be well placed for observing from the Northern Hemisphere this year, due to its relatively low altitude, but all is not lost. NASA have just released this beautiful, “close to natural” colour, image from the Hubble Space Telescope. It shows the Galilean moon Ganymede beginning to disappear behind the southwestern part of Jupiter’s enormous disc. You can watch a video of Ganymede disappearing behind Jupiter (over the course of two hours) on the NASA Hubble site. The images were taken in April 2007 and, as can be seen in the crop of the main image below, they show the huge rocky and icy moon in quite some detail.

ganymedehubbleGanymede disappearing. Credit: NASA, ESA, and E. Karkoschka (Univ. of Arizona)

Compare this new Hubble image of Ganymede to the one (below) from the New Horizons mission en-route to Pluto and you get a feel for just how good Hubble’s resolution is! The bright splodge towards the upper middle of Ganymede’s terminator in the New Horizons image is a huge crater known as Tros and it’s clearly visible, as a bright white spot, in Hubble’s shot as well. There are features smaller than Tros visible in the Hubble image too. That’s not to say that the New Horizons image isn’t any good. Far from it, it’s amazing — it’s just that Hubble is one impressive instrument!

newhorizonsganymedeA view of Ganymede from the New Horizons spacecraft as it whisked by.
Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Southwest Research Institute

Anyway I’m moving a little away from my point. Not only is Hubble’s new shot a wonderful picture, full of intriguing details on both Jupiter and Ganymede (especially the high resolution versions), it also illustrates nicely how astronomers have been able to study Jupiter’s atmosphere. The method astronomers have been using to do this is also similar to how astronomers ‘probe’ the atmospheres of distant exoplanets. Ganymede is reflecting light from the Sun back towards us (that’s how we can see it). That light passes through the upper reaches of Jupiter’s atmosphere, towards us, as Ganymede disappears behind the limb of the huge planet. By spectroscopically studying the chemical fingerprints stamped on this light, by Jupiter’s atmosphere, astronomers can then work out important properties and compositions of the gases in this part of the Jovian atmosphere.

exoplanetlimbAn illustration showing light passing through the atmosphere of an exoplanet.
Credit: ESA, NASA and Frederic Pont (Geneva University Observatory)

In a very similar way, when studying exoplanets, astronomers have been able to detect the chemical signatures of interesting molecules in exoplanetary atmospheres, that have been stamped on the light from the exoplanet’s parent star. So it isn’t just in studying the gas giants of our own Solar System that this versatile astronomical technique is used. It will be interesting to see what these observations from Hubble tell us about Jupiter’s atmosphere. If they are anything like the results seen from studying the atmospheres of distant exoplanets, they will be very interesting indeed.