HiRISE Mars Digital Elevation Models: Difficult to Build, Easy on the Eye

DEM images of Columbia Hills on Mars (USGS/HiRISE)
DEM images of Columbia Hills on Mars (USGS/HiRISE)

If there’s one instrument that should get the Mars Orbiting Science Award of 2008 it’s the High Resolution Imaging Science Experiment (HiRISE). Flying on board NASA’s Mars Reconnaissance Orbiter (MRO), HiRISE has been taking some astonishing imagery of the Martian surface since 2006. In fact, the HiRISE image gallery has become the staple of my high resolution Mars photo collection, and the studies being carried out by this fantastic instrument have formed the basis of many articles.

However, the most useful images to come from HiRISE are also the rarest. Digital Elevation Models (DEMs) come from the use of stereo image pairs (more commonly seen in anaglyphs generated by the HiRISE team to give the viewer a 3D impression of the Martian landscape). In the case of DEMs, some pretty neat science can be done, generating images of the Red Planet’s terrain in unrivalled precision. Seeing the Victoria Crater DEM is a particular joy
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MRO Spots Mars Dust Storm in the Making

Wind whipping up a dust storm on Mars (NASA)
Wind whipping up a dust storm on Mars (NASA)

One of the overriding features in the Martian atmosphere is the troublesome dust storm. Sometimes, these storms can last months and can span the entire planet. As testified by the solar panels on rovers Spirit and Opportunity, dust storms block sunlight from passing through the atmosphere and can deposit a thick red layer over the robots, amplifying the dust storm’s damaging effects.

In the stunning image above, the Mars Reconnaissance Orbiter (MRO) captured the dust being blown up from the Red Planet’s surface. In short, this is the source of a growing dust storm from a canyon system, injecting a huge amount of material into the skies…
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Introducing the Exomoon, and Detecting them via Exoplanet Wobble

Can astronomers really detect exomoons?
Can astronomers really detect exomoons?

Exomoon: The natural satellite of an exoplanet.

Before today, I hadn’t heard anything about the possibility of looking for moons orbiting planets in other star systems. Sorry, exomoons orbiting exoplanets in other star systems. But a British astronomer has calculated that it is possible to not only detect exomoons, but it is possible to deduce their distance from the parent exoplanet and their mass.

All this is done by measuring the exoplanet’s “wobble”; a practice more commonly used in the pursuit of the exoplanets themselves. By detecting the wobble of distant stars, the gravitational pull of the exoplanet becomes obvious. The same can be done with exoplanets, possibly revealing the presence of Earth-like exomoons.

Of the 300+ exoplanets discovered, 30 are within the habitable zones of their stars. If these large gas giant exoplanets (usually several times the mass of Jupiter) have an exoplanet system of their own, these exomoons also fall within the habitable zone…

Makes you think, doesn’t it?

For the full article, check out Astronomers Now Looking For Exomoons Around Exoplanets on the Universe Today…

The Cancer Spreads: Mars Science Laboratory Delayed Until 2011

The Mars Science Laboratory (MSL) project is failing. But it is not suffering from technical failure en-route to the Red Planet, it hasn’t gotten itself stuck in a Martian sand-trap, it hasn’t even fallen foul of the “Galactic Ghoul”; the MSL is suffering from an overlooked space exploration hazard: bad management. According to today’s (not unexpected) NASA announcement, the MSL will not be launched until 2011.

I had a very bad feeling about today’s press conference, and it looks like my fears were justified. Due to technical difficulties, the launch of the MSL is being delayed by two years, as the overrun will ensure the mission misses the next Mars launch window. So I have to ask: why is an over-budget, behind schedule, poorly managed mission being allowed to sap the budgets of other NASA programs when the solution is so obvious?
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Another Exoplanet Candidate Identified by ESO

It would appear that yet another extrasolar planet has been directly observed!

Only last week, the Hubble Space Telescope released news that it had spotted an exoplanet orbiting the star Fomalhaut. This is the first ever direct observation of an exoplanet in optical wavelengths. On the same day, joint observations by the ground-based (adaptive optics-powered) Keck II and Gemini infrared telescopes discovered a collection of three large alien worlds orbiting a star catalogued as HR 8799.

Today, a completely different observatory appears to have discovered yet another exoplanet orbiting the hot star Beta Pictoris (in the constellation of Pictor). European Southern Observatory (ESO) astronomers have directly imaged β Pictoris b, an alien planet orbiting 8 AU from its host star.

A phenomenal achievement considering β Pictoris is over 63 light years away…
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Dust Really IS a Problem for Spirit

The ninja rover, NASA's answer to creeping up on Martian lifeforms...
The ninja rover, NASA's answer to creeping up on Martian lifeforms...

Talk about having a bad dust day. Only last night on Astroengine Live I was discussing the near-death experience Mars Exploration Rover Spirit survived a few days ago. Much to NASA’s (and the science-loving world’s) relief, the Sun-blocking dust storm in Gusev Crater couldn’t beat down this tough wheeled warrior. Even though her solar panels are coated in a thick layer of red dust, she battles on to see another sol. According to NASA, Spirit will remain in a recovery mode until next month at least, giving the batteries some time to recharge…
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Alien Worlds: Extrasolar Planets Imaged for First Time

Two of the three confirmed planets orbiting HR 8799 indicated as
Two of the three confirmed planets orbiting HR 8799 indicated as “b” and “c” on the image above. “b” is the ~7 Jupiter-mass planet orbiting at about 70 AU, “c” is the ~10 Jupiter-mass planet orbiting the star at about 40 AU. Due to the brightness of the central star, it has been blocked and appears blank in this image to increase visibility of the planets (Gemini Observatory)

The day has finally come. We now have direct, infrared and optical observations of planets orbiting other stars. Yesterday, reports from two independent sources surfaced, one from the Gemini and Keck II observatories and the second from the Hubble Space Telescope. Brace yourself for an awe-inspiring display of planets orbiting two stars…

The Gemini/Keck observations were carried out using adaptive optics technology to correct in real-time for atmospheric turbulence. The stunning images of a multiple planetary star system were then constructed from infrared emissions (the image, top, was constructed by Keck II as a follow-up to to the Gemini observations). The system in question is centred around a star called HR 8799, approximately 130 light years from Earth and in the constellation of Pegasus. The entire press release can be found at the Gemini observatory site, where they give the discovery a full run-down.

On the same day, the Hubble Space Telescope team also released images of one extrasolar planet, only this time in optical wavelengths. Although the exoplanet in Hubble’s images is less obvious than the infrared Gemini/Keck II images, incredible detail has been attained, showing a ring of dust around the star Fomalhaut (located in the constellation of Piscis Austrinus). Fomalhaut is 25 light years away and the star’s daughter planet (Fomalhaut b) is only a little under 3 Jupiter masses.

Estimated to be no more than three times Jupiter's mass, the planet, called Fomalhaut b, orbits the bright southern star Fomalhaut, located 25 light-years away in the constellation Piscis Austrinus (NASA/ESA)
Estimated to be no more than three times Jupiter’s mass, the planet, called Fomalhaut b, orbits the bright southern star Fomalhaut, located 25 light-years away in the constellation Piscis Austrinus (NASA/ESA)

For more news on these discoveries, check out the Gemini/Keck II press release and the Hubble announcement. I’ll leave the ground-breaking announcement to the guys who have spent many years working to achieve this monumental goal.

Wow.

Sources: Gemini, ESA

A Mystery Aurora above Saturn’s Mysterious North Pole Hexagon

The aurora above Saturn's North Pole hexagon (NASA)

Not only does Saturn have a mysterious hexagonal shape etched into the bands of cloud above its north pole, it also has a unique magnetic structure. This is suggested by recent results recorded by the NASA Cassini probe that passed over the pole to see a huge active auroral region, much larger and more dynamic than expected. Interestingly, the NASA press release has not linked the strange aurora with the long-lived hexagonal shape in the gas giant’s atmosphere. Could the hexagon be formed by a unique magnetic structure above Saturn? Or could both phenomena be connected in some other way?
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Phoenix is Dead, Spirit is Failing

Mars dust is a big problem for technology; it’s very fine, abrasive and sticks to everything. Airborne dust has been blamed for accelerating Phoenix’s death, and the hardy Mars Exploration Rover Spirit looks like it has finally met its match. The critical issue here is a build-up of the red powder over the surface of the energy-collecting solar panels our robotic explorers depend on to power their experiments and movement over the Martian terrain. If solar cells cannot receive light, electricity cannot be generated, hastening the end of of Phoenix, and possibly one of the rover twins…
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Strangest Kuiper Belt Objects: The Top Five

From Pluto, looking at its icy moons in the Kuiper belt (NASA)

The Kuiper belt is strange. Most of this strangeness probably comes from the fact that we are only just beginning to uncover this mysterious region of the Solar System. Unlike the Oort Cloud which (possibly) lies beyond 3 × 1012 km away (over 20,000 AU, or a whopping 0.3 light years), we can actually observe the objects inside the Kuiper belt as, compared to the Oort Cloud, the Kuiper belt is on our interplanetary doorstep.

But that doesn’t mean it’s close. The Kuiper belt exists in a region of space 30–55 AU from the Sun; this is where Pluto lives (as Pluto itself is a “Kuiper belt object”, or KBO). As astronomical techniques become more advanced however, we are able to discover more KBOs in the zoo of icy-rocky bodies that live in this region.

Having just written about an oddball pair of “highly split” KBOs, I feel compelled to list my top five favourite KBOs. Here are my favourites, as some are really funny-lookin’ and others have some serious personal issues…
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