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On Mars, the wind wins

ESP_039057_1485_1.0x A piece of Mars: This scene (600×450 m or 1969×1476 ft) is covered in small craters, formed by the splash of a larger crater nearby. They cover everything, even the bright ripples visible on the right. So the ripples were there before the impact that formed all these little craters. And yet… there are itsy little gray ripples on the upper right, merging with the crater rims – these are new ripples, younger than the craters. On Mars, it’s the wind that wins in the end. (HiRISE ESP_039057_1485, NASA/JPL/Univ. of Arizona)

Wind eroded mantle

ESP_039195_1755_0.398xA piece of Mars: The curving ridge of a mountain has signs of many small landslides. Mantled on top of these is an older set of landslides that has been partially eroded away. The rippled edge of this older deposit suggests that it is wind that has done the erosion. So the history here goes: mountains, then landslides, then wind erosion, then new smaller landslides. (HiRISE ESP_039195_1755 NASA/JPL/Univ. of Arizona)

Bearded craters and dunes

A piece of Mars: This 600×450 m (1969×1476 ft) scene has a complex sedimentary history. How are bearded craters and dunes formed? They weren’t always bearded. At some point, a deposit of bright material accumulated on this surface, and was then eroded so that all that remains of it is what is protected by topography (anything that pokes up like dunes or crater rims). Can you find the boulder that has tumbled downslope (it too has a beard!). (HiRISE ESP_038826_1700, NASA/JPL/Univ. of Arizona)

Hello from AAS!

Happy new year, Internet! I’m starting off the year at the 225th meeting of the American Astronomical Society. It’s an annual conference where all the professional astronomers in the United States get together and talk about space! There’s been some really cool presentations, including the discovery of Earth-sized planets in possibly habitable orbits around other stars by Kepler. Sounds pretty cool right?

A subset of the GPI team was here for the AAS. We gave an update on the GPI Exoplanet Survey, presented posters on debris disks and exoplanets imaged by GPI, and even had a press conference on recent GPI results!

In addition to all the GPI results, the GPI team also had a team lunch to talk about starlight subtraction. Even with the star masked out, starlight still diffracts around the coronagraph and hides the faint exoplanets and debris disks that we are trying to see. As you might guess, starlight subtraction is a really important for GPI, especially with the kickoff of the GPI Exoplanet Survey just a couple of months ago. The content of meeting was a bit technical so I’ll spare you the summary here. It was a productive lunch though, and overall it’s been a great conference!

The only good picture is the one in which my eyes are closed.

The GPI Team in Seattle. Photo credit: Marshall Perrin

The Gemini Planet Imager Produces Stunning Observations In Its First Year


GPI imaging of the planetary system HR 8799 in K band, showing 3 of the 4 planets. (Planet b is outside the field of view shown here, off to the left.) These data were obtained on November 17, 2013 during the first week of operation of GPI and in relatively challenging weather conditions, but with GPI’s advanced adaptive optics system and coronagraph the planets can still be clearly seen and their spectra measured (see Figure 2). Image Credit: Christian Marois (NRC Canada), Patrick Ingraham (Stanford University) and the GPI Team.

Gemini Observatory
Media Advisory

For release at the American Astronomical Society meeting press confer-ence January 6, 2015, 10:15am (PST)

Publication-quality images available at:


Stunning exoplanet images and spectra from the first year of science operations with the Gemini Planet Imager (GPI) were featured today in a press conference at the 225th meeting of the American Astronomical Society (AAS) in Seattle, Washington. The Gemini Planet Imager GPI is an advanced instrument designed to observe the environments close to bright stars to detect and study Jupiter-like exoplanets (planets around other stars) and see proto-stellar material (disk, rings) that might be lurking next to the star.


Happy New Year to the Planet!

I decided to do something new to start the New Year. I translated a podcast from a program called Geopolitics on France Inter written by Anthony Bellanger. You can listen to the original French version here.

I like the text since it is quite optimistic and it summarizes the progresses that we have made over the past 50 years. The world is not perfect yet, but it is indeed a better place.


Are there any reasons to wish people a Happy New Year 2015?

I believe there are many and would like to explain why.

First: our health. Never have so many people all over the world been so healthy and well cared for.

It may seem strange to say that when nearly 8,000 people have died of Ebola in West Africa in recent months, and when the epidemic is far from defeated—yet it’s true.

Over the last half century , the infant mortality rate has fallen by two-thirds and the average human lifespan has increased by twenty years and continues to grow. Better yet, the difference in life expectancy between rich and poor countries is narrowing year by year.

Thanks to modern medicine, diseases that decimated entire populations throughout history are almost eradicated. The number of polio cases, for example, has fallen by 99% since 1988.

Between 2000 and 2015, the number of global malaria cases has dropped in half thanks to a global mobilization against the disease. Even AIDS, which appeared only 30 years ago, is now tested for and treated all over the world.

What about hunger and education?

Here, too, things are looking up. Hunger around the world declines annually. Since the early 90s — only 25 ago! — the percentage of undernourished people around the world has fallen by half.

The great famines that killed tens of thousands of people in the 1980s — in Ethiopia, for example —have disappeared. The world is better organized than ever and extremely efficient at delivering emergency medical and food aid when and where it is needed.

On the education front, results are even more impressive: In only 10 years, school enrollment for boys and girls has increased from 84 to 89% in primary grades and 60 to 73% in secondary grades. Around the world, three out of four children go to school until they are at least 14 years old!

We see similar improvements in the area of extreme poverty, which has fallen by 50 percent since 1990. This is unheard of in human history.

What is the source of this improvement?

We all are! Despite what we may hear or say, international institutions — the UN, NGOs and many others —work effectively: they treat, train, vaccinate, feed and intervene anywhere in the world where they are needed.

Even freedom is rising: in the last half century, the number of democratic states has tripled, and half the world’s population now lives under this type of government which — though often imperfect — is a unique achievement in human history.

So yes, one may wish people a Happy New Year, knowing that there will be wars, massacres, and many other disasters but also knowing that we have never been better educated, cared for and nurtured than we are in 2015.

The long, low dune

ESP_038615_1665_1.0xA piece of Mars: A long, low dune covered in long, linear ripples stretches across the scene (600×450 m; 1969×1476 ft). Dark gray areas on the dune show where sand has most recently moved. A small slip face has formed on the southeast side of the dune, but ripples have formed on it, so there haven’t been any recent avalanches here. (ESP_038615_1665, NASA/JPL/Univ. of Arizona)

Wind, wind, impact(!), and then more wind…

ESP_038918_1650_0.437xA piece of Mars: Some time ago, something hit the ground on Mars and made this impact crater, right into a field of ripples. Stuff thrown up during the impact fell back down, burying the ripples with the gray ejecta rays that radiate from the crater. But the wind kept blowing, and in some places you can see where new ripples have formed on top of the ejecta. That’s Mars for you: wind, wind, wind, impact(!), more wind… (HiRISE ESP_038918_1650, NASA/JPL/Univ. of Arizona)

AGU Fall Meeting 2014: Solar System Small Bodies: Relics of Formation and New Worlds to Explore

Can you believe it is December already!? As usual, it is a busy month with the AGU Fall Conference.  I co-organized a session on small solar system bodies with Padma Yanamandra-Fisher (PSI)  and Julie Castillo (JPL).  We will talk about recent discoveries in this emerging field including the discovery of rings around Chariklo, the understanding of regolith motion on asteroids, the new lander for Hayabusa 2 (MASCOT) and off course adaptive optics observations of asteroids. Below more info. See you there!

Where: Thursday, December 18, 2014 01:40 PM – 03:40 PM
When: Moscone West 3002

Why: The composition and physical properties of Small Solar System Bodies (SSSBs), remnants of the formation of planets, are key to better understand the origins of our solar system and their potential as resources is necessary for robotic and human exploration. Missions such as ESA/Gaia, NASA/OSIRIS-REx, JAXA/Hyabusa-2, NASA/Dawn and NASA/New Horizons, to study asteroids, comets, dwarf planets and TNOs are poised to provide new in situ information. on SSSBs.  Recent remote observations of bright and main belt comets; asteroid Chariklo, with its ring system; asteroid and KBO binaries illustrate that the distinction between comets and asteroids is blurred, providing a new paradigm for such classification. This session welcomes abstracts on the remarkable results bringing information on the internal structure and composition of SSSBs based on space and ground-based data, numerical models, as well as instrument/mission concepts in theprospect of future exploration.

Artistic representation of the triple asteroid system showing the large 270-km asteroid Sylvia surrounded by its two satellites, Romulus and Remus. The differentiated interior of the asteroid is shown through a cutaway diagram. The primary asteroid of the system may have a dense, regularly-shaped core, surrounding by a fluffy or fractured material. The two moons are shown to be strongly elongated, and composed of two lobes, as suggested by the recently observed occultation data by the satellite Romulus. (credits: D. Futselaar & F. Marchis)

Artistic representation of the triple asteroid system showing the large 270-km asteroid Sylvia surrounded by its two satellites, Romulus and Remus. The differentiated interior of the asteroid is shown through a cutaway diagram. The primary asteroid of the system may have a dense, regularly-shaped core, surrounding by a fluffy or fractured material. The two moons are shown to be strongly elongated, and composed of two lobes, as suggested by the recently observed occultation data by the satellite Romulus. (credits: D. Futselaar & F. Marchis)


Aeolian shoreline

ESP_038799_1590_1.0xA piece of Mars: On the left is a steep slope leading to a hill. On the right are waves – but not waves of water or any other kind of liquid. These are dunes or very large ripples, blown by the wind into intricate patterns. Sharp eyes might spy boulders that have rolled downslope into this “sea” – there’s even a dotted track that one boulder made as it went. Can you find the boulder? (HiRISE ESP_038799_1590, NASA/JPL/Univ. of Arizona)