ESA astronaut Thomas Pesquet with NASA astronauts Shane Kimbrough and Peggy Whitson shows how it’s done.
The Sentinel-2B Earth observation satellite will soon be launched and join the Copernicus program, the world’s largest environmental monitoring program which is headed by the European Commission in partnership with ESA.
Sentinel 1 and 2 are already in orbit and providing valuable data for science and safety. Data from the satellites prompted the evacuation of the Halley VI research station in Antarctica. The satellites are monitoring a large crack that formed in the Brunt Ice shelf, a floating ice shelf in the Weddell sea region The crack formed in October and was dubbed the Halloween Crack. The crack grew by as much as 600 meters a day during November and December and the British Antarctic Base (BAS) Halley VI found itself only 17 km away.
Now new cracks have formed and puts the base and the between 20 and 70 people in jeopardy. The base is mobile and has already moved 23 km inland. BAS used radar images from Sentinel-1 and optical images from Sentinel-2 to monitor the situation and out of an abundance of caution have decided to close the base at least temporarily.
Glad to see an update and that all is going along nicely with this ESA and Japanese mission to Mercury.
The galaxy above called IC-3639 has an Active Galactic Nucleus that is actually obscured which leads to even more questions. AGN’s are super-massive black holes (in the order of a million to probably hundreds of million solar masses) that are accreting massive amounts of matter, which is to say “feeding”. The accretion disc makes the Active Galaxies among the brightest objects in terms of electromagnetic radiation, so bright it is not often whether or not a galaxy is active, is in question, IC 3639 is such a galaxy.
A word about black holes in general because some people have a mistaken impression of black holes as marauding monsters roaming the universe looking for innocent planets to swallow up, that just came up on an outing with friends. No, a black holes don’t really do that. In fact if you took a black hole of one-solar-mass and swapped it with our Sun our solar system would just keep right on going just like it does now, aside from light and heat of course, the fabric of space-time would be just as it is now.
IC 3639, a galaxy with an active galactic nucleus, is seen in this image combining data from the Hubble Space Telescope and the European Southern Observatory.
This galaxy contains an example of a supermassive black hole hidden by gas and dust. Researchers analyzed NuSTAR data from this object and compared them with previous observations from NASA’s Chandra X-Ray Observatory and the Japanese-led Suzaku satellite. The findings from NuSTAR, which is more sensitive to higher energy X-rays than these observatories, confirm the nature of IC 3639 as an active galactic nucleus that is heavily obscured, and intrinsically much brighter than observed.
NuSTAR is a Small Explorer mission led by Caltech and managed by JPL for NASA’s Science Mission Directorate in Washington. NuSTAR was developed in partnership with the Danish Technical University and the Italian Space Agency (ASI). The spacecraft was built by Orbital Sciences Corp., Dulles, Virginia. NuSTAR’s mission operations center is at UC Berkeley, and the official data archive is at NASA’s High Energy Astrophysics Science Archive Research Center. ASI provides the mission’s ground station and a mirror archive. JPL is managed by Caltech for NASA.
Image and caption: NASA/JPL-Caltech/ESO/STScI
I remember this very well!
While this scene looks like the mesmerising result of shaking up a festive snow globe, it is in fact the disturbing effect of one of the most powerful solar storms ever recorded.
Over two weeks in October and November 2003 the Sun was unprecedentedly active, with giant sunspots – over 10 times the diameter of Earth – generating flares on an almost daily basis.
Solar flares are classed according to the energy they release at X-ray wavelengths. There are five major categories: A, B, C, M and X, further divided into 10 subclasses. M1 flares are 10 times more powerful than C1, and X1 flares are 10 times more powerful than M1 flares, or 100 times more powerful than C1.
Some of the flares witnessed in this two-week period were so powerful they broke right through the top of the X-class range, which is usually given as X10. A flare erupting on 4 November was estimated to have reached at least X28.
The ESA/NASA Solar and Heliospheric Observatory (SOHO), launched in 1995 and still operating today, was monitoring the Sun’s stormy behaviour during this time. This image shows its detectors being completely swamped by high-energy protons that were accelerated to nearly the speed of light (300 000 km/s) in the X17 flare of 28 October 2003.
When Earth is in the firing line of associated coronal mass ejections (CMEs), it can lead to beautiful and bright auroras in the atmosphere, giving unparalleled insight into the interaction of the Sun and Earth.
CMEs can also cause serious disruption to radio communications, air traffic control and power grids.
Although these powerful storms reveal the extremes of the Sun’s activity, fortunately for Earth, those on the scale of the 2003 events do not occur very often.
The image was taken by SOHO’s LASCO C3 instrument. A special disc (indicated by the large blue circle) inside the instrument blocks the Sun (indicated by the inner white circle), so that details of the extended outer solar atmosphere can be observed. Watch a movie of the event depicted in this scene, here.
Credits: SOHO (ESA & NASA)
Having examined and precisely measured the positions and brightness of over a BILLION stars, Gaia could well be the greatest mission nobody talks about.
ESA’s Gaia is surveying stars in our Galaxy and local galactic neighbourhood in order to build the most precise 3D map of the Milky Way and answer questions about its structure, origin and evolution.
Launched in 2013, Gaia has already generated its first catalogue of more than a billion stars – the largest all-sky survey of celestial objects to date.
To achieve its scientific aims, it points with ultra-high precision, and to enable the control team to monitor spacecraft performance, Gaia regularly reports to the ground information about its current attitude and the stars that have been observed.
These engineering data have been accumulated over 18 months and combined to create a ‘map’ of the observed star densities, from which a beautiful and ghostly virtual image of our magnificent Milky Way galaxy can be discerned, showing the attendant globular clusters and Magellanic clouds.
Where there are more stars, as in the Galactic centre, the map is brighter; where there are fewer, the map is darker. The map includes brightness data corresponding to several million stars.
More information on Gaia mission operations
The last of the NAVCAM images are now archived. The images in the latest archive release are from the Rosetta’s last month of activity during the fantastic mission around Comet 67P/Churyumov-Gerasimenko.
This and other images can be found with the ESA Archive Image Browser
ESA’s description of the image above, one of the last five from Rosetta’s NAVCAM taken on 30 September 2016:
Single frame enhanced NavCam image taken on 29 September 2016 at 23:25 GMT, when Rosetta was 19.4 km from the centre of the nucleus of Comet 67P/Churyumov-Gerasimenko. The scale at the surface is about 1.7 m/pixel and the image measures about 1.7 km across.
Image (and description): ESA/Rosetta/NAVCAM – CC BY-SA IGO 3.0
Here’s an update from an earlier post. Nice work from the HiRise camera on the Mar Reconnaissance Orbiter. You can see a larger version of the image above by clicking it. There is a larger version yet you can get from NASA which I recommend.
This Oct. 25, 2016, image shows the area where the European Space Agency’s Schiaparelli test lander reached the surface of Mars, with magnified insets of three sites where components of the spacecraft hit the ground. It is the first view of the site from the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter taken after the Oct. 19, 2016, landing event.
The Schiaparelli test lander was one component of ESA’s ExoMars 2016 project, which placed the Trace Gas Orbiter into orbit around Mars on the same arrival date.
This HiRISE observation adds information to what was learned from observation of the same area on Oct. 20 by the Mars Reconnaissance Orbiter’s Context Camera (CTX). Of these two cameras, CTX covers more area and HiRISE shows more detail. A portion of the HiRISE field of view also provides color information. The impact scene was not within that portion for the Oct. 25 observation, but an observation with different pointing to add color and stereo information is planned.
This Oct. 25 observation shows three locations where hardware reached the ground, all within about 0.9 mile (1.5 kilometer) of each other, as expected. The annotated version includes insets with six-fold enlargement of each of those three areas. Brightness is adjusted separately for each inset to best show the details of that part of the scene. North is about 7 degrees counterclockwise from straight up. The scale bars are in meters.
At lower left is the parachute, adjacent to the back shell, which was its attachment point on the spacecraft. The parachute is much brighter than the Martian surface in this region. The smaller circular feature just south of the bright parachute is about the same size and shape as the back shell, (diameter of 7.9 feet or 2.4 meters).
At upper right are several bright features surrounded by dark radial impact patterns, located about where the heat shield was expected to impact. The bright spots may be part of the heat shield, such as insulation material, or gleaming reflections of the afternoon sunlight.
According to the ExoMars project, which received data from the spacecraft during its descent through the atmosphere, the heat shield separated as planned, the parachute deployed as planned but was released (with back shell) prematurely, and the lander hit the ground at a velocity of more than 180 miles per hour (more than 300 kilometers per hour).
At mid-upper left are markings left by the lander’s impact. The dark, approximately circular feature is about 7.9 feet (2.4 meters) in diameter, about the size of a shallow crater expected from impact into dry soil of an object with the lander’s mass — about 660 pounds (300 kilograms) — and calculated velocity. The resulting crater is estimated to be about a foot and a half (half a meter) deep. This first HiRISE observation does not show topography indicating the presence of a crater. Stereo information from combining this observation with a future one may provide a way to check. Surrounding the dark spot are dark radial patterns expected from an impact event. The dark curving line to the northeast of the dark spot is unusual for a typical impact event and not yet explained. Surrounding the dark spot are several relatively bright pixels or clusters of pixels. They could be image noise or real features, perhaps fragments of the lander. A later image is expected to confirm whether these spots are image noise or actual surface features.
Figure 1 is an unannotated version of the full scene, which covers an area about 0.9 mile (1.5 kilometers) wide. It is a portion of HiRISE observation ESP_048041_1780.
The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA’s Science Mission Directorate, Washington.
Image Credit:NASA/JPL-Caltech/Univ. of Arizona
These “before and after” images from the Mars Reconnaissance Orbiter probably show Schiaparelli test lander. Initial reports show the thrusters did activate but failed at some point. We will know quite a lot more fairly soon. The decent data has been downlinked and is being studied. I am hearing reports the lander fell from 2 to 4 km; I thought the shield was supposed to separate at 7 km and the parachute was to be jettisoned and thrusters fired at just over 1 km, well below that reported altitude (link).
So we will wait and see. Here’s the image description from NASA (with source image links):
This comparison of before-and-after images shows two spots that likely appeared in connection with the Oct. 19, 2016, Mars arrival of the European Space Agency’s Schiaparelli test lander.
The images were taken by the Context Camera (CTX) on NASA’s Mars Reconnaissance Orbiter on May 29, 2016, and Oct. 20, 2016.
The area indicated with a black outline is enlarged at right. The bright spot near the lower edge of the enlargement is interpreted as likely to be the lander’s parachute, which was deployed and then released during the descent through the Martian atmosphere. The larger dark spot near the upper edge of the enlargement was likely formed by the Schiaparelli lander. The spot is elliptical, about 50 by 130 feet (15 by 40 meters) in size, and is probably too large to have been made by the impact of the heat shield. The location information confirmed by this image will aid imaging the site with the High Resolution Imaging Science Experiment (HiRISE) camera, providing more details to use in interpretation. The main image covers an area about 2.5 miles (4 kilometers) wide, at about 2 degrees south latitude, 354 degrees east longitude, in the Meridiani Planum region of Mars. The scale bars are in meters. North is up. The before and after images are available separately as Figure A (from CTX observation J03_046129_1800) andFigure B (from CTX observation J08_047975_1779).
CTX was built by and is operated by Malin Space Science Systems, San Diego. NASA’s Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA’s Science Mission Directorate, Washington.
Image Credit: NASA/JPL-Caltech/MSSS
Click the image for the annotated version.
The original caption:
The dusty side of the Sword of Orion is illuminated in this striking infrared image from the European Space Agency’s Hershel Space Observatory.
This immense nebula is the closest large region of star formation, situated about 1,500 light years away in the constellation of Orion. The parts that are easily observed in visible light, known alternatively as the Orion Nebula or Messier 42, correspond to the light blue regions. This is the glow from the warmest dust, illuminated by clusters of hot stars that have only recently been born in this chaotic region.
The red spine of material running from corner to corner reveals colder, denser filaments of dust and gas that are scattered throughout the Orion nebula. In visible light this would be a dark, opaque feature, hiding the reservoir of material from which stars have recently formed and will continue to form in the future.
Herschel data from the PACS instrument observations, at wavelengths of 100 and 160 microns, is displayed in blue and green, respectively, while SPIRE 250-micron data is shown in red.
Within the inset image, the emission from ionized carbon atoms (C+), overlaid in yellow, was isolated and mapped out from spectrographic data obtained by the HIFI instrument. A version without the inset is also available.
Herschel is a European Space Agency mission, with science instruments provided by consortia of European institutes and with important participation by NASA. While the observatory stopped making science observations in April 2013, after running out of liquid coolant as expected, scientists continue to analyze its data. NASA’s Herschel Project Office is based at JPL. JPL contributed mission-enabling technology for two of Herschel’s three science instruments. The NASA Herschel Science Center, part of IPAC, supports the U.S. astronomical community. Caltech manages JPL for NASA.