Category Archives: Asteroids & Comets

Philae lander on Comet 67P/C-G has been found

The European Space Agency (ESA) announced today that the Philae spacecraft, deployed from the Rosetta mother ship on November 14, 2014 to land on Comet 67P/Churyumov–Gerasimenko has finally been found. After several bounces it had ended up in a shadowed area. After a short time it went silent since the solar panels could not replenish its battery and before its location could be determined.

Philae found!

Less than a month before the end of the mission, Rosetta’s high-resolution camera has revealed the Philae lander wedged into a dark crack on Comet 67P/Churyumov–Gerasimenko.

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Rosetta’s lander Philae has been identified in OSIRIS narrow-angle camera images taken on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel. Philae’s 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae’s orientation. A Rosetta Navigation Camera image taken on 16 April 2015 is shown at top right for context, with the approximate location of Philae on the small lobe of Comet Churyumov-Gerasimenko marked.
The images were taken on 2 September by the OSIRIS narrow-angle camera as the orbiter came within 2.7 km of the surface and clearly show the main body of the lander, along with two of its three legs.

The images also provide proof of Philae’s orientation, making it clear why establishing communications was so difficult following its landing on 12 November 2014.

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Close-up of the Philae lander, imaged by Rosetta’s OSIRIS narrow-angle camera on 2 September 2016 from a distance of 2.7 km. The image scale is about 5 cm/pixel. Philae’s 1 m-wide body and two of its three legs can be seen extended from the body. The images also provide proof of Philae’s orientation. The image is a zoom from a wider-scene, and has been interpolated.

“With only a month left of the Rosetta mission, we are so happy to have finally imaged Philae, and to see it in such amazing detail,”

says Cecilia Tubiana of the OSIRIS camera team, the first person to see the images when they were downlinked from Rosetta yesterday.

“After months of work, with the focus and the evidence pointing more and more to this lander candidate, I’m very excited and thrilled that we finally have this all-important picture of Philae sitting in Abydos,”

says ESA’s Laurence O’Rourke, who has been coordinating the search efforts over the last months at ESA, with the OSIRIS and SONC/CNES teams.

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An OSIRIS narrow-angle camera image taken on 2 September 2016 from a distance of 2.7 km in which Philae was definitively identified. The image has been processed to adjust the dynamic range in order to see Philae while maintaining the details of the comet’s surface. Philae is located at the far right of the image, just above centre. The image scale is about 5 cm/pixel.
Philae was last seen when it first touched down at Agilkia, bounced and then flew for another two hours before ending up at a location later named Abydos, on the comet’s smaller lobe.

After three days, Philae’s primary battery was exhausted and the lander went into hibernation, only to wake up again and communicate briefly with Rosetta in June and July 2015 as the comet came closer to the Sun and more power was available.

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A number of Philae’s features can be made out in this image taken by Rosetta’s OSIRIS narrow-angle camera image on 2 September 2016. The images were taken from a distance of 2.7 km, and have a scale of about 5 cm/pixel. Philae’s 1 m wide body and two of its three legs can be seen extended from the body. Several of the lander’s instruments are also identified, including one of the CIVA panoramic imaging cameras, the SD2 drill and SESAME-DIM (Surface Electric Sounding and Acoustic Monitoring Experiment Dust Impact Monitor).
However, until today, the precise location was not known. Radio ranging data tied its location down to an area spanning a few tens of metres, but a number of potential candidate objects identified in relatively low-resolution images taken from larger distances could not be analysed in detail until recently.

While most candidates could be discarded from analysis of the imagery and other techniques, evidence continued to build towards one particular target, which is now confirmed in images taken unprecedentedly close to the surface of the comet.

At 2.7 km, the resolution of the OSIRIS narrow-angle camera is about 5 cm/pixel, sufficient to reveal characteristic features of Philae’s 1 m-sized body and its legs, as seen in these definitive pictures.

“This remarkable discovery comes at the end of a long, painstaking search,” says Patrick Martin, ESA’s Rosetta Mission Manager. “We were beginning to think that Philae would remain lost forever. It is incredible we have captured this at the final hour.”

[ Matt Taylor, ESA’s Rosetta project scientist says,]

“This wonderful news means that we now have the missing ‘ground-truth’ information needed to put Philae’s three days of science into proper context, now that we know where that ground actually is!” …

[ Holger Sierks, principal investigator of the OSIRIS camera adds,]

“Now that the lander search is finished we feel ready for Rosetta’s landing, and look forward to capturing even closer images of Rosetta’s touchdown site,” …

The discovery comes less than a month before Rosetta descends to the comet’s surface. On 30 September, the orbiter will be sent on a final one-way mission to investigate the comet from close up, including the open pits in the Ma’at region, where it is hoped that critical observations will help to reveal secrets of the body’s interior structure.

Further information on the search that led to the discovery of Philae, along with additional images, will be made available soon.

Video: TMRO 9.25 – Daniel Faber, Deep Space Industries

The latest episode of TMRO.tv is now available on line: Daniel Faber, Deep Space Industries – TMRO

Deep Space Industries is an asteroid mining company, changing the economics of the space industry by providing the technical resources, capabilities and system integration required to prospect for, harvest, process, manufacture and market in-space resources. These resources, found on easily accessible near Earth asteroids, will provide unlimited energy and supplies for a growing space economy. We are joined by DSI CEO Daniel Faber to talk about the new space economy and how mining asteroids can change the way we explore the cosmos.

TMRO:Space is a crowd funded show. If you like this episode consider contributing to help us to continue to improve. Head over to http://www.patreon.com/tmro for information, goals and reward levels. Don’t forget to check out our SpacePod campaign as well over at http://www.patreon.com/spacepod

Space mining CEO & OSIRIS-REx scientist to host Google Hangout to talk about asteroids and Xtronaut game

Chris Lewicki of the  asteroid mining company Planetary Resources and Prof. Dante Lauretta of the University of Arizona and a scientist on the OSIRIS-REx asteroid mission (see earlier posting) will host a Google Hangout at 11:00 am PT (2:00 pm ET, 6:00 pm GMT) on Friday: Chris Lewicki & Dante Lauretta talk about asteroids, launches, and Xtronaut: The Game of Solar System Exploration! – Google+.

Do you like playing board games? Do you like STEM education? Have you ever wanted to plan your own mission to space? Then you will love this!

You are invited to a Google Hangout on Air to learn about an amazing new game that mixes fun, STEM and space all together on one board.

Xtronaut: The Game of Solar System Exploration captures the challenges and fun of planning a space mission and combines real rocket science with mission planning, strategy, politics, and interactive play. We have been playing this game in the office and can assure you it is JUST like planning a real mission!

The game was envisioned by Planetary Resources advisor, Dante Lauretta, Ph.D. Dante is a Professor at the University of Arizona, Principal Investigator of the NASA OSIRIS-REx asteroid sample return mission, and founder of Xtronaut.

During the hangout, our President and CEO Chris Lewicki will challenge Dante to a game, and discuss the exciting developments in asteroid science and exploration with the upcoming launches of OSIRIS-REx and our Arkyd 6.

Sign up to participate: RSVP for the Hangout by clicking here.

You can also purchase Xtronaut: The Game of Solar System Exploration on Amazon.com.

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Videos: OSIRS-REx mission to the asteroid Bennu

On September 8th a ULA Atlas V rocket will launch the OSIRIS-REx (Origins, Spectral Interpretation, Resource Identification, Security-Regolith Explorer)  from Cape Canaveral. The spacecraft’s mission is to visit the asteroid Bennu and bring back a small sample of it to earth. Analysis of the sample will provide hints about the conditions of the early solar system and provide clues on such as to how water and organic molecules came to the Earth. The mission will also add to the general knowledge about asteroids including possible resources of use in space and on earth.

On Wednesday, NASA held a panel briefing to  discuss the meeting with the press:

This video describes the Bennu asteroid:

This video shows the trajectory of OSIRIS-REx reaches Bennu and returns to earth, taking advantage of the fact that the asteroid’s orbit is near earth and crosses earth’s:

Perseid meteor shower peak approaching

The annual Perseid meteor showers are underway. Here is a guide for observing the shooting stars: Viewing the 2016 Perseids – American Meteor Society

The Perseids are active from July 13th through August 26th. Maximum activity is predicted to occur on the morning of August 12th, when rates in excess of 1 per minute may be seen from dark sky sites. On the morning of maximum the waxing gibbous moon will set between midnight and 0100 local daylight time as seen from mid-northern latitudes. This will free up the prime observing hours from interfering moonlight.

A meteor shower happens when the Earth’s orbit crosses the trail of dust particles left by a comet. The Perseids are produced by the trail of Comet Swift-Tuttle as seen in this image:

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Although the dust particles are tiny, they are going so fast relative to the earth they can still produce a bright meteor when crashing through the atoms in the upper atmosphere.

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