Mostrando entradas con la etiqueta The ExoMars 2016 misión. Mostrar todas las entradas
Mostrando entradas con la etiqueta The ExoMars 2016 misión. Mostrar todas las entradas

domingo, 18 de diciembre de 2016

ESA : Skimming an alien atmosphere .- Desnatando una atmósfera extraña

http://www.esa.int/Our_Activities/Operations/Skimming_an_alien_atmosphere

The ExoMars Trace Gas Orbiter is on a multiyear mission to understand the tiny amounts of methane and other gases in Mars’ atmosphere that could be evidence for possible biological or geological activity.
Trace Gas Orbiter at Mars
 
16 December 2016
After the smooth arrival of ESA’s latest Mars orbiter, mission controllers are now preparing it for the ultimate challenge: dipping into the Red Planet’s atmosphere to reach its final orbit.
The ExoMars Trace Gas Orbiter is on a multiyear mission to understand the tiny amounts of methane and other gases in Mars’ atmosphere that could be evidence for possible biological or geological activity.
Following its long journey from Earth, the orbiter fired its main engine on 19 October to brake sufficiently for capture by the planet’s gravity.
It entered a highly elliptical orbit where its altitude varies between about 250 km and 98 000 km, with each circuit taking about four Earth days.
Ultimately, however, the science goals and its role as a data relay for surface rovers mean the craft must lower itself into a near-circular orbit at just 400 km altitude, with each orbit taking about two hours.

Aerobraking: the ultimate challenge

Mission controllers will use ‘aerobraking’ to achieve this, commanding the craft to skim the wispy top of the atmosphere for the faint drag to steadily pull it down.
“The amount of drag is very tiny,” says spacecraft operations manager Peter Schmitz, “but after about 13 months this will be enough to reach the planned 400 km altitude while firing the engine only a few times, saving on fuel.”
 
 
During aerobraking, the team at ESA’s mission control in Darmstadt, Germany, must carefully monitor the craft during each orbit to ensure it is not exposed to too much friction heating or pressure.
The drag is expected to vary from orbit to orbit because of the changing atmospheric, dust storms and solar activity. This means ESA’s flight dynamics teams will have to measure the orbit repeatedly to ensure it does not drop too low, too quickly.
The aerobraking campaign is set to begin on 15 March, when Mars will be just over 300 million km from Earth, and will run until early 2018.

Stepping up to the start

ExoMars/TGO mission controllers at ESOC are now working intensively to prepare the craft, the flight plan and ground systems for the campaign.
Mission controllers
 
Mission controllers are now working intensively to prepare the craft, the flight plan and ground systems for the campaign.
First, on 19 January, they will adjust the angle of the orbit with respect to the Mars equator to 74º so that science observations can cover most of the planet.
Next, to get into an orbit from where to start aerobraking, the high point will be reduced on 3 and 9 February, leaving the craft in a 200 x 33 475 km orbit that it completes every 24 hours.
ESA mission controllers have some previous experience with aerobraking using Venus Express, although that was done at the end of the mission as a demonstration. NASA also used aerobraking to take the Mars Reconnaissance Orbiter and other spacecraft into low orbits at Mars.
“This will be our first time to use aerobraking to achieve an operational orbit, so we’re taking the extra time available now to ensure our plans are robust and cater for any contingencies,” says flight director Michel Denis.

Beginning to slow down

Aerobraking proper will begin on 15 March with a series of seven thruster firings, about one every three days, that will steadily lower the craft’s altitude at closest approach – from 200 km to about 114 km.
 
Flight dynamics experts at our ESOC operations centre work on every ESA mission, from those in very low orbits, like Swarm and CryoSat, to those exploring our Solar System, like Rosetta and ExoMars.
Flight dynamics team
 
“Then the atmosphere can start its work, pulling us down,” says Peter Schmitz. “If all goes as planned, very little fuel will then be needed until the end of aerobraking early in 2018, when final firings will circularise the 400 km orbit.”
No date has been set, but science observations can begin once the final orbit is achieved. In addition, the path will provide two to three overflights of each rover every day to relay signals.

Spacecraft A-OK

Overall, the spacecraft is in excellent health. On 30 November, it received an updated ‘operating system’. To date, only one ‘safe mode’ has been triggered, when a glitch caused the craft to reboot and wait for corrective commands. That happened during preliminary testing of the main engine, when a faulty configuration was quickly identified and fixed.
"We are delighted to be flying such an excellent spacecraft,” says Michel. “We have an exciting and challenging mission ahead of us.”

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ESA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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domingo, 23 de octubre de 2016

NASA : La Sonda Espacial MRO de la NASA Localiza a Schiaparelli

https://www.lanasa.net/
http://www.esa.int/Our_Activities/Space_Science/ExoMars/Mars_Reconnaissance_Orbiter_views_Schiaparelli_landing_site

22.10.16.- La sonda espacial Mars Reconnaissance Orbiter (MRO) de la NASA ha identificado nuevas marcas en la superficie del Planeta Rojo que se cree están relacionadas con el módulo de aterrizaje de pruebas Schiaparelli de la misión ExoMars de la Agencia Espacial Europea (ESA), que llegó a Marte el 19 de Octubre.
La nueva imagen muestra un punto brillante que puede ser el paracaídas de Schiaparelli, y una mancha oscura grande interpretada como el resultado de los efectos de la propia sonda después de una caída libre con un tiempo mayor de lo previsto, después de que los propulsores se apagasen antes de tiempo. La imagen fue tomada por la cámara de Contexto (CTX) de la sonda espacial MRO de la NASA en Marte.
La información de la ubicación obtenida por la imagen de cámara CTX será utilizada para obtener más imágenes con la cámara de alta resolución HiRISE de MRO. Los investigadores de la Agencia Espacial Europea (ESA) y la NASA analizarán las imágenes para obtener información sobre la secuencia de eventos en el día del aterrizaje de Schiaparelli, posiblemente complementando los datos transmitidos desde el módulo de prueba durante su descenso.
La ubicación del punto brillante interpretado como el paracaídas es 353,79 grados de longitud este, 2,07 grados de latitud sur, y está muy de cerca del cálculo de la ESA para el lugar de aterrizaje sobre la base de datos del día del aterrizaje. Esto está dentro de la zona de aterrizaje prevista y aproximadamente a 5,4 kilómetros al oeste del centro del lugar de aterrizaje. Una mancha oscura más grande y elíptica, aproximadamente de 15 por 40 metros podría ser el módulo de aterrizaje que llegó a la superficie del suelo y presenta un color más oscuro.

Esta comparación del antes y el después de las imágenes muestra dos puntos que probablemente surgieron en relación con la llegada a Marte del módulo de aterrizaje Schiaparelli de la Agencia Espacial Europea el 19 de octubre. Las imágenes son de la Cámara de Contexto de la sonda espacial MRO de la NASA, actualmente orbitando Marte. Image Credit: NASA/JPL-Caltech/MSSS

Los Datos del Descenso de Schiaparelli Continúan Analizándose

 
ESTADO ACTUAL DE LA MISIÓN
20.10.16.-
Los datos clave que el módulo demostrador Schiaparelli envió ayer al Satélite para el estudio de Gases Traza durante su descenso a la superficie de Marte ya se han transmitido a la Tierra y en estos momentos están siendo analizados por expertos.
Los primeros indicadores de las señales de radio, capturadas tanto por el Giant Metrewave Radio Telescope (GMRT), un conjunto experimental de telescopios situado cerca de Pune, India, como por el orbitador Mars Express de la ESA, sugieren que el módulo habría completado con éxito la mayoría de los pasos de su descenso de 6 minutos a través de la atmósfera marciana: por ejemplo, la deceleración mientras atravesaba la atmósfera y el despliegue del paracaídas y el escudo térmico. 
Sin embargo, tanto el GMRT como Mars Express dejaron de recibir señales poco antes del momento previsto para el contacto del módulo con la superficie del planeta. Las discrepancias entre los dos conjuntos de datos están siendo analizadas por expertos de la ESA en el Centro de Operaciones Espaciales de Darmstadt, Alemania. 

La telemetría detallada grabada por el TGO era necesaria para comprender mejor la situación. Mientras Schiaparelli efectuaba su descenso, el orbitador llevaba a cabo una maniobra crucial de inserción orbital en Marte, que completó satisfactoriamente. Estos datos de gran importancia fueron registrados por Schiaparelli y reenviados a la Tierra a primeras horas de la mañana de hoy. 
Tras su análisis parcial, estos datos confirman que las fases de entrada y descenso se llevaron a cabo según lo programado, y que los acontecimientos empezaron a desviarse de lo previsto tras el desprendimiento del escudo térmico posterior y el paracaídas. Parece que tal desprendimiento se produjo antes de lo previsto, aunque el análisis aún no ha concluido. 
También se ha confirmado que los propulsores se activaron brevemente, aunque parece que se apagaron antes de lo esperado, a una altitud aún por confirmar. 
“Tras los acontecimientos de ayer, contamos con un impresionante satélite orbitando alrededor de Marte, listo para llevar a cabo misiones científicas y transmitir datos de la futura misión ExoMars 2020 —afirma Jan Wörner, director general de la ESA—. El principal objetivo de Schiaparelli era probar las tecnologías de aterrizaje europeas. Parte de su labor era registrar los datos durante el descenso y es importante que sepamos qué ha pasado para tomar medidas de cara al futuro”. 
David Parker, director de Vuelos Tripulados y Exploración Robótica de la ESA, añade: “En lo relativo al módulo de prueba Schiaparelli, los datos que estamos recibiendo nos permitirán entender a la perfección la secuencia de los hechos y por qué no se produjo un aterrizaje suave”. 
“Desde el punto de vista de la ingeniería, eso es precisamente lo que esperamos de un artefacto de pruebas y, gracias a él, ahora disponemos de datos extremadamente valiosos con los que trabajar. Formaremos una comisión de investigación para estudiar a fondo los datos, pero por el momento no podemos especular más allá”. 
NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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lunes, 10 de octubre de 2016

ESA : Call for media: ExoMars arrives at the Red Planet .- Llamado a los medios de comunicación: ExoMars llega al planeta rojo

http://www.esa.int/Our_Activities/Space_Science/ExoMars/Call_for_media_ExoMars_arrives_at_the_Red_Planet
ExoMars 2016 approaching Mars

Call for media: ExoMars arrives at the Red Planet

7 October 2016
The ExoMars 2016 mission will enter orbit around the Red Planet on 19 October. At the same time, its Schiaparelli lander will descend to the surface. Representatives of traditional and social media are invited to attend a two-day event at ESA’s ESOC control centre in Darmstadt, Germany.
ExoMars is a joint endeavour between ESA and Russia’s Roscosmos space agency, and comprises the Trace Gas Orbiter (TGO) and the Schiaparelli entry, descent and landing demonstrator.
TGO will make a detailed inventory of Mars’ atmospheric gases, with particular interest in rare gases like methane, which implies that there is an active, current source. TGO aims to measure methane’s geographical and seasonal dependence and help to determine whether it stems from a geological or biological source.
TGO will start its science mission at the end of 2017, following a year of complex aerobraking manoeuvres to circularise its orbit. It will also act as a relay for ESA’s ExoMars 2020 rover.
Schiaparelli will separate from TGO on 16 October, entering the atmosphere for a six-minute descent to a region in Meridiani Planum, on 19 October.
 
 
 
It will test a range of technologies to enable a controlled descent and landing on Mars in preparation for future missions, including a heatshield, a parachute, a propulsion system and a crushable structure.
Schiaparelli also carries a small science package that will record the wind speed, humidity, pressure and temperature at its landing site, as well as obtain the first measurements of electric fields on the surface of Mars that may provide insight into how dust storms are triggered.
The separation of Schiaparelli from TGO will be covered online. Media are invited to join mission experts at ESOC on 19 October to follow the orbit insertion of TGO and the landing of Schiaparelli, and to attend a briefing on 20 October when the first descent camera images are expected.

Provisional schedule at ESOC, 19–20 October

(all times in CEST, programme/times subject to change)
19 October
15:00–22:00 (Doors open at 14:00)
The event programme for media and ExoMars project members will bring both groups together to follow the highlights of the orbit insertion of TGO and of the entry, descent and landing of Schiaparelli. During the programme confirmations for mission success of TGO and Schiaparelli are expected. On stage, ExoMars engineers and scientists from ESA, Roscosmos and partner agencies will relay the technical and operational challenges of landing on Mars and will explain the scientific questions that are driving these ambitious Mars robotic exploration programme. Operational status updates will be broadcasted live from the ExoMars control room into the stage programme.
There will be live video connections to an Italian ExoMars event taking place in Rome and to the postflight tour of ESA astronaut Tim Peake, who will stop by in London.
The event will also be live-streamed online at
and will be broadcasted over satellite.
A special ESA social-TV programme will be available via Facebook Live on ESA’s Facebook page at http://www.facebook.com/ESA.
20 October
10:00–11:00 (Doors open at 09:00)
This media briefing will summarise the events of the night before, during which more telemetry and data are expected to arrive from TGO and Schiaparelli. ExoMars engineers, scientists and project managers will provide briefings on TGO and Schiaparelli. Images taken during the descent from Schiaparelli will also be presented.
The media briefing will be streamed live online at
and broadcast over satellite.
Media accreditation
Media representatives holding a valid press-ID should register here.
Social media users such as Youtubers, Tweeps, Bloggers, etc. may apply for social media credentials here.
Given the expected high demand and limits owing to logistical, security and health and safety constraints, it is possible that not all applications will be successful. Applicants will be informed whether they have been successful at the latest on 11 October.

Follow online
Separation will be reported online on 16 October at 17:20 GMT /19:20 CEST.
The media briefings scheduled for 19 and 20 October will be live streamed via
Realtime coverage of operational milestones in the lead up to separation on 16 October through until landing and orbit insertion on 19 October and in the days after will be provided in a frequently updated article at
Milestones will also be reported via Twitter and Facebook. Follow @esaoperations, @ESA_TGO, @ESA_EDM and @ESA_ExoMars or #ExoMars.
A special ESA social-TV programme will be available on ESA’s Facebook page at
For detailed background information on the mission, see:

For further information, please contact:
ESA Media Relations Office
Tel: +33 1 53 69 72 99
Email: media@esa.int
ESA
Guillermo Gonzalo Sánchez Achutegui
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