Mostrando entradas con la etiqueta the ExoMars Trace Gas Orbiter. Mostrar todas las entradas
Mostrando entradas con la etiqueta the ExoMars Trace Gas Orbiter. Mostrar todas las entradas

domingo, 12 de febrero de 2017

ESA : Angling up for Mars science .- Buscando la ciencia de Marte

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

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
 
7 February 2017
ESA’s latest Mars orbiter has moved itself into a new path on its way to achieving the final orbit for probing the Red Planet.
The ExoMars Trace Gas Orbiter arrived last October on a multiyear mission to understand the tiny amounts of methane and other gases in the atmosphere that could be evidence for biological or geological activity.
In January, it conducted a series of crucial manoeuvres, firing its main engine to adjust its orbit around Mars.
The three firings shifted its angle of travel with respect to the equator to almost 74º from the 7º of its October arrival. This essentially raised the orbit from equatorial to being much more north–south.
The arrival orbit was set so that it could deliver the Schiaparelli lander to Meridiani Planum, near the equator, with good communications.
Once science observations begin next year, the new 74º orbit will provide optimum coverage of the surface for the instruments, while still offering good visibility for relaying data from current and future landers.

Mission controllers at work

7 to 74: The angle of TGO’s orbit before and after the orbital inclination change manoeuvres in January/February 2017.
TGO orbital inclination - before and after
 
The change was achieved in three burns on 19, 23 and 27 January, overseen by the mission control team working at ESA’s operations centre in Darmstadt, Germany.
“The manoeuvres were performed using the main engine in three steps to avoid a possible situation where the spacecraft could end up on a collision course with Mars in case of any unexpected early termination or underperformance of the engine,” said spacecraft operations manager Peter Schmitz.
Peter notes the engine delivered very precise levels of thrust: “All three were completed to within just a few tenths of a percent of the target thrust, resulting in the craft’s orbital plane being off by just a few fractions of a degree, which is trivial.”
A final, minor trim was made on 5 February, at the same time lowering the altitude above Mars at closest approach from 250 km to 210 km.

Atmospheric drag a vuelo

The inclination change was also a necessary step for the next challenge: a months-long ‘aerobraking’ campaign designed to bring the spacecraft to its near-circular final science orbit, at an altitude of around 400 km.
Mission controllers will command the craft to skim the wispy top of the atmosphere, generating a tiny amount of drag that will steadily pull it down. The process is set to begin in mid-March, and is expected to take about 13 months.
 
ExoMars first year in orbit
                                

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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.
ESA
Guillermo Gonzalo Sánchez Achutegui
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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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jueves, 8 de diciembre de 2016

ESA : ExoMars orbiter images Phobos .- Imágenes del Satélite Fobos de Marte por ExoMars orbiter

http://www.esa.int/Our_Activities/Space_Science/ExoMars/ExoMars_orbiter_images_Phobos
http://www.esa.int/esl/ESA_in_your_country/Spain/El_orbitador_de_ExoMars_fotografia_Phobos
                                
Primera imagen en color de Phobos tomada por ExoMars

El orbitador de ExoMars fotografía Phobos

6 diciembre 2016
El Satélite para el estudio de Gases Traza (TGO) de ExoMars ha fotografiado la luna marciana Phobos durante el segundo conjunto de mediciones científicas de prueba realizado desde su llegada al Planeta Rojo el día 19 de octubre. 
El TGO, fruto de la colaboración entre ESA y la agencia rusa Roscosmos, llevó a cabo sus primeras mediciones científicas de calibración entre el 20 y el 28 de noviembre.
La semana pasada se publicaron datos de ejemplo de la primera órbita, centrados en el propio planeta. Durante la segunda órbita, los instrumentos realizaron una serie de mediciones de Phobos, una luna de 27 × 22 × 18 km que gira a tan solo 6.000 km de Marte. 
 
Phobos en 3D
 
El 26 de noviembre, la cámara del TGO capturó imágenes de esta luna a una distancia de 7.700 km, en el tramo de su órbita más cercano a Marte. Durante su órbita elíptica de 4,2 días, el TGO llega a situarse a 230-310 km de la superficie en el momento del periastro y a alejarse hasta unos 98.000 km en el apoastro.
La imagen compuesta en color se ha creado a partir de varias imágenes individuales tomadas con distintos filtros. Estos filtros se han optimizado para destacar las diferencias en la composición mineralógica, que en la imagen procesada se ven en tonos más azules o rojos.
También hay un anaglifo creado a partir de un par estereoscópico de imágenes, que puede verse con gafas 3D de color rojo-azul. 
“Aunque otras misiones, como las sondas Mars Express de la ESA y Mars Reconnaissance Orbiter de la NASA, han aportado imágenes en mayor resolución de Phobos, las capturadas en esta nueva órbita han servido para probar adecuadamente lo que podemos conseguir con nuestros datos en muy poco tiempo”, afirma Nick Thomas, investigador principal del equipo de la cámara CaSSIS de la Universidad de Berna, Suiza.
“Las imágenes nos han proporcionado una gran cantidad de información práctica sobre la calibración del color de la cámara y su temporización interna”.
Otros dos instrumentos también han llevado a cabo mediciones de calibración de Phobos, cuyos datos están siendo analizados por los equipos.
“Estamos muy satisfechos con los resultados de las dos órbitas científicas de prueba; además, los datos de calibración nos servirán para mejorar las mediciones una vez que comencemos con la misión científica principal el año que viene”, añade Håkan Svedhem, científico del proyecto TGO de la ESA. 
 
Segunda órbita científica de ExoMars
 
La misión ahora vuelve a centrarse en los preparativos para el aerofrenado, necesario para que el satélite entre en su órbita casi circular a finales de 2017. En breve ofreceremos más detalles sobres las próximas operaciones.
El principal objetivo científico del TGO es elaborar un inventario detallado de los gases poco comunes de la atmósfera, que constituyen menos del 1% de su volumen, incluyendo metano, vapor de agua, dióxido de nitrógeno y acetileno.
Resulta de especial interés el metano, que en la Tierra se produce sobre todo por actividad biológica y, en menor medida, durante procesos geológicos, como ciertas reacciones hidrotermales. 
La nave también buscará agua o hielo bajo la superficie, y ofrecerá imágenes contextuales en color y estereoscópicas de las formaciones superficiales, incluyendo aquellas que pudieran estar relacionadas con posibles fuentes de gases traza.
El TGO también funcionará como relé de datos para vehículos y robots actuales y futuros en Marte, como la segunda misión ExoMars, que incluirá un rover y una plataforma científica de superficie, y cuyo lanzamiento está previsto para 2020. 
 
Para más información: Nicolas Thomas
Center for Space and Habitability, University of Bern
Correo electrónico: nicolas.thomas@space.unibe.ch
Håkan Svedhem
ESA ExoMars TGO Project Scientist
Correo electrónico: hakan.svedhem@esa.int
Markus Bauer








ESA Science and Robotic Exploration Communication Officer









Teléfono: +31 71 565 6799









Móvil: +31 61 594 3 954









Correo electrónico: markus.bauer@esa.int
ExoMars first colour image of Phobos
 
ENGLISH VERSION:

ExoMars orbiter images Phobos

6 December 2016
The ExoMars Trace Gas Orbiter has imaged the martian moon Phobos as part of a second set of test science measurements made since it arrived at the Red Planet on 19 October.
The Trace Gas Orbiter (TGO), a joint endeavour between ESA and Roscosmos, made its first scientific calibration measurements during two orbits between 20 and 28 November.
Example data from the first orbit were published last week, focusing on Mars itself. During the second orbit, the instruments made a number of measurements of Phobos, a 27×22×18 km moon that orbits Mars at a distance of only 6000 km.
 
Phobos in 3D
 
The camera imaged the moon on 26 November from a distance of 7700 km, during the closest part of the spacecraft’s orbit around Mars. TGO’s elliptical orbit currently takes it to within 230–310 km of the surface at its closest point and around 98 000 km at its furthest every 4.2 days.
A colour composite has been created from several individual images taken through several filters. The camera’s filters are optimised to reveal differences in mineralogical composition, seen as ‘bluer’ or ‘redder’ colours in the processed image.
An anaglyph created from a stereo pair of images captured is also presented, and can be viewed using red–blue 3D glasses.
“Although higher-resolution images of Phobos have been returned by other missions, such as ESA’s Mars Express and NASA’s Mars Reconnaissance Orbiter, this provided a good test of what can be done with our data in a very short time,” says Nick Thomas, principal investigator of the CaSSIS camera team at the University of Bern.
“The images have given us a lot of useful information about the colour calibration of the camera and its internal timing.”
Two other instruments also made calibration measurements of Phobos, and the teams are analysing their data.
“We’re very happy with the results of both test science orbits and will be using these calibration data to improve our measurements once we begin the main science mission later next year,” adds Håkan Svedhem, ESA’s TGO Project Scientist.
 
ExoMars science orbit 2

The focus of the mission now returns to preparations for aerobraking required to bring the spacecraft towards its near-circular science orbit by the end of 2017. More details on the upcoming operations will be provided soon.
TGO’s main scientific goal is to make a detailed inventory of rare gases that make up less than 1% of the atmosphere’s volume, including methane, water vapour, nitrogen dioxide and acetylene.
Of high interest is methane, which on Earth is produced primarily by biological activity, and to a smaller extent by geological processes such as some hydrothermal reactions. 
The spacecraft will also seek out water or ice just below the surface, and will provide colour and stereo context images of surface features, including those that may be related to possible trace gas sources.
TGO will also act as a data relay for present and future landers and rovers on Mars, including the second ExoMars mission that will feature a rover and surface science platform, and which is scheduled for launch in 2020.
  ESA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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domingo, 30 de octubre de 2016

ESA : Thumbs up .- Con los pulgares hacia arriba del manager Peter Schmitz

http://www.esa.int/spaceinimages/Images/2016/10/Thumbs_up

On 19 October 2016, Spacecraft Operations Manager Peter Schmitz gives the thumbs up in the main control room at ESA’s ESOC mission control centre shortly after the ExoMars Trace Gas orbiter (TGO) arrived at the Red Planet

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  • Title Thumbs up
  • Released 27/10/2016 11:58 am
  • Copyright ESA/J. Mai
  • Description
    Spacecraft operations manager Peter Schmitz gives the thumbs up in the main control room at ESA’s control centre in Darmstadt, Germany, on 19 October 2016, shortly after the ExoMars Trace Gas Orbiter arrived at the Red Planet.
    The spacecraft fired its main engine for 139 minutes to slow it down to be captured by Mars, entering an elliptical 101 000 x 3691 km orbit (with respect to the centre of the planet). It is in excellent health and will start making observations to calibrate its science instruments during two circuits in November 2016.
    More information on ExoMars/TGO operations.
Traducción :
Gerente de operaciones de la nave Peter Schmitz da los pulgares para arriba en la sala de control principal en el centro de control de la ESA en Darmstadt, Alemania, el 19 de octubre de 2016, poco después de la traza ExoMars Gas Orbiter llegó al planeta rojo.

La nave espacial encendió su motor principal para 139 minutos para reducir la velocidad para ser capturado por Marte, entrando en una elíptica 101 000 x 3691 kilometros órbita (con respecto al centro del planeta). Está en excelente estado de salud y comenzará a hacer observaciones para calibrar sus instrumentos científicos durante dos circuitos, en noviembre de 2016.
  • Id 367757

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ESA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com
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