Here is a collection of tweets from this event.
[View the story “Moon, Mars and the Search for Life in the Universe” on Storify]
Here is a collection of tweets from this event.
[View the story “Moon, Mars and the Search for Life in the Universe” on Storify]
I like to tell the story of a Frenchman, who had an
announcement back in 1894 that he was going to swim the Atlantic. To be an adventure
you have to satify 3 conditions:
But we did that, we flew 240,000 miles and landed on
the rim of a 600m diameter crater.
Provided techniques that mission control and flight crews needed for all the
other Apollo missions, to land in more exotic places on the lunar surface.
So its been that way and I don’t have any answers on
how to change that, how to get the support levels guaranteed that we had in
Apollo, but we’ve really had nothing since then, and I feel sorry if I were in
Charlie Bolden’s shoes today, trying t balance what he’s having to balance and
being pulled in different directions without enough money. Its hard to get a
major program established and to be funded to go and execute it properly,
certainly in the near future.
WC: I can tell you that our attitude was both good and
bad over the history of the Apollo program. When the Apollo 1 fire happened,
there were so many things wrong with that spacecraft, and we were aware of a
lot of them, but we were over-confident, thought we could compensate for
things. But the vehicle was not as good as it should’ve been. They always assessed
changes assessed on costs, weight and schedule impacts. After they had the fire
and they started fixing everything, there were more than 1000 changes made after
Apollo 1, and the vehicle that we flew was near perfect. I think our attitude
that contributed to having that fire. When it came to Apollo 13 I was across
the street, Jack Swigert was pilot there, we had worked for months on
malfunction procedures. When the calls came into Mission control I listened for
15 mins, MC were doing all they could to prepare. I listened for 15 minutes and
went home and went to sleep because I went home knowing they had done
everything they could possibly do at that stage.
JM: I was backup crew until just before the fire. The
problem was we had a fire problem. We had had this problem right through
Mercury and Gemini into Apollo and we didn’t really appreciate that the
spacecraft had such pressurised oxygen that if you lit a cigarette that it
would light up on fire. We really didn’t face up to the fire problem until
after Apollo 1. Then we flew with nothing flammable in the spacecraft – even personal
effects were encased in an unflammable material.
JM: When we flew Gemini 4 they wanted us to keep the
helmets on with faceplates closed for 4 days so we wouldn’t breathe moisture
into the cabin as they were worried about whether things were sealed
>EM: I’d like to add to the remarks in a slightly
different vein. The future is going to be quite different to what it is right
now. We are overpopulating the planet, running out of resources, we are going
to have to look to space and other planets and other ways to keep this going.
The space effort and going to Mars and perhaps eventually beyond our solar
system that’s what its got to be about. I think the best testament for it now
is that we’re going to have trouble in this century keeping things going well.
Lets be bold, we’re in a very small solar system, that has right now endangered
since beginning of 20th century, consumption is totally out of hand,
we have some serious problems. Perhaps continuing to go into space and develop
tools is one of the ways out of this. I suggest we look at this.
We will be continuing exploration beyond Earth orbit
depending on numerous factors, it may be all US or it may be international
collaboration or maybe a mixture of the two. My advice would be to try to think
what things will be like by the time you individually are in your late 20s or
early 30s and pursue early job assignments to make you the best qualified for
whatever interests you. Then find something that interests you and go for it.
WC: If someone had told me in the 1950s that it was
possible to go to the Moon it would have been laughed as ridiculous. But if I
were to tell anyone in the audience they could go to Mars it’s a lot more
sensible than it was in the 50s talking about going to the Moon.
Reception to celebrate ESA astronaut Tim Peake on behalf of the UK Space Agency at the Houses of Parliament
I was excited to receive an invitation three days in advance of this reception on Monday 20th May and wondered with intrigue as to what the “ESA Astronaut announcement” would be. I leapt out of bed on the Sunday morning when the news broke on Twitter that Tim had been assigned to a five month mission in 2015, as by my previous calculations and hearsay on various forums, I had thought 2016 was the earliest he could hope for. A few hours later I had verified the content of the embargoed press release – Tim really was assigned to the November 2015 launch!
Thomas Reiter, David Willetts, Tim Peake and David Parker © Max Alexander 2013 Max Alexander/UK Space Agency |
I was unfortunately unable to attend the press conference on Monday morning at the Science Museum, where Thomas Reiter (Director of Human Spaceflight at the European Space Agency), David Willetts (Minister for Universities and Science) and David Parker (Head of the UK Space Agency) made the announcement that British astronaut Tim Peake was to fly a long duration five month mission to the International Space Station, launching on a Soyuz rocket from Baikonaur in November 2015.
We were delighted to join the event at the House of Commons, with Maggie Lieu, Richard Painter, Alex Dawn and Tom Nordheim of UKSEDS and myself and Abigail Calzada Diaz of SGAC in attendance.
Alex Dawn, Alistair Scott, David Willetts, Maggie Lieu, Jane MacArthur |
It was great to be able to congratulate Tim Peake in person after this momentous announcement and for us to keep a connection with him, after meeting him at the Farnborough International Airshow last year, and at his Space Boffins podcast and British Interplanetary Society talk earlier this year. Tim commented on his Twitter following being around 4,000 last week, 7,000 when he got off the plane during the weekend of the leaked announcement and 11,000 after the resulting media frenzy surrounding the press conference.
Tim will be relocating to Houston for training with his crewmates, and despite several years of training already, there is still more to learn, particularly with grappling the SpaceX Dragon during docking to the ISS and possibly Orbital Science’s Cygnus by 2015. It is too far ahead to have any idea as to whether he may do an EVA while on station, but all astronauts remain trained and prepared for this eventuality.
BIS President Alistair Scott looks forward to Tim Peake being the first BIS member in space!
Our first poster on Wednesday evening was from the Mars Analogue mission run in Morocco by the Austrian Space Forum. Ania Losiak had masterminded a mapping process for our science team which underpinned all the planning for the mission and became our main database of experimental results, as well as being an experiment in itself that we can compare what was planned to what actually happened, which we hope to be able to improve in future analogue missions.
Ania Losiak, our poster and me |
Note the toffees stuck to our display board, to encourage people to view
our poster – Ania is an expert at how to attract an audience
(considering there are over 8000 posters displayed during the week)!
On Thursday evening it was time for our post-Alpbach workshop poster, showing our improved Uranus mission and detailed trade study. My team mate Andrea also had her own poster 3 floors away and across the building, so it was convenient for me to present the post-Alpbach poster.
Me, Andrea Maier and Michaela Gitsch, the Alpbach Summer School Director |
After the full day at EGU I went to the European Space Policy Institute for evening talks and a reception, where I met a number of people from SGAC.
Friday evening was “Yuri’s Night”, a celebration of Yuri Gagarin’s first spaceflight 52 years earlier, where I was delighted to be reunited with many members of the Austrian Space Forum from the Mars 2013 mission.
Diedrich Moehlmann, DLR, set out to convince us that liquid
water can and does temporarily exist between two surfaces such as two grains of
rock in the upper surface of Mars today and to indicate where it may be found.
Water in the upper surface of present Mars, shown by hydrogen enriched
soil which is indicated by deep blue in this false-colour map of Mars
Credit: NASA/Feldman (Neutron spectrometer, Mars Odyssey) |
Moehlmann introduced the concept of ‘deliquescence’ – a
process that temporarily liquefies salts by uptake of atmospheric water.
Deliquescence is a key process to repetitively form liquid brines on present
Mars, as it can operate at remarkably low relative humidity. Iinner walls of
cracks could be temporarily covered, and narrow tips filled, by liquid
interfacial water.
Click here for the full abstract of his presentation at EGU 2013.
Monday morning saw huge advance queues eagerly awaiting the 8am registration opening. Planetary sessions started about Mercury, though notably the first speaker had withdrawn to the new NASA policy of no conference travel expenses following sequestration. This is to be a theme of the conference, though in some cases other co-authors have managed to step in on behalf of absent colleagues.
John Grotzinger, Sushil Atreya, Sylvestre Maurice, Javier Gómez-Elvira, Igor Mitrofanov |
The much anticipated event of the day was the MSL Curiosity press conference at 11am, with John Grotzinger and colleagues delivering the latest discoveries from this amazing mobile laboratory on Mars.
The results were neatly summarised by Jonathan Amos for the BBC, while some of the more detailed graphs and information are on the JPL website. For further details on the speakers and the full recorded press conference stream, click here.
The afternoon continued with a 90 minute session of more detailed updates from MSL, standing room only in one of the largest conference rooms due to its popularity. This was also streamed online and can be found here. The other half of the MSL update session is on Wednesday morning, streaming from 10:30 (CEST) on the same page.
Professor Tilman Spohn gave the Runcorn-Florensky Medal lecture, exploring the thermal history of planetary objects: “From Asteroids to super-Earths, from plate-tectonics to life”.
The European Geosciences Union General Assembly takes place from 7-13th April 2013. Over 11,000 attendees are registered at this largest meeting for geoscientists in Europe, I’m honoured to have my blog featured on their official blog roll.
I look forward to covering the Mars and lunar session, starting with the MSL press conference this morning at 11am (CET) together with a smattering of volcanology and geology over the week.
If you are here, don’t forget to download the EGU app, which makes it much easier to browse the mammoth programme and flag up what you want to attend, as well as having a dedicated inbuilt Twitter feed tracking the hashtag #EGU2013.
If you want to take a breather at some point, I can highly recommend the Natural History Museum. Show your EGU2013 pass to get a discount (5 euro entry fee) and don’t miss room five with the 900kg meteorite – see my next blog post! Amazing collection of meteorites including Mars and lunar samples.
The Natural History Museum boasts the oldest meteorite collection in the world, with the first two pieces entering the collection in 1778. It pre-dates the study of meteoritics and is one of the largest collections.
This 300kg meteorite Knyahinya, greets you as you enter the room, from a witnessed fall in 1866 in the Ukraine Carpathians. For a long time this frgament was the largest known stony meteorite.
Knyahinya |
Fantastic informational displays and interactive “is this a meteorite?” stands keep it interesting for the family, for example with a magnifier you can move along over a whole range of different types of meteorite with the corresponding information appearing on screen as you move it.
Pieces of the Moon
The first of these, a breccia, was found in Oman, while the others are the main mass and slice of a meteorite Dar al Gani found in Libya. The central piece is one of the largest ever found at 400g, from the lunar highlands.
(Click the picture for full size to read) |
Chassigny |
Shergotty |
Carbonaceous Chondrites
These contain carbonaceous inclusions, the small white spots, which were the first solids to condense in the solar nebula, making them among the most primitive meteorites known.
Fossil meteorites
I was interested to learn about fossil meteorites from these two specimens which landed on the sea floor and were embedded in sediment. With time, this formed hard limestone, the sea withdrew and they have been recovered from the Thorsberg quarry in southern Sweden where more than 100 specimens have been found, almost all the ones found to date are from this site. The shape remains intact, but most of the meteoritic material has been replaced by other materials, apart from a few tiny crystals of chromite.
Other meteorites
You can’t ignore the largest piece in
the Austrian collection, this 909kg iron meteorite, from the Youndegin
fall in Western Australia, found in 1884, though apparently a 2625kg
meteorite was later discovered and also attributed to this fall.
Eagle Station |
This is of course just one room of the huge museum, well worth making time if you are ever in Vienna!
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We met Dallas Campbell, star of Supersized Earth and other documentaries including a particularly great programme about the Voyager spacecraft, as well as shuttle astronaut Jon McBride, who flew as pilot on Challenger for mission STS-41-G back in 1984. He was very gracious about signing autographs for the long lines of young people, excited to meet an astronaut.
Professor Charles Cockell |
Dr Ignas Snellen from Leiden University mourned the fact that with the Terrestrial Planet Finder and Darwin missions having been cancelled, it is unlikely there will be a dedicated space telescope to search for biomarker gases in exoplanet atmospheres within his lifetime. He reviewed the exciting results from ground-based telescopes and extrapolated to what may be obtained with the planned E-ELT in terms of better data in the future.
Dr Giovanna Tinetti, UCL,summarised how it is crucial to have more information about exoplanet atmospheres in order for further progress. The number of discoveries of exoplanets is increasing at a fast pace, yet with only weight, size and orbital information for about one third of them, and atmospheric temperature and compositional information for less than 20, it is not yet possible to have any detailed classification system.
Dr Tinetti, Dr Snellen & Prof Cockell |
For gas exoplanets, looking at chemical compositional ratios via spectroscopy such as carbon to oxygen ratio, and the amount of hydrogen escaping will give clues as to planetary formation and evolution, while albedos, thermal emissions and the day/night variation give information about the energy budget and planet-star interaction. For terrestrial planets, finding out if they have an atmosphere, and how evolved the atmosphere is will also help to answer planetary formation and evolution questions.
Some of the current issues facing exoplanets research are:
– Needing better resolution spectroscopy to improve and constrain our knowlege of exoplanet atmospheres
– Better absolute calibration between different instruments. Much continuing research is from combining data sets from different instruments but this can only give answers as good as the absolute calibration.
– Data is sparse, with not enough wavelength coverage and often not simultaneous measurements
– Very low signal to noise ratio (SNR) observations
– Stellar activity is largest source of astrophysical noise
Habitable Worlds With No Signs Of Life
Professor Charles Cockell, University of Edinburgh, started off by dividing all habitats into three:
1) Uninhabitable
2) Habitable & inhabited
3) Habitable but uninhabited: these show no surface signatures of life, perhaps a planet two young for an origin of life, or conditions too transient or inappropriate, or perhaps origin of life is very rare
60-80% of biomass on the Earth is cryptic, which means it would not show clear surface signatures although there may be hidden signatures, cryptic habitats, for example organisms living in the interior of surface rocks, in salts, in the deep subsurface or ice sheets as in the slide below.
We need to know a lot more about biotic atmospheres in order to
be able to tell them apart. Better resolution imagery and spectroscopy
will not currently be able to unequivocally determine if a world is
inhabited or not, as most habitated worlds in the cosmos will have no
remotely detectable signs of life.
Professor Cockell took the following hypothesis, saying it needs to be rejected if we are to find life: “Most habitable worlds in the cosmos will have no remotely detectable signs of life”. For this to be rejected, he suggests the following conditions:
1) When planets are habitable, the origin of life usually occurs
2) Once life originates it will usually evolve metabolisms that produce unequivocal biosignature gases which have spectral properties that clearly distinguish them from abiotic materials
3) Once organisms evolve, they will colonise a planet at high biomass
4) Once the planet is colonised, they will produce enough surface biosignatures at sufficient concentrations to be detectable to alien observers.
He suggested that currently the most reliable biosignature is oxygen at high concentration, and particularly if it is found to be in disequilibrium.
Professor Steve Miller, UCL, concluded the successful meeting with the following remarks:
“It is 21 years since Aleksander Wolszczan and Dale Frail (21/4/92) found the first exoplanet orbiting a pulsar, and 18 years
since Michel Mayor and Didier Queloz found the second exoplanet (6/10/95) orbiting a main sequence star, so however you measure it, Exoplanetology has “come
of age”!”
He summarised the meeting as having a feeling of impatience,
as more data, more missions, more instruments are wanted and needed to
satisfy the thirst for knowledge held by researchers in the exoplanet community.
Further information:
There is an EChO conference (Exoplanet Characterisation Observatory mission) being held at ESTEC, on 1-3rd July 2013.