Tag Archive for 'science'

[Science] A natural nuclear reactor on Mars? Not likely…

A nuclear explosion on Mars? Not likely...

A nuclear explosion on Mars? Not likely…

An article by SF writer Charles Stross has been doing the rounds over the past week, describing an LPSC abstract which mentions “evidence” for a possible ancient nuclear explosion on Mars, caused by a “natural nuclear reactor” going critical. A lot of folks seem to be getting a bit excited by this because (not unreasonably) they think that since it’s published it must be scientifically valid, and I feel obliged to put on my party pooper hat and point out that it probably isn’t.

So first things first – here’s the LPSC abstract.

Now, you may be surprised to know that there IS actually such a thing as a “natural nuclear reactor”. We have evidence that at least one existed on Earth – at Oklo in Ghana – and you can read all about it on its wikipedia page. Essentially, you can get circumstances occurring in nature that are similar to those that occur in a nuclear fission reactor, if you have the right combination of geology, radioactive ore bodies and groundwater acting as a moderator. (you’ll note that the Mars “reactor” got a mention on the wikipedia page – that’s likely to be disappearing soon, given the scrutiny the abstract is now receiving).

So, why should we be skeptical of this LPSC abstract?

Peer review

Peer-review is a pretty important part of scientific methodology – it’s the process by which ideas are discussed and scrutinised and criticised and accepted (or rejected) by the scientific community. For a paper to be accepted for publication it must pass the peer-review process, which means that experts in the field have looked at the science, examined the evidence, and possibly duplicated any described experiments themselves and verified that the conclusions reached are valid. If they don’t then the paper is rejected, and the authors must either do more work to demonstrate their hypothesis or just start again and try another approach (or move on to something else). However, the article being discussed here is not a paper, it’s a conference abstract.

Conference Abstracts are not the same as papers. Conference abstracts are normally short summaries of work in progress – especially for teams working on ongoing missions – or interesting hypotheses that could be considered, and they may or may not be developed into papers later on (LPSC, DPS, and AGU are three of the big planetary conferences where abstracts are presented). Some are presented at the conference as posters or talks where they can be discussed further. Some of them get shot down, some pass scrutiny – that’s how science works. I’ve submitted and presented a few LPSC abstracts myself while I was at university – some worked out, some didn’t. The important thing though is that they are not peer-reviewed at all.

At this point I would like to strenuously and enthusiastially point out that the vast majority of abstracts submitted to LPSC are perfectly good science written by scientists and students of science. However, because (as far as I’m aware) the abstracts are not checked or vetted after they’re submitted, a handful of abstracts about… well, I’ll be charitable and call them “less likely scenarios” do slip through. For example, I remember reading one abstract a few years back suggesting that the sun had accreted around a neutron star – which makes no sense in terms of stellar formation/evolution at all. It probably got a few chuckles from those who noticed it, but otherwise it passed by unnoticed at the conference itself because its authors didn’t show up to elaborate on it (granted, a lot of authors aren’t able to turn up to LPSC for many reasons – but if you have a controversial idea then it helps if you show up to defend it!).

So – the important thing to be aware of here is that this is an LPSC abstract that has not been peer-reviewed, which means that its conclusions should be viewed with quite a bit of skepticism.

What about the science though?

There are questions to be raised about the author’s credibility – it doesn’t help that he previously authored an article suggesting that the so-called “Face on Mars” was created by an ancient martian civilisation (even if there ever was any doubt about its origins – not that I think there was – we now have plenty of evidence to show that it’s a completely natural feature). But be that as it may, the proper way to proceed is to analyse the science. Unfortunately, it seems to me that the science in the paper is not very good. Here are a few issues I found:

a) he says that the “reactor” was “tamped” by the overlying rock but doesn’t provide any calculations to support this (and for all I know he forgot that Mars has lower gravity than Earth, so pressure is lower at a given depth). That’s a fairly critical part of the scenario that we just have to take his word for.

b) He also doesn’t provide a satisfactory explanation of how the radioactive ore body forms and how it’s concentrated on Mars in the first place (radioactive ores are not usually concentrated by asteroid impacts).

c) He doesn’t provide any evidence for this supposed explosion beyond “it looks like the radioactive stuff was concentrated around a depression” which could have been caused by a number of other means (e.g. it could have been an depression caused by an ancient asteroid impact). Occam’s Razor seems sorely lacking.

d) I didn’t see a source mentioned for the maps of K and Th distribution presented in the abstract.

e) We know of precisely one natural nuclear reactor on Earth, which implies that they’re somewhat unlikely to form… and it didn’t blow up. And yet there was supposedly one on Mars that did? Seems like a lot of unlikely coincidences would have to line up to make that happen on the next planet over from us.

f) And he spends a lot of time telling us his interpretation of the data, and not a lot of time just objectively describing the data and saying what other options could explain it.

g) if this happened so long ago, why would there be evidence left on the surface after a billion years of deposition and erosion (and redeposition) by the winds that scour the surface of Mars? Surely that would have redistributed the material (if not hidden it)?

And this is before I even get to the nuclear physics side of it… I’ll leave that for others more knowledgeable about the subject. Either way, while some discussion and dissection of the evidence is happening now on various internet fora (now that it’s got some attention), so far the verdict is that the evidence to support the hypothesis is lacking.

So in the end I’d say that the “evidence for a nuclear reactor on Mars” – particularly one that exploded and blasted radioactive material across the planet – seems to be rather unconvincing! It’s an interesting idea to examine and dissect (that’s pretty much why it’s there, after all), but this does show that we need to always critically assess what we see on the internet so that we don’t mistake unreviewed conference abstracts for peer-reviewed science!

[b]Addendum[/b]: And funnily enough, this LPSC abstract even gets a mention in this rather excellent video (around the 2:47 mark) explaining how the popular media often doesn’t really understand the science it reports.

[Stellar Mapping] Brown Dwarf dataset added, plus some major updates!

I’ve added a new Brown Dwarf dataset to the Stellar Mapping page (thanks to LiNeNoiSe for pointing this out to me)! This should hopefully be the last major update to the stellar datasets for a while – the next project on the list is to figure out what the reworked Arms for 2300AD might look like based on the realistic data.

The new catalogue is the LDwarf dataset – this is a list of brown dwarfs taken from the IPAC Brown Dwarf Archives (this dataset was last updated on 14 Feb 2011). It is not a complete list of all known brown dwarfs – these are the only the ones for which parallax data is provided there.

L Dwarf dataset, looking Corewards

While some of the distances presented in this dataset are derived from trigonometric parallaxes, others are derived instead from (spectro)photometric parallaxes. Trigonometric parallaxes are derived by measuring the angular shift of a star relative to the background stars as the earth moves around the sun on its orbit (the stellar distances in the HIPX, RECONS and other datasets here are derived using this method) – these are generally more accurate than photometric parallaxes. “Photometric parallaxes” are techically not really “parallaxes” at all – instead the spectral type of the object is checked against luminosity models to get an estimate of its luminosity, which is used along with the observed visual/IR magnitude to calculate the distance to the object. Unfortunately this method is not very precise, and some of the photometric parallaxes for these objects in the LDwarf dataset have very large error bars – but this is the best data that is currently available.

One of these systems – SDSS J141-134 – is listed in the original data as having a (photometric) parallax of 127 +/- 27 mas. This places it almost in the right location to allow a 7.7 ly link between Xi Bootis and CE Bootis, which would be very useful in the 2300AD setting. I have changed its parallax to 122 mas on this list (which is comfortably within its error bars, and allows it to connect those two stars and link to the stars around Arcturus). The original (127 mas) data for this system is listed in the text file in the LDwarf.zip file if it’s needed.

It should also be noted that two Brown Dwarfs (UGPS J072227.51-054031.2 and DENIS J081730.0-615520) are located within the RECONS sphere. These are not listed in the RECONS data, but are retained here since their parallaxes indicate that they are within 22.8 lightyears of Sol (even given their large error bars). They do not make a significant difference to the 2300AD route distribution.

Some of the Brown Dwarfs in this list are members of multiple systems that are listed in other datasets presented on this site. These are listed as complete multiple star systems on this list (the other components are duplicated here using the original data) – the datasets should merge seamlessly when combined (the ID numbers are preserved in both lists) but some components may be duplicated – this should not create problems since they will have the same name and position.

Other Updates

I’ve also made several other updates to the datasets, so you’ll need to download them again to get the latest versions!

  • The Pleiades Corridor has been updated to use Extended Hipparcos data.
  • The Yale and Gliese 3 Historical Datasets have been moved into a blog article to separate them from the more accurate datasets on the Stellar Mapping page.
  • The Extended Hipparcos and CTIOPI datasets have been updated to include Multiple Systems. A and B components of some of the multiple stars in the original data were separated by several lightyears due to parallax inconsistencies – these were listed separately, but now they have been combined nto Multiple star systems that are located at the XYZ co-ordinates of the original A component.
  • The Further Stars list is still using New Reduction Hipparcos (and other) data. I will be updating it to HIPX at a later date, but it does contain duplicate stars in different positions and should be considered to be less accurate than the other datasets!
  • [Stellar Mapping] Historical Datasets (Yale & Gliese3)

    As part of this weekend’s update to my Stellar Mapping page (more details about that will be in the next post), I’ve decided to move the Historical datasets (Yale and Gliese3) onto a blog post since they’re no longer accurate and probably aren’t being used much anyway (there’s a link from the Stellar Mapping page to this blog post). So, here they are!

    Historical Datasets

    Historical databases should not be considered “accurate” by modern standards, and have been largely superseded by the ones listed in the “Accurate Datasets” section. The full Yale and Gliese catalogues have been clipped at 300 ly from Sol.

    Yale Trigonometric Parallaxes, Fourth Edition: The Yale catalogue (a.k.a the General Catalogue of Trigonometric Parallaxes, or GCTP) is a historical dataset that was one of the most accurate near star catalogues before Hipparcos, with parallax measurements taken from the ground-based observations. It includes many fainter stars that are not in the Hipparcos catalogue, but the distance accuracy is much lower. It also include many stars that are in the Hipparcos catalogue, but because of the lower accuracy they are somewhat shifted from their Hipparcos-derived positions – the difference increases with distance from Sol. However, the Yale catalogue does include Spectral data for most stars. As such, the Yale and Hipparcos catalogues should NOT be combined.

    Source: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=I/238A/picat.
    Number of star systems: 6,051
    Distance range: 22.8 – 300 lightyears from Sol.
    Accuracy: Positional data are less accurate than Hipparcos, but spectral data is included. Physical data are not accurate. All stars are listed as single stars.

     

    Gliese Nearby Stars, Preliminary 3rd Version: The Gliese catalogue is one of the “classic” historical star catalogues – it was updated in 1991, and includes all stars known at the time within 25 pc of Sol, and a few that are further out. It has low accuracy, but again includes some of the dimmer stars that Hipparcos does not include. The 2300AD star map is apparently based on the 2nd version of this catalogue.

    Source: http://vizier.u-strasbg.fr/viz-bin/VizieR?-source=V/70A.
    Number of star systems: 3,667
    Distance range: 22.8 – 300 lightyears from Sol.
    Accuracy: Positional data are less accurate than Hipparcos, but spectral data is included. Physical data are not accurate. All stars are listed as single stars.

    [Stellar Mapping] Extended Hipparcos dataset added!

    I’ve now replaced the New Reduction Hipparcos data with the new Extended Hipparcos (HIPX) dataset published in 2012 by Anderson & Francis (see this paper for all the details). The HIPX dataset expands the original dataset to include luminosities, spectral types and much more useful astronomical data from a variety of sources, making this the definitive source of information about these stars! The searchable online HIPX catalogue is located at http://vizier.u-strasbg.fr/viz-bin/VizieR-3?-source=+V/137A/XHIP.

    The HIPX data replaces the New Reduction Hipparcos data on this website – Astrosynthesis and Galactic XYZ data have both been updated! In most cases the HIPX XYZ data is identical to the New Reduction Hipparcos XYZs, but issues with the parallaxes for some of the multiple systems in the New Reduction data led to significant inaccuracies there – in those cases, the parallaxes were reverted back to the original Hipparcos parallax data (again, refer to the XHIP paper for further explanation).

    The XHIP data includes more star names (including common/arabic names), which are also presented here. However, note that Gliese numbers higher than 3000 have been removed for ease of reference. Technically these numbers aren’t “Gliese numbers”, they’re “NN” or “Wo(oley)” numbers. Because this could cause confusion, I decided to remove them instead of editing them all, but this isn’t a huge loss since the stars can still be tracked using their HIP numbers or other names.

    If you’ve been using the New Reduction data, then be sure to head over to my Stellar Mapping page to download the new Extended Hipparcos dataset!

    ———————————-

    In other news, my Stellar Mapping page now has the Atomic Rockets Seal of Approval! This is Winchell Chung’s way of saying that he likes my work, and I’m very happy about that because I’ve been a fan of his Atomic Rockets website pretty much since it first appeared online (it’s a great resource for any SF fan)! His 3D Starmaps site is also one of the main inspirations for my own stellar mapping efforts! Thanks, Winchell! :)

    [Stellar Mapping] CTIOPI dataset added, Stellar Mapping page reorganised!

    I have now added the CTIOPI (Cerro Tololo Interamerican Observatory Parallax Investigation) dataset to my Stellar Mapping page! CTIOPI is another dataset from the RECONS group, aimed at locating red, white, and brown dwarfs that are within 25pc of Sol – it adds 164 stars that are mostly contained within 300 ly of Sol. However, it only covers (roughly) the southern sky as viewed from Earth, so only about half of the volume around Sol contains stars from this dataset – that said, the distribution of CTIOPI stars could be used as a guideline for adding fictional stars in the rest of the volume.

    CTIOPI dataset, looking corewards.

    I have also edited the DENSE dataset to remove all the stars that were duplicated in CTIOPI and HIPPARCOS datasets – the most accurate data has been retained (the original DENSE dataset is no longer available here, though I may make it available again in a later blog update). The CTIOPI dataset has also been edited somewhat to remove duplicates (none of the CTIOPI stars have HIP numbers though, though it does include one star – HIP 3856 – that is missing from the Hipparcos dataset). All CTIOPI entries within 22.7 lightyears have also been removed to avoid overlap with RECONS.

    This means that there should now be no duplicated stars at all if the RECONS, DENSE, CTIOPI and HIPPARCOS datasets are used together, so the combined dataset is now about as accurate as it can be. Full details of these edits can be found in the “CTIOPI-DENSE merging details” section in the Astrosynthesis.txt and Galactic.txt files contained in the new RECONS-DENSE-CTIOPI.zip file available from Section 2 of the Stellar Mapping page.

    I’ve also updated and reorganised the Stellar Mapping page to (hopefully) make it easier to decide which datasets to use. If you have already downloaded the DENSE dataset then you should download it again to make sure you have the latest version!

    [Stellar Mapping] The 2300AD Near Star Map

    The 2300AD Near Star Map

    The 2300AD RPG – originally published by Game Designer’s Workshop in 1988 – presented an excellent gritty, realistic near-future hard sci-fi setting with lots of exploration, mystery, and interesting aliens. It’s also about to be republished by Mongoose Publishing as a setting for their version of the Traveller RPG!

    One of 2300AD’s most interesting features is that the setting is built around a realistic (for the 1980s) Near Star List based on the Gliese Catalogue (2nd Version). FTL travel in 2300AD has a maximum range of 7.7 lightyears, resulting in the creation of “Arms” that extend from Sol to connect only the stars that are within this range of eachother (this limit can potentially be extended to 11.55 ly using Stutterwarp tugs, but this is expensive and uncommon).

    There are three of these Arms, each colonised by a different political power in the setting – the French Arm, the Chinese Arm, and the American Arm. The French Arm stretches “upwards” from Sol towards Galactic North, ending at the orange giant star Arcturus. The American and Chinese Arms share the same beginning, but split off so that the American Arm heads Coreward/Spinward while the Chinese Arm sprawls around the (galactic) southern part of the solar neighbourhood.

    Unfortunately the Near Star List (NSL) has not been updated for the new version of 2300AD. A lot of stars have been discovered in the solar neighbourhood since the late 1980s (as shown on my Stellar Mapping page), and the locations and distances of existing stars have been greatly refined since then too – so how does the updated stellar data affect the Arms?
    Continue reading ‘[Stellar Mapping] The 2300AD Near Star Map’

    [Stellar Mapping] How to make your own stellar database!

    Looks like my new Stellar Mapping page has been well received so far – thanks to everyone who has shown an interest in it, I hope you’re finding it useful!

    In this article I’m going to show you how to make your own stellar database, with the same tools I used to construct the ones I presented on my mapping page. For this exercise we’ll be relying on something called VizieR, which is a huge online database of thousands of star catalogues. You’ll need to have a basic understanding astronomy to make the most out of this, but it’s not that tricky.

    Let’s say you want to make a database of stars in a corridor between Sol and the famous Pleiades star cluster (if you’re familiar with the 2300AD RPG, this is essentially the path the Bayern took to the Pleiades). We’ll be using the Hipparcos star catalogue, since it has the most accurate parallax measurements (from which we can derive distances).

    Continue reading ‘[Stellar Mapping] How to make your own stellar database!’

    Website Update: Stellar Mapping page updated!

    My new Stellar Mapping page is finally online! This is a complete rewrite of my previous “Realistic Astrography” page, and now includes Equatorial to Galactic co-ordinate conversion files, the complete RECONS (2012) and DENSE star lists, as well as all the data from the Hipparcos, Gliese 3, and Yale catalogues for stars out to 300ly from Sol! And the Further Stars list is also in there too :)

    RECONS-coreward

    RECONS dataset, looking towards the galactic core.

    The focus has moved away from Traveller and its hex map format (I realised that I was taking accurate data and then making it inaccurate by forcing it into hex map format, so I’ve dropped that completely) and moved towards raw data and Astrosynthesis, but this will still be very useful for anyone interested in using realistic data for the stars near Sol.

    You can check it out at http://evildrganymede.net/rpgs/stellar-mapping/

    I’ll be writing some articles in the coming weeks to expand this – this will include how to use the Vizier stellar databases, and what this means for the 2300AD RPG!

    Website update: Further Stars List uploaded!

    EDIT: This has been superseded by my new Stellar Mapping page!

    I’ve finally added the “Further Star List” to my Realistic Near-Sol Astrography webpage – it’s an excel file containing accurate locations of a selection of major stars (including Vega, Deneb, 51 Pegasi, Spica, Bellatrix and Algol) that are more than 10pc from Sol.

    The format is a bit raw (and I’m not entirely sure why I selected those specific stars to list!). The dark red X/Y/Z columns show the distances in each direction (Sol is the origin, +X is Coreward, +Y is Spinward, +Z is “above” Sol). If you have trouble interpreting it, let me know!

    You can doublecheck the stars too – you can use the Convert spreadsheet in Section 1 of the mapping page to convert the RA/Dec of any stars into X/Y/Z coordinates. If you have astronomy software like Celestia, open it up and activate the Galactic Grid and rotate it so that you’re facing 0° latitude and 0° longitude – you’re now looking directly along the +X axis. Turn to look at 0° Lat, 90° Lon and you’re looking directly along the +Y axis. Look at the Galactic north pole, and you’re looking directly along the +Z axis. You should be able to find your stars using this (e.g. Aldebaran is pretty much directly along the -X direction, and down a bit on the Z axis. Look towards 180° Lon direction and -20° Lat, and there it is!).

    I’ve been sitting on this for six and a half years (!!) and finally decided that I’m never going to draw hexmaps showing these stars, so I may as well just release the data and let other people figure it out! Enjoy! :)

    The link is at http://evildrganymede.net/rpgs/stellar-mapping/.