WEBVTT FILE 1 00:00:00.060 --> 00:00:08.429 Hi my name is Eleanor Lutz and I like to use art and data visualization ah to try 2 00:00:08.429 --> 00:00:13.740 and take scientific topics and share them with the general public, so my most 3 00:00:13.740 --> 00:00:21.539 recent project was a series of about ten different maps of astronomy data taken 4 00:00:21.539 --> 00:00:27.900 from open sources like NASA and the USGS so I'd like to talk a little about some 5 00:00:27.900 --> 00:00:31.380 of the things I learned from making these maps and then some of the design 6 00:00:31.380 --> 00:00:37.110 decisions behind each one, so to give you a bit of background when I share these 7 00:00:37.110 --> 00:00:40.770 maps all of the code is open sourced on github 8 00:00:40.770 --> 00:00:46.410 with tutorials so that anybody who wants can make the maps themselves. I also have 9 00:00:46.410 --> 00:00:51.059 the maps available as posters and the people who tend to generally use them 10 00:00:51.059 --> 00:00:55.410 are people who have young kids or our teachers and classrooms so that's really 11 00:00:55.410 --> 00:01:02.160 the kind of audience that I'm designing for, this first map shows the orbit paths 12 00:01:02.160 --> 00:01:09.540 of about 18,000 asteroids in the solar system, so this map was probably the 13 00:01:09.540 --> 00:01:13.590 most difficult one for me because I needed to pull together data from about 14 00:01:13.590 --> 00:01:20.340 five different open data sources and put them together and the the question I 15 00:01:20.340 --> 00:01:25.380 really tried to answer while making this map was what was the the general message 16 00:01:25.380 --> 00:01:32.340 I wanted to get across to these children or the general public and for me what 17 00:01:32.340 --> 00:01:36.259 was the most awesome thing about this data was just that there are so many 18 00:01:36.259 --> 00:01:41.640 asteroids all over the solar system and I'm not actually a space scientist so 19 00:01:41.640 --> 00:01:46.110 this is something that was really surprising to me so I decided to use 20 00:01:46.110 --> 00:01:51.840 design decisions that would really emphasize that point so for example I'm 21 00:01:51.840 --> 00:01:57.180 showing you all of the orbits here on a logarithmic scale with most of the map 22 00:01:57.180 --> 00:02:02.490 focus on the first billion kilometers from the Sun and this was a design 23 00:02:02.490 --> 00:02:07.200 choice that let me include everything to the boundaries of the solar system but 24 00:02:07.200 --> 00:02:12.510 still leave enough space to see just how many asteroids are in the inner 25 00:02:12.510 --> 00:02:14.930 areas 26 00:02:19.319 --> 00:02:26.489 okay so for other projects I had to do much less data wrangling so this is a 27 00:02:26.489 --> 00:02:33.500 geologic map of Mars some of you might recognize the data from the USGS map 28 00:02:33.500 --> 00:02:39.780 which basically had all the data I'm showing here already laid out and 29 00:02:39.780 --> 00:02:46.019 organized the main design choices I did here was really to work with the 30 00:02:46.019 --> 00:02:51.239 language in the map the original map was I think intended for scientific 31 00:02:51.239 --> 00:02:56.989 audiences so the labeling and the colors were very difficult to understand 32 00:02:56.989 --> 00:03:02.549 especially for young audiences so in the bottom here I've really shortened all 33 00:03:02.549 --> 00:03:07.109 the descriptions and tried to use vocabulary that everybody could 34 00:03:07.109 --> 00:03:18.030 understand. I also changed the colors of the map, so here's a zoomed in version 35 00:03:18.030 --> 00:03:22.560 I've decided to really emphasize the volcanic geologic region so I'm making 36 00:03:22.560 --> 00:03:28.019 them a really bright red and then also to emphasize the difference between the 37 00:03:28.019 --> 00:03:32.180 northern and southern hemispheres by putting slightly different color schemes 38 00:03:32.180 --> 00:03:38.010 so I want to point out that sometimes these design decisions don't necessarily 39 00:03:38.010 --> 00:03:43.199 make the map more legible I think some of the volcanic regions in particular 40 00:03:43.199 --> 00:03:49.229 can be a little hard to read but because these maps weren't for a scientific 41 00:03:49.229 --> 00:03:55.409 purpose I could make design decisions that were a little more creative and 42 00:03:55.409 --> 00:04:01.400 that emphasized the volcanoes or these other features the planet 43 00:04:05.380 --> 00:04:13.260 sometimes I needed to do a little more simplification of the data to have the 44 00:04:13.260 --> 00:04:18.900 data fit and look well at the size that I was going for so this is a geologic 45 00:04:18.900 --> 00:04:25.020 map of the moon the difficulty here was that because the data for the moon was 46 00:04:25.020 --> 00:04:30.930 much more detailed the geologic features were a lot finer and many of them 47 00:04:30.930 --> 00:04:35.160 couldn't actually be seen at the scale that I was showing at these posters 48 00:04:35.160 --> 00:04:41.880 these clusters size, so when I went through the data I that many of the 49 00:04:41.880 --> 00:04:49.410 smaller geologic features were actually different ages of the same material and 50 00:04:49.410 --> 00:04:57.090 this was causing a lot of noise in areas that had been sampled many times, so what 51 00:04:57.090 --> 00:05:01.680 I decided to do for this map was to simplify it to a level where you could 52 00:05:01.680 --> 00:05:07.140 see individual geologic features, so this map doesn't actually include the 53 00:05:07.140 --> 00:05:12.450 different ages of the materia,l it's combined the material the same type of 54 00:05:12.450 --> 00:05:17.420 geologic material for many different ages 55 00:05:26.060 --> 00:05:31.730 okay, I also had to combine I think six different data sets for this moon 56 00:05:31.730 --> 00:05:35.840 geology map, you can actually see the boundaries here where some of the data 57 00:05:35.840 --> 00:05:41.120 sources don't agree with each other, so that was a part where in the previous 58 00:05:41.120 --> 00:05:47.240 map I also decided to include the different data sources as a reference 59 00:05:47.240 --> 00:05:50.160 for why those differences existed 60 00:05:56.120 --> 00:06:01.490 okay I also designed a series of topographic maps of the rocky planets 61 00:06:01.490 --> 00:06:04.729 and the moon so for these maps I use the digital 62 00:06:04.729 --> 00:06:10.639 elevation model from the USGS as well as a database of names that I could 63 00:06:10.639 --> 00:06:16.370 download and plot onto each of these maps in Python, so one of the challenges 64 00:06:16.370 --> 00:06:21.650 of making topographic maps for space was that I found it was very difficult to 65 00:06:21.650 --> 00:06:25.760 kind of understand the scale of the planet because there are no oceans or 66 00:06:25.760 --> 00:06:32.540 other large differences in the in the surface, so what I try to do with these 67 00:06:32.540 --> 00:06:39.470 maps is use a color scale that was very variable from the the lowest parts here 68 00:06:39.470 --> 00:06:42.050 in Navy to the highest parts of the planet and 69 00:06:42.050 --> 00:06:51.500 orange and yellow and making these double color decisions for each of the 70 00:06:51.500 --> 00:06:56.180 planets I think really helped emphasize the scale of the planet by adding a 71 00:06:56.180 --> 00:06:59.840 little more interest in by helping differentiate between the different 72 00:06:59.840 --> 00:07:02.050 elevations 73 00:07:05.670 --> 00:07:10.620 I also made a map of the earth so if you look at this online it's actually 74 00:07:10.620 --> 00:07:14.880 animated so that each of the frames shows the Arctic ice for that particular 75 00:07:14.880 --> 00:07:19.580 month of the year and this is using blue marble data from NASA 76 00:07:23.040 --> 00:07:25.280 okay and this 77 00:07:25.290 --> 00:07:30.180 final set of maps I want to talk about is a map of the constellations as seen 78 00:07:30.180 --> 00:07:36.330 from Earth, so this was one of my favorite maps to work on because there's 79 00:07:36.330 --> 00:07:41.160 just a huge amount of data available, here I've already limited the data I'm 80 00:07:41.160 --> 00:07:47.550 showing to the 8,000 or so stars you can actually see from Earth but there's 81 00:07:47.550 --> 00:07:53.760 still a lot of data a lot of information about the size of the stars and as well 82 00:07:53.760 --> 00:08:00.210 as the constellations and the names of each star this map is actually part of a 83 00:08:00.210 --> 00:08:07.350 series, so here is just the you know the scientific data without the labels and 84 00:08:07.350 --> 00:08:14.190 the lines that people have added and what I realized here was that these 85 00:08:14.190 --> 00:08:20.700 constellations, come from many different cultures so here I'm showing you the 86 00:08:20.700 --> 00:08:26.400 same stars but in this map I'm showing also the constellations from about 30 87 00:08:26.400 --> 00:08:33.599 different cultures or civilizations from around the world each color here is data 88 00:08:33.599 --> 00:08:39.960 from a different culture this is from an open database called Stellarium and what 89 00:08:39.960 --> 00:08:45.240 I really like about this map is that even though it's kind of a tangled mess 90 00:08:45.240 --> 00:08:50.850 of lines you can see that some stars are really popular the ones the large ones 91 00:08:50.850 --> 00:08:57.420 circled with large outlines with a most popular but some constellations are also 92 00:08:57.420 --> 00:09:04.560 very unique so the stars outlined in an outline with just one cultures color is 93 00:09:04.560 --> 00:09:11.220 not used by any other culture in this database so I really enjoyed this 94 00:09:11.220 --> 00:09:16.860 project in particular because I was able to combine scientific data from this 95 00:09:16.860 --> 00:09:21.280 large database with cultural data and kind of 96 00:09:21.280 --> 00:09:25.960 the human history of how we've been looking at stars and working with 97 00:09:25.960 --> 00:09:33.430 astronomy for many hundreds and thousands of years so as I said again 98 00:09:33.430 --> 00:09:37.990 all of this code is available open source please feel free to find me 99 00:09:37.990 --> 00:09:42.430 afterwards if you're interested in learning more about the project and 100 00:09:42.430 --> 00:09:46.480 thank you so much for everyone for listening and for NASA and AGU for 101 00:09:46.480 --> 00:09:49.200 letting me come here