@ToOpenScience

@theAGU TOPS🚀 Part of #NASATOPS mission to unlock the full potential of a more equitable, impactful, efficient, scientific future. Not an official NASA account

 Everywhere
github.com/nasa/Transform-to-Open-Science
Joined May 2022
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  • Followers594
.@theAGU, #NASATOPS team, and the wonderful TOPS Community Panelists met last week for two days of open science planning and dreaming... plus an awesome tour of @NASAJPL's museum! #IHeartOpenScience
Various TOPS team members and panelists posing for a photo with the Mars Rover in the JPL Visitor Center.

ALT Various TOPS team members and panelists posing for a photo with the Mars Rover in the JPL Visitor Center.

TOPS team members and panelists posing for a photo with another Mars Rover at JPL.

ALT TOPS team members and panelists posing for a photo with another Mars Rover at JPL.

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Day 3 at #NASAScience #OSSDR: At its core, #OpenScience principles embrace transparency, collaboration, and participation. #DEIA is fundamental to Open Science. How can we make #DataScience more #equitable, #accessible and #inclusive for all? RT with your ideas!
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Today at the #NASA Open Source Science Data Repositories Workshop 2022: peer-to-peer learning about #OpenScience and #OpenSource, collaboration and building community, and creativity and innovation during the various unconference sessions. #IHeartOpenScience
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4 days of #OpenData talk with scientists about upcoming #OpenScience data, tools, and software. Let’s talk about #Science and #DataScience! Changing the landscape for science together at the @NASA Open Source Science Data Repositories Workshop 2022!
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👀📢🚀Want some NASA funding??👀📢🚀 @NASA #openscience wants a proposal from YOU! 🎉 ~ $3 Million / year !! 🎉 We are looking for 3 different types of proposals. More info in this 🧵(1/5)
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Get ALL the info here: F.14 Transform to Open Science Training (TOPST). go.nasa.gov/3xgUorP But wait, there is MORE! Ask questions & get answers at our next community forum -- register here: go.nasa.gov/3RAD9cU 🧵(5/5)
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Interested in getting involved in #OpenScience? Join TOPS for a monthly community forum to hear how NASA Biological & Physical Sciences and Heliophysics are using open science practices. @NASASpaceSci @NASASun @SamGebre1 @AeroSciengineer. Register at go.nasa.gov/3crKGeY
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#NASATOPS Subject Matter Expert Dr. Natasha Batalha (@NASAWebb) co-authored a paper on discovering Carbon Dioxide in the atmosphere of exoplanet WASP-39b. This is #OpenScience in action, as the #JWST data became available one month ago! xitter.cf/NASAWebb/status/156280…
NASA Webb Telescope
@NASAWebb25 Aug 2022
Catch your breath — Webb has captured the first clear evidence of carbon dioxide (CO2) in the atmosphere of a planet outside of our solar system! WASP-39 B is a gas giant closely orbiting a Sun-like star 700 light years away: go.nasa.gov/3PIRGSc
The graphic shows the transmission spectrum of the hot gas giant exoplanet WASP-39 b, captured using Webb's NIRSpec Bright Object Time-Series Spectroscopy mode, and is titled accordingly. An illustration of the planet and its star is in the background. The vertical y axis is labeled “amount of light blocked” and runs from 2.00 percent (less light blocked) to 2.35 percent (more light blocked). The x axis is labeled “wavelength of light” and ranges from 3.00 microns to 5.6 microns. The data points are plotted as white circles with gray error margin bars running through the circles. A curvy blue line represents a best-fit model. A prominent peak in the blue line is labeled “Carbon Dioxide, CO2,” indicating the presence of carbon dioxide in the exoplanet. This peak is centered around 4.3 microns and has a y value of between 2.25 and 2.30 percent of light blocked. The baseline is between 2.10 and 2.17 percent.

ALT The graphic shows the transmission spectrum of the hot gas giant exoplanet WASP-39 b, captured using Webb's NIRSpec Bright Object Time-Series Spectroscopy mode, and is titled accordingly. An illustration of the planet and its star is in the background. The vertical y axis is labeled “amount of light blocked” and runs from 2.00 percent (less light blocked) to 2.35 percent (more light blocked). The x axis is labeled “wavelength of light” and ranges from 3.00 microns to 5.6 microns. The data points are plotted as white circles with gray error margin bars running through the circles. A curvy blue line represents a best-fit model. A prominent peak in the blue line is labeled “Carbon Dioxide, CO2,” indicating the presence of carbon dioxide in the exoplanet. This peak is centered around 4.3 microns and has a y value of between 2.25 and 2.30 percent of light blocked. The baseline is between 2.10 and 2.17 percent.

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To build an equitable and diverse #OpenScience community, everyone is part of the puzzle! TOPS at #SNC22 #justiceingeoscience
A completed TOPS puzzle

ALT A completed TOPS puzzle

Conference participants working on a giant TOPS puzzle

ALT Conference participants working on a giant TOPS puzzle

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Learn about where we are at with the TOPS OpenCore curriculum and how to get involved on July 14. Register at github.com/nasa/Transform-to… Hear from the Team/Leads @cyndibughall @libcce @yoyehudi @yalahowy @NatashaBatalha @shilaan01 @dontusethiscode @RiddleMeCam #NASATOPS #OpenScience
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