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Investigations with Doppler spectroscopy </div> </a></li> <li> <a href="/dois" alt="Digitial Object Indentifiers" class="nav_header" title="Digitial Object Indentifiers">DOIs</a> </li> </ul> </div> <div class='col-md-3'> <ul> <li> <a href="/projects/category/missions-and-centers" class="nav_header">Missions & Centers</a> </li> <li> <a href="/project/euclid">Euclid <div class='small'> Euclid NASA Science Center at IPAC </div> </a></li> <li> <a href="/project/nexsci">NExScI <div class='small'> NASA Exoplanet Science Institute </div> </a></li> <li> <a href="/project/ztf">ZTF <div class='small'> Zwicky Transient Facility </div> </a></li> </ul> </div> <div class='col-md-3'> <ul> <li> <a href="/projects/status/in-development" class="nav_header">In Development</a> </li> <li> <a href="/project/ariel-case">ARIEL/CASE <div class='small'> Atmospheric Remote-sensing Infrared Exoplanet Large-survey </div> </a></li> <li> <a href="/project/dsa-2000">DSA-2000 <div class='small'> Deep Synoptic Array 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Rubin Observatory </div> </a></li> <li> <a href="/project/spherex">SPHEREx <div class='small'> Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer </div> </a></li> <li> <a href="/project/uvex">UVEX <div class='small'> Ultraviolet Explorer </div> </a></li> </ul> </div> <div class='col-md-3'> <ul> <li> <a href="/future/projects/mission-studies-and-proposals" class="nav_header">Mission Studies & Proposals</a> </li> <li> <a href="/project/iscea">ISCEA <div class='small'> Infrared SmallSat for Cluster Evolution Astrophysics </div> </a></li> <li> <a href="/project/joint-survey-processing">JSP <div class='small'> Joint Survey Processing </div> </a></li> <li> <a href="/project/prima">PRIMA <div class='small'> Probe Far-Infrared Mission for Astrophysics </div> </a></li> </ul> </div> </div> </div> <div class='sub_nav_pane' id='education_subnav'> <div class='row'> <div class='col-md-3 right'> <ul> <li> <a href="/outreach#more-epo-projects" class="nav_header">More EPO Projects</a> </li> <li> <a href="/project/cool-cosmos">Cool Cosmos </a></li> <li> <a href="/project/explore-exoplanets">Explore Exoplanets: The Discoverers </a></li> <li> <a href="/project/nitarp">NITARP <div class='small'> NASA/IPAC Teacher Archive Research Program </div> </a></li> </ul> </div> <div class='col-md-3 right'> <ul> <li> <a href="/outreach#universe-of-learning" class="nav_header">NASA Universe of Learning</a> </li> <li> <a href="/project/astropix">AstroPix </a></li> <li> <a href="/project/uol-astrovisualization">Astrovisualization Community of Practice </a></li> <li> <a href="/project/universe-unplugged">Universe Unplugged </a></li> </ul> </div> <div class='col-md-3 right'> <ul> <li> <a href="/outreach" class="nav_header">Overview</a> </li> </ul> <ul> <li> <a href="/outreach#key_expertise" class="nav_header">Key Expertise</a> </li> <li> <a href="/page/education">Education</a> </li> <li> <a href="/page/visualization">Science Visualization & 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class='container'> <div class='row'> <div class='col-md-12'> <h1 class='page_title'> In Development </h1> </div> </div> </div> </div> <div class='container offset_container'> <div class='row'> <div class='col-md-12'> <div class='content_box leading_box'> <p> IPAC is involved in the development of a range of future observational facilities both in space and on the ground. IPAC contributes expertise in science formulation, data science, mission management, technology development, public outreach and communications. In particular, projects currently in development leverage IPAC's experience in maximizing the scientific return from targeted exploration of the infrared-submillimeter universe, all-sky surveys, and time series observations. IPAC science staff participate in setting the science requirements for these facilities. </p> </div> </div> </div> </div> <div class='container pb-30'> <div class='row'> <div class='col-md-12'> <a class='offset_anchor' name='ariel-case'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Ariel_space_high_res1" src="/system/activities/images/88/small/ariel_space_high_res1.jpg?1638217728" /> </div> <div class='col-md-8'> <h3> ARIEL/CASE <div class='small'> Atmospheric Remote-sensing Infrared Exoplanet Large-survey </div> </h3> <p> ARIEL, the Atmospheric Remote-sensing Infrared Exoplanet Large-survey, is a European Space Agency (ESA) M-class mission, with participation from NASA, to survey and characterize the atmospheres of 1000 exoplanets. ARIEL is a 1 m class telescope with 3 photometric channels and 3 spectroscopic channels covering continuously 0.5 to 8 microns in wavelengths. The goal of ARIEL is to survey ~1000 transiting exoplanets from gas giants to rocky planets in the hot to temperate zones of their host stars. ARIEL is expected to launch in 2029. </p> <a href="/project/ariel-case" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='col-md-4 hidden-xs hidden-sm'> <img alt="Ariel_space_high_res1" src="/system/activities/images/88/small/ariel_space_high_res1.jpg?1638217728" /> </div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='dsa-2000'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Dsa-2000" src="/system/activities/logos/110/small/DSA-2000.png?1738111592" /> </div> <div class='col-md-8'> <h3> DSA-2000 <div class='small'> Deep Synoptic Array </div> </h3> <p> The DSA-2000 is proposed to be a world-leading radio survey telescope and multi-messenger discovery engine. The array will consist of 2000 × 5m dishes instantaneously covering the 0.7 – 2 GHz frequency range, spanning an area of 19 km × 15 km in a radio-quiet valley in Nevada. It will have near complete sampling of the uv-plane allowing us to replace a traditional correlator digital backend with a “radio camera” that produces images in real-time. In a five-year initial survey, the DSA-2000 will image the entire viewable sky (~31,000 deg²) repeatedly over sixteen epochs, detecting >1 billion radio sources in a combined full-Stokes sky map with 500 nJy/beam rms noise. As a radio survey instrument it will be unprecedented relative to any instrument existing or planned. </p> <a href="/project/dsa-2000" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='lunar-trailblazer'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Logo" src="/system/activities/logos/86/small/logo.png?1607650634" /> </div> <div class='col-md-8'> <h3> LTB <div class='small'> Lunar Trailblazer </div> </h3> <p> NASA's Lunar Trailblazer targets one of the most surprising discoveries of the decade: water on the Moon. As a NASA SIMPLEx (Small Innovative Missions for Planetary Exploration) program mission selection, Lunar Trailblazer achieves critical advancements for science as a lower-budget, ride-along mission. Science objectives include studying the form, abundance, and distribution of water on the Moon, as well as the lunar water cycle. Lunar Trailblazer is scheduled to launch in towards the end of February 2025. The mission PI is Bethany Ehlmann (Caltech). </p> <a href="/project/lunar-trailblazer" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='col-md-4 hidden-xs hidden-sm'> <img alt="Logo" src="/system/activities/logos/86/small/logo.png?1607650634" /> </div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='roman'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Stsci-h-p1939a-f-3840x2560" src="/system/activities/images/10/small/STScI-H-p1939a-f-3840x2560.jpg?1568657563" /> </div> <div class='col-md-8'> <h3> Roman <div class='small'> Nancy Grace Roman Space Telescope </div> </h3> <p> The Nancy Grace Roman Space Telescope is a NASA observatory designed to explore the Universe in search of answers to fundamental questions about dark energy, exoplanets, and infrared astrophysics. The telescope has a 2.4 m primary mirror (the same size as the Hubble Space Telescope), but will have a field of view that is more than 200 times greater than that of the Hubble Space Telescope's WFC3 IR Channel, capturing much more of the sky in one pointing. The primary instrument, the Wide Field Instrument (WFI), will measure light from hundreds of millions of galaxies over the course of the prime mission lifetime and will perform a microlensing survey of the inner Milky Way to find exoplanets down to a tenth of Earth's mass. The Coronagraph Instrument will directly detect Jupiter analog exoplanets and dust and debris disks around nearby stars. The Nancy Grace Roman Space Telescope is designed for a five year prime mission and has been committed to be launched no later than May 2027. </p> <a href="/project/roman" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='neo-surveyor'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Neocam_wide" src="/system/activities/images/18/small/neocam_wide.jpg?1565396277" /> </div> <div class='col-md-8'> <h3> NEO Surveyor <div class='small'> Near-Earth Object Surveyor </div> </h3> <p> NEO Surveyor is a new mission that is designed to discover and characterize most of the potentially hazardous asteroids that are near the Earth. NEO Surveyor consists of an infrared telescope and wide-field camera operating at thermal infrared wavelengths. NEO Surveyor's primary science objectives are to assess the present-day risk of near-Earth object (NEO) impact, study the origin and ultimate fate of our solar system's asteroids, and find the most suitable NEO targets for future exploration by robots and humans. The NEO Surveyor mission has been funded for development by NASA, with a launch date of no later than June 2028. </p> <a href="/project/neo-surveyor" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='col-md-4 hidden-xs hidden-sm'> <img alt="Neocam_wide" src="/system/activities/images/18/small/neocam_wide.jpg?1565396277" /> </div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='spherex'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Spherex-2020logo_color_white_bg" src="/system/activities/logos/80/small/spherex-2020logo_color_white_bg.png?1676315075" /> </div> <div class='col-md-8'> <h3> SPHEREx <div class='small'> Spectro-Photometer for the History of the Universe, Epoch of Reionization and Ices Explorer </div> </h3> <p> SPHEREx is a NASA Medium Explorer mission designed to 1) constrain the physics of inflation by measuring its imprints on the three-dimensional large-scale distribution of matter, 2) trace the history of galactic light production through a deep multi-band measurement of large-scale clustering, and 3) investigate the abundance and composition of water and biogenic ices in the early phases of star and planetary disk formation. SPHEREx will obtain near-infrared 0.75-5.0 um spectra every 6" over the entire sky. It implements a simple instrument design with a single observing mode to map the entire sky four times during its nominal 25-month mission. SPHEREx will also have strong scientific synergies with other missions and observatories, resulting in a rich legacy archive of spectra that will bear on numerous scientific investigations. The mission PI is Jamie Bock (Caltech). SPHEREx is scheduled to launch towards the end of February 2025. </p> <a href="/project/spherex" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='uvex'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Uvex_logo_light-c2b2b2bdfb840522ad1a98ebf46e6a63fc7ad7ba70020d520e741a924a0f675f" src="/system/activities/logos/89/small/uvex_logo_light-c2b2b2bdfb840522ad1a98ebf46e6a63fc7ad7ba70020d520e741a924a0f675f.png?1665696874" /> </div> <div class='col-md-8'> <h3> UVEX <div class='small'> Ultraviolet Explorer </div> </h3> <p> The Ultraviolet Explorer (UVEX) is targeted to launch in 2030 as NASA’s next Astrophysics Medium-Class Explorer mission. UVEX will undertake a synoptic survey of the entire sky in the near-UV and far-UV, probing the dynamic universe with a sensitivity more than 50 times better than GALEX. UVEX will also have a powerful broadband spectroscopic capability. UVEX will address fundamental questions from the Astro2020 Decadal Survey, and study the evolution of low-metallicity, low-mass galaxies. UVEX time-domain surveys will probe the aftermaths of gravitational wave-discovered compact object mergers, discover fast UV transients, and diagnose the early stages of explosive phenomena. </p> <a href="/project/uvex" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='col-md-4 hidden-xs hidden-sm'> <img alt="Uvex_logo_light-c2b2b2bdfb840522ad1a98ebf46e6a63fc7ad7ba70020d520e741a924a0f675f" src="/system/activities/logos/89/small/uvex_logo_light-c2b2b2bdfb840522ad1a98ebf46e6a63fc7ad7ba70020d520e741a924a0f675f.png?1665696874" /> </div> <div class='clearfix'></div> </div> </div> </div> <div class='col-md-12'> <a class='offset_anchor' name='rubin'></a> <div class='content_box project_box odd_activity_row'> <div class='row'> <div class='col-md-4 activity_image visible-xs-block visible-sm-block'> <img alt="Rubin_logo063" src="/system/activities/logos/28/small/rubin_logo063.jpg?1675108651" /> </div> <div class='col-md-8'> <h3> Rubin <div class='small'> Vera C. Rubin Observatory </div> </h3> <p> The Vera C. Rubin Observatory (formerly known as the Large Synoptic Survey Telescope) is one of the next generation of great observatories, designed to conduct a ten- year survey of the dynamic Universe. The Rubin Observatory will have an exceptionally wide field of view and the ability to survey the entire visible sky every three nights. The astronomical catalogs produced by the Rubin Observatory will be thousands of times larger than from the largest current surveys. Astronomers will use this wealth of data to better understand dark matter and dark energy, the formation and structure of the Milky Way, the transient optical sky, hazardous asteroids, and the remote solar system. The Rubin Observatory is currently under construction in northwestern Chile and it is expected to begin operations in the 2020s. </p> <a href="/project/rubin" class="quaternary_color more_link">More Information <i class='fa fa-chevron-right'></i> </a></div> <div class='clearfix'></div> </div> </div> </div> </div> </div> </div> <div class='footer_box'> <div class='container'> <div class='row'> <div class='col-md-4'> <div class='footer_group affiliates'> <a href="http://www.ipac.caltech.edu" alt="Infrared Processing and Analysis Center" title="Infrared Processing and Analysis Center"><img alt="Ipac" src="/assets/ipac-4c1a46bd7efc14226bcc882880fc2871.png" /></a> <a href="http://www.caltech.edu" alt="California Institute of Technology" title="California Institute of Technology"><img alt="Caltech" src="/assets/caltech-8ad9780e54d034d665af4a3dbd37d62c.png" /></a> </div> </div> <div class='col-md-8 footer_wrapper'> <div class='row'> <div class='col-xs-6 col-md-3'> <div class='footer_group'> <p class='list_header'> Policies </p> <ul class='page_links'> <li> <i class='fa fa-angle-right'></i> <a href="/page/privacy">Privacy Policy</a> </li> <li> <i class='fa fa-angle-right'></i> <a href="/page/image-use-policy">Image Use Policy</a> </li> </ul> </div> </div> <div class='col-xs-6 col-md-3'> <div class='footer_group'> <p class='list_header'> Get in Touch </p> <ul class='page_links'> <li> <i class='fa fa-angle-right'></i> <a href="/page/contact#visitor-information">Visit IPAC</a> </li> <li> <i class='fa fa-angle-right'></i> <a href="/page/contact">Contact Us</a> </li> <li> <i class='fa fa-angle-right'></i> <a href="/staff">People</a> </li> <li> <i class='fa fa-angle-right'></i> <a href="/page/opportunities">Job Opportunities</a> </li> </ul> </div> </div> <div class='col-xs-6 col-md-3'> <div class='footer_group'> <p class='list_header'> Stay in Touch </p> <ul class='page_links'> <li> <i class='fa fa-angle-right'></i> <a href="https://www.facebook.com/caltechipac/">Facebook</a> </li> <li> <i class='fa fa-angle-right'></i> <a href="https://twitter.com/caltechipac">Twitter</a> </li> </ul> </div> </div> </div> </div> </div> </div> </div> <script> //<![CDATA[ (function(i,s,o,g,r,a,m){i['GoogleAnalyticsObject']=r;i[r]=i[r]||function(){ (i[r].q=i[r].q||[]).push(arguments)},i[r].l=1*new Date();a=s.createElement(o), m=s.getElementsByTagName(o)[0];a.async=1;a.src=g;m.parentNode.insertBefore(a,m) })(window,document,'script','https://www.google-analytics.com/analytics.js','ga'); ga('create', 'UA-35868239-14', 'auto'); ga('send', 'pageview'); //]]> </script> <script src="/assets/application-dd3d068431ffda3da184aa851ca157d3.js" type="text/javascript"></script> </body> </html>