{
    "id": 12410,
    "url": "https://svs.gsfc.nasa.gov/12410/",
    "page_type": "Produced Video",
    "title": "Small Satellites for Earth Science",
    "description": "NASA has embraced the revolution in small spacecraft and satellites, from CubeSats you can hold in your hand to microsatellites the size of a small washing machine. The technology helps advance scientific and human exploration, reduces the cost of new missions, and expands access to space. The briefing will discuss NASA's overall program, technology development initiatives, and new Earth-observing missions that use individual and constellations of small satellites to study climate change, hurricanes and clouds.Briefing PanelistsEllen Stofan, chief scientists at NASA Headquarters in WashingtonThomas Zurbuchen, associate administrator for the Science Mission Directorate at NASA HeadquartersSteve Jurczyk, associate administrator for the Science Mission Directorate at NASA HeadquartersMichael Freilich, director of the Earth Science Division at NASA HeadquartersAaron Ridley, mission constellation scientist for NASA's Cyclone Global Navigation Satellite System (CYGNSS) at the University of Michigan in Ann ArborBill Swartz, CubeSat principal investigator for the Radiometer Assessment using Vertically Aligned Nanotubes (RAVAN) project at Johns Hopkins University Applied Physics Laboratory in Laurel, MarylandWilliam Blackwell, principal investigator for the Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsat (TROPICS) mission at the Massachusetts Institute of Technology Lincoln Laboratory, Lexington, Mass.More information is available. || ",
    "release_date": "2016-11-07T13:45:00-05:00",
    "update_date": "2024-10-10T00:16:50.783742-04:00",
    "main_image": {
        "id": 418497,
        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_4.jpg",
        "filename": "CYGNSS_4.jpg",
        "media_type": "Image",
        "alt_text": "Credit: University of Michigan\r",
        "width": 1920,
        "height": 1080,
        "pixels": 2073600
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    "main_video": null,
    "main_credits": {
        "Produced by": [
            {
                "name": "Kathryn Mersmann",
                "employer": "USRA"
            }
        ],
        "Written by": [
            {
                "name": "Ellen T. Gray",
                "employer": "ADNET Systems, Inc."
            }
        ]
    },
    "progress": "Complete",
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            "id": 332043,
            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332043",
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            "description": "NASA has embraced the revolution in small spacecraft and satellites, from CubeSats you can hold in your hand to microsatellites the size of a small washing machine. The technology helps advance scientific and human exploration, reduces the cost of new missions, and expands access to space. The briefing will discuss NASA's overall program, technology development initiatives, and new Earth-observing missions that use individual and constellations of small satellites to study climate change, hurricanes and clouds.<br><br>Briefing Panelists<br><br>\t<b>Ellen Stofan</b>, chief scientists at NASA Headquarters in Washington<br><br>\t<b>Thomas Zurbuchen</b>, associate administrator for the Science Mission Directorate at NASA Headquarters<br><br>\t<b>Steve Jurczyk</b>, associate administrator for the Science Mission Directorate at NASA Headquarters<br><br>\t<b>Michael Freilich</b>, director of the Earth Science Division at NASA Headquarters<br><br>\t<b>Aaron Ridley</b>, mission constellation scientist for NASA's Cyclone Global Navigation Satellite System (CYGNSS) at the University of Michigan in Ann Arbor<br><br>\t<b>Bill Swartz</b>, CubeSat principal investigator for the Radiometer Assessment using Vertically Aligned Nanotubes (RAVAN) project at Johns Hopkins University Applied Physics Laboratory in Laurel, Maryland<br><br>\t<b>William Blackwel</b>l, principal investigator for the Time-Resolved Observations of Precipitation structure and storm Intensity with a Constellation of Smallsat (TROPICS) mission at the Massachusetts Institute of Technology Lincoln Laboratory, Lexington, Mass.<br><br><a href=\"/12411\">More information</a> is available.",
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            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332044",
            "widget": "Single image",
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            "description": "<b>Figure 1</b> Tropical cyclone track forecasts have improved in accuracy by ~50% since 1990, but there has been essentially no improvement in the accuracy of intensity forecasts. We need wind measurements IN the hurricane.<p><p>Credit: NOAA/NWS",
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                        "alt_text": "Figure 1 Tropical cyclone track forecasts have improved in accuracy by ~50% since 1990, but there has been essentially no improvement in the accuracy of intensity forecasts. We need wind measurements IN the hurricane.Credit: NOAA/NWS",
                        "width": 973,
                        "height": 777,
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                        "alt_text": "Figure 1 Tropical cyclone track forecasts have improved in accuracy by ~50% since 1990, but there has been essentially no improvement in the accuracy of intensity forecasts. We need wind measurements IN the hurricane.Credit: NOAA/NWS",
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            "description": "<b>Figure 2</b> Top panel: Historical storm tracks. Bottom left panel: CYGNSS measurements from one orbit over 1.5 hours. Bottom right panel: CYGNSS measurements from 15 orbits over 24 hours.<p>\rCredit: University of Michigan\r",
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                        "media_type": "Image",
                        "alt_text": "Figure 2 Top panel: Historical storm tracks. Bottom left panel: CYGNSS measurements from one orbit over 1.5 hours. Bottom right panel: CYGNSS measurements from 15 orbits over 24 hours.\rCredit: University of Michigan\r",
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                        "media_type": "Image",
                        "alt_text": "Figure 2 Top panel: Historical storm tracks. Bottom left panel: CYGNSS measurements from one orbit over 1.5 hours. Bottom right panel: CYGNSS measurements from 15 orbits over 24 hours.\rCredit: University of Michigan\r",
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            "description": "<b>Figure 3</b> The CYGNSS mission takes advantage of GPS signals bouncing off the ocean to measure wind speed. Eight identical small satellites, each about the size of a microwave oven, flying in formation carry custom modified GPS receivers pointed at the oceans. When the water is smooth – not windy – the GPS signals reflect back uniformly, like the moon on a pond reflected as if in a mirror. When the water is choppy – windy – the signals reflect back in in the same direction but distorted, like the moon reflection on a choppy pond being distorted by ripples. <p>\rCredit: University of Michigan\r",
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                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_3.jpg",
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                        "media_type": "Image",
                        "alt_text": "Figure 3 The CYGNSS mission takes advantage of GPS signals bouncing off the ocean to measure wind speed. Eight identical small satellites, each about the size of a microwave oven, flying in formation carry custom modified GPS receivers pointed at the oceans. When the water is smooth – not windy – the GPS signals reflect back uniformly, like the moon on a pond reflected as if in a mirror. When the water is choppy – windy – the signals reflect back in in the same direction but distorted, like the moon reflection on a choppy pond being distorted by ripples. \rCredit: University of Michigan\r",
                        "width": 1024,
                        "height": 768,
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            "id": 332047,
            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332047",
            "widget": "Single image",
            "title": "",
            "caption": "",
            "description": "Credit: University of Michigan\r",
            "items": [
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                    "id": 263697,
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                    "instance": {
                        "id": 418497,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_4.jpg",
                        "filename": "CYGNSS_4.jpg",
                        "media_type": "Image",
                        "alt_text": "Credit: University of Michigan\r",
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                        "height": 1080,
                        "pixels": 2073600
                    }
                },
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                    "id": 263698,
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                        "id": 418498,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_4_searchweb.png",
                        "filename": "CYGNSS_4_searchweb.png",
                        "media_type": "Image",
                        "alt_text": "Credit: University of Michigan\r",
                        "width": 320,
                        "height": 180,
                        "pixels": 57600
                    }
                },
                {
                    "id": 263699,
                    "type": "media",
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                    "instance": {
                        "id": 418499,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_4_thm.png",
                        "filename": "CYGNSS_4_thm.png",
                        "media_type": "Image",
                        "alt_text": "Credit: University of Michigan\r",
                        "width": 80,
                        "height": 40,
                        "pixels": 3200
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 332048,
            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332048",
            "widget": "Single image",
            "title": "",
            "caption": "",
            "description": "<b>Figure 4</b> Top: Artist drawing of one of the eight CYGNSS satellites in orbit.<p>Bottom: A CYGNSS satellite in the lab during construction. <p>\rCredit: University of Michigan\r",
            "items": [
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                    "id": 263700,
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                    "instance": {
                        "id": 418501,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_5_print.jpg",
                        "filename": "CYGNSS_5_print.jpg",
                        "media_type": "Image",
                        "alt_text": "Figure 4 Top: Artist drawing of one of the eight CYGNSS satellites in orbit.Bottom: A CYGNSS satellite in the lab during construction. \rCredit: University of Michigan\r",
                        "width": 1024,
                        "height": 741,
                        "pixels": 758784
                    }
                },
                {
                    "id": 263701,
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                    "instance": {
                        "id": 418500,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_5.png",
                        "filename": "CYGNSS_5.png",
                        "media_type": "Image",
                        "alt_text": "Figure 4 Top: Artist drawing of one of the eight CYGNSS satellites in orbit.Bottom: A CYGNSS satellite in the lab during construction. \rCredit: University of Michigan\r",
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                        "height": 720,
                        "pixels": 715680
                    }
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            ],
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            "id": 332049,
            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332049",
            "widget": "Single image",
            "title": "",
            "caption": "",
            "description": "<b>Figure 5</b> All eight CYGNSS observatories prepped for launch on the Pegasus rocket. Launch is currently scheduled for Dec. 12, 2016 from Cape Canaveral, Florida.<p>\rCredit: University of Michigan\r",
            "items": [
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                    "id": 263702,
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                        "id": 418502,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_6.png",
                        "filename": "CYGNSS_6.png",
                        "media_type": "Image",
                        "alt_text": "Figure 5 All eight CYGNSS observatories prepped for launch on the Pegasus rocket. Launch is currently scheduled for Dec. 12, 2016 from Cape Canaveral, Florida.\rCredit: University of Michigan\r",
                        "width": 1364,
                        "height": 751,
                        "pixels": 1024364
                    }
                },
                {
                    "id": 263703,
                    "type": "media",
                    "extra_data": null,
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                    "instance": {
                        "id": 418503,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/CYGNSS_6_print.jpg",
                        "filename": "CYGNSS_6_print.jpg",
                        "media_type": "Image",
                        "alt_text": "Figure 5 All eight CYGNSS observatories prepped for launch on the Pegasus rocket. Launch is currently scheduled for Dec. 12, 2016 from Cape Canaveral, Florida.\rCredit: University of Michigan\r",
                        "width": 1024,
                        "height": 563,
                        "pixels": 576512
                    }
                }
            ],
            "extra_data": {}
        },
        {
            "id": 332050,
            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332050",
            "widget": "Single image",
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            "description": "<b>Figure 6</b>  Climate change occurs when there is a change in the balance between incoming energy and outgoing energy from Earth. Virtually all the energy input to Earth comes from the sun. This is approximately balanced by Earth putting energy back into space from a combination of reflected solar energy and thermally emitted energy. The inputs and outputs are not exactly balanced. Part of the reason is greenhouse gases, which trap some of the energy that would otherwise go back to space. This small imbalance leads to changes in Earth’s climate.<p>\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
            "items": [
                {
                    "id": 263704,
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                    "instance": {
                        "id": 418504,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/RAVAN_Swartz_1.jpg",
                        "filename": "RAVAN_Swartz_1.jpg",
                        "media_type": "Image",
                        "alt_text": "Figure 6  Climate change occurs when there is a change in the balance between incoming energy and outgoing energy from Earth. Virtually all the energy input to Earth comes from the sun. This is approximately balanced by Earth putting energy back into space from a combination of reflected solar energy and thermally emitted energy. The inputs and outputs are not exactly balanced. Part of the reason is greenhouse gases, which trap some of the energy that would otherwise go back to space. This small imbalance leads to changes in Earth’s climate.\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
                        "width": 1024,
                        "height": 768,
                        "pixels": 786432
                    }
                },
                {
                    "id": 439036,
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                    "instance": {
                        "id": 1100701,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/small-satellites-for-earth-science-fig-6.hwshow",
                        "filename": "small-satellites-for-earth-science-fig-6.hwshow",
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        {
            "id": 332051,
            "url": "https://svs.gsfc.nasa.gov/12410/#media_group_332051",
            "widget": "Single image",
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            "description": "<b>Figure 7</b> Radiometer Assessment using Vertically Aligned Nanotubes, or RAVAN, is a 3 Unit CubeSat that is going to demonstrate new technologies for measuring energy at the top of the atmosphere. These observations have the potential to improve spaceborne measurements of Earth’s energy imbalance in the future. RAVAN is funded by NASA’s Earth Science Technology Office.<p>\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
            "items": [
                {
                    "id": 263705,
                    "type": "media",
                    "extra_data": null,
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                    "instance": {
                        "id": 418505,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/RAVAN_Swartz_2.jpg",
                        "filename": "RAVAN_Swartz_2.jpg",
                        "media_type": "Image",
                        "alt_text": "Figure 7 Radiometer Assessment using Vertically Aligned Nanotubes, or RAVAN, is a 3 Unit CubeSat that is going to demonstrate new technologies for measuring energy at the top of the atmosphere. These observations have the potential to improve spaceborne measurements of Earth’s energy imbalance in the future. RAVAN is funded by NASA’s Earth Science Technology Office.\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
                        "width": 1024,
                        "height": 768,
                        "pixels": 786432
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                }
            ],
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        {
            "id": 332052,
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            "widget": "Single image",
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            "description": "<b>Figure 8</b> RAVAN will demonstrate the use of vertically aligned carbon nanotubes as the absorber in a compact and accurate radiometer. The carbon nanotubes stand on end like a bundle of straws or trees in a forest. They appear incredibly black because once energy is absorbed inside the tubes it is very difficult to reflect out. This makes them effective absorbers of Earth’s outgoing energy at ultraviolet, visible and infrared wavelengths of light. In the picture, the quarter inch patch in the center is a small “forest” of nanotubes.<p>\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
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                {
                    "id": 263706,
                    "type": "media",
                    "extra_data": null,
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                    "instance": {
                        "id": 418506,
                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/RAVAN_Swartz_3.jpg",
                        "filename": "RAVAN_Swartz_3.jpg",
                        "media_type": "Image",
                        "alt_text": "Figure 8 RAVAN will demonstrate the use of vertically aligned carbon nanotubes as the absorber in a compact and accurate radiometer. The carbon nanotubes stand on end like a bundle of straws or trees in a forest. They appear incredibly black because once energy is absorbed inside the tubes it is very difficult to reflect out. This makes them effective absorbers of Earth’s outgoing energy at ultraviolet, visible and infrared wavelengths of light. In the picture, the quarter inch patch in the center is a small “forest” of nanotubes.\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
                        "width": 1024,
                        "height": 768,
                        "pixels": 786432
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            ],
            "extra_data": {}
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            "widget": "Single image",
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            "description": "<b>Figure 9</b> If the first RAVAN pathfinder mission is successful, the next step would be proposing a constellation of multiple RAVAN satellites distributed around the planet to measure Earth’s outgoing energy globally, 24/7.<p>\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
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                    "id": 263707,
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                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/RAVAN_Swartz_4.jpg",
                        "filename": "RAVAN_Swartz_4.jpg",
                        "media_type": "Image",
                        "alt_text": "Figure 9 If the first RAVAN pathfinder mission is successful, the next step would be proposing a constellation of multiple RAVAN satellites distributed around the planet to measure Earth’s outgoing energy globally, 24/7.\rCredit: Johns Hopkins University Applied Physics Laboratory\r",
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                        "height": 768,
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                },
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            "description": "<b>Figure 10</b> An important way to improve forecasts of tropical cyclone intensity is to see what’s going on inside and around them while they’re happening. That’s the goal of the TROPICS mission, 12 CubeSats that will fly in formation to track the temperature and humidity of storm environments. The TROPICS CubeSats will get very frequent measurements, similar to X-rays, that cut through the overall cloud-cover (black and white part of the image) so we can see the storm’s underlying structure (shown in color). The storm structures known as the eyewall – tall clouds, wind and rain around the eye – and rainbands – the rainy parts of the spiral arms – give us clues about whether a storm is primed to intensify into a category 4 or 5 storm, something everyone in their path needs to know.<p>\rCredit: Scott Braun, NASA GSFC (colored part of image); and Naval Research Laboratory (black/white part of image)\r",
            "items": [
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                    "id": 263708,
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                        "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012410/Blackwell_Figure1.png",
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                        "media_type": "Image",
                        "alt_text": "Figure 10 An important way to improve forecasts of tropical cyclone intensity is to see what’s going on inside and around them while they’re happening. That’s the goal of the TROPICS mission, 12 CubeSats that will fly in formation to track the temperature and humidity of storm environments. The TROPICS CubeSats will get very frequent measurements, similar to X-rays, that cut through the overall cloud-cover (black and white part of the image) so we can see the storm’s underlying structure (shown in color). The storm structures known as the eyewall – tall clouds, wind and rain around the eye – and rainbands – the rainy parts of the spiral arms – give us clues about whether a storm is primed to intensify into a category 4 or 5 storm, something everyone in their path needs to know.\rCredit: Scott Braun, NASA GSFC (colored part of image); and Naval Research Laboratory (black/white part of image)\r",
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                        "alt_text": "Figure 10 An important way to improve forecasts of tropical cyclone intensity is to see what’s going on inside and around them while they’re happening. That’s the goal of the TROPICS mission, 12 CubeSats that will fly in formation to track the temperature and humidity of storm environments. The TROPICS CubeSats will get very frequent measurements, similar to X-rays, that cut through the overall cloud-cover (black and white part of the image) so we can see the storm’s underlying structure (shown in color). The storm structures known as the eyewall – tall clouds, wind and rain around the eye – and rainbands – the rainy parts of the spiral arms – give us clues about whether a storm is primed to intensify into a category 4 or 5 storm, something everyone in their path needs to know.\rCredit: Scott Braun, NASA GSFC (colored part of image); and Naval Research Laboratory (black/white part of image)\r",
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            "description": "<b>Figure 11</b> With 12 individual CubeSats, one of the TROPICS constellation CubeSats will fly over any part of the tropics (between 40 degrees latitude North and South) about every half hour. This frequent revisit time will allow the mission to capture the quickly changing features of tropical cyclones as they progress. Each CubeSat in the constellation is about the size of a loaf of bread and weighs eight pounds, flying 350 miles above Earth. They each host a sophisticated microwave instrument that scans across Earth’s surface once every two seconds to provide three-dimensional information on the storm’s structure, like a CAT-Scan. The CubeSats’ small size (relative to present weather satellites that can be almost as large as a SUV) allows them to be built and launched quickly and at low cost.<p>\rCredit: MIT Lincoln Laboratory\r",
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                        "alt_text": "Figure 11 With 12 individual CubeSats, one of the TROPICS constellation CubeSats will fly over any part of the tropics (between 40 degrees latitude North and South) about every half hour. This frequent revisit time will allow the mission to capture the quickly changing features of tropical cyclones as they progress. Each CubeSat in the constellation is about the size of a loaf of bread and weighs eight pounds, flying 350 miles above Earth. They each host a sophisticated microwave instrument that scans across Earth’s surface once every two seconds to provide three-dimensional information on the storm’s structure, like a CAT-Scan. The CubeSats’ small size (relative to present weather satellites that can be almost as large as a SUV) allows them to be built and launched quickly and at low cost.\rCredit: MIT Lincoln Laboratory\r",
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                        "alt_text": "Figure 11 With 12 individual CubeSats, one of the TROPICS constellation CubeSats will fly over any part of the tropics (between 40 degrees latitude North and South) about every half hour. This frequent revisit time will allow the mission to capture the quickly changing features of tropical cyclones as they progress. Each CubeSat in the constellation is about the size of a loaf of bread and weighs eight pounds, flying 350 miles above Earth. They each host a sophisticated microwave instrument that scans across Earth’s surface once every two seconds to provide three-dimensional information on the storm’s structure, like a CAT-Scan. The CubeSats’ small size (relative to present weather satellites that can be almost as large as a SUV) allows them to be built and launched quickly and at low cost.\rCredit: MIT Lincoln Laboratory\r",
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            "description": "<b>Figure 12</b> Each TROPICS CubeSat has three things: the science instrument, solar panels, and the spacecraft bus which runs the whole operation. The bus manages the power system, controls the spin and orientation of the instrument as well as its operation, and communicates with the ground over a radio link. \r\rOver the last five years, technology has advanced rapidly to miniaturize the systems of both the spacecraft bus and the science instrument. This has led to the development of advanced components such as reaction wheels that spin up to 10,000 rotations per minute inside the spacecraft to keep it stable and high-resolution cameras that continuously track stars in the sky to enable attitude determination. \r\rPrevious NASA-funded CubeSat missions serve as pathfinders and test beds for these new technologies. One example that feeds into the TROPICS mission is the MiRaTA CubeSat project, led by Prof. Kerri Cahoy at MIT. Many of the key microwave instrument technologies were first developed and tested by the MiRaTA project, reducing risk for the TROPICS mission.<p>\rCredit: MIT Lincoln Laboratory\r",
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                        "alt_text": "Figure 12 Each TROPICS CubeSat has three things: the science instrument, solar panels, and the spacecraft bus which runs the whole operation. The bus manages the power system, controls the spin and orientation of the instrument as well as its operation, and communicates with the ground over a radio link. \r\rOver the last five years, technology has advanced rapidly to miniaturize the systems of both the spacecraft bus and the science instrument. This has led to the development of advanced components such as reaction wheels that spin up to 10,000 rotations per minute inside the spacecraft to keep it stable and high-resolution cameras that continuously track stars in the sky to enable attitude determination. \r\rPrevious NASA-funded CubeSat missions serve as pathfinders and test beds for these new technologies. One example that feeds into the TROPICS mission is the MiRaTA CubeSat project, led by Prof. Kerri Cahoy at MIT. Many of the key microwave instrument technologies were first developed and tested by the MiRaTA project, reducing risk for the TROPICS mission.\rCredit: MIT Lincoln Laboratory\r",
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            "description": "<b>Figure 13</b> The TROPICS and MiRaTA projects are made up of a broad team drawing from a national lab (MIT Lincoln Laboratory), universities (including MIT and University of Massachusetts), NASA, and NOAA. Students involved in the projects bring boundless energy that can be effectively brought to bear under the guidance of seasoned experts and faculty.<p>\rCredit: MIT Lincoln Laboratory\r",
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                        "alt_text": "Figure 13 The TROPICS and MiRaTA projects are made up of a broad team drawing from a national lab (MIT Lincoln Laboratory), universities (including MIT and University of Massachusetts), NASA, and NOAA. Students involved in the projects bring boundless energy that can be effectively brought to bear under the guidance of seasoned experts and faculty.\rCredit: MIT Lincoln Laboratory\r",
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        {
            "id": 12411,
            "url": "https://svs.gsfc.nasa.gov/12411/",
            "page_type": "Produced Video",
            "title": "NASA to Launch New Small Satellite Missions to do Real Science",
            "description": "NASA is about to launch six new next-generation Earth-observing small satellites — some as small as a loaf of bread. These tiny spacecraft are helping to foster creative and cost-effective approaches to studying our planet. This page contains a short overview video as well as a series of conceptual animations of small sats being launched, deployed, in orbit over the Earth collecting data, and in comparison in size to both a person and a traditional large satellite. Note:  While these animations are based on real satellite models, they are intended to be generic and not perfectly descriptive of any particular small sat mission. For more on NASA’s small satellite program: https://www.nasa.gov/press-release/nasa-to-hold-media-call-on-new-small-satellite-missions-to-study-earth. || ",
            "release_date": "2016-11-07T12:00:00-05:00",
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                "url": "https://svs.gsfc.nasa.gov/vis/a010000/a012400/a012411/Words_on_screen_final.00360_print.jpg",
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                "media_type": "Image",
                "alt_text": "This short overview video outlines the capabilities of small satellites. Complete transcript available.",
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