https://www.nasa.gov/missions/tech-demonstration/deep-space-atomic-clock/what-is-an-atomic-clock/ NASA Logo * Explore Search [ ] NASA Logo * News & Events News & Events + All NASA News + Video Series on NASA+ + Podcasts + Blogs + Newsletters + Social Media + Media Resources + Events + Upcoming Launches & Landings + Virtual Guest Program * Multimedia Multimedia + NASA+ + Images + NASA Live + NASA Apps + Podcasts + Image of the Day + e-Books + Sounds and Ringtones + Interactives + STEM Multimedia * NASA+ Search [ ] Suggested Searches * Climate Change * Artemis * Expedition 64 * Mars perseverance * SpaceX Crew-2 * International Space Station * View All Topics A-Z * Home * Missions * Humans in Space * Earth & Climate * The Solar System * The Universe * Science * Aeronautics * Technology * Learning Resources * About NASA * Espanol ----------------------------------------------------------------- * News & Events * Multimedia * NASA+ Featured There are three images. The top right is Cassiopeia A. This image of Cassiopeia A resembles a disk of electric light with red clouds, glowing white streaks, red and orange flames, and an area near the center of the remnant resembling a somewhat circular region of green lightning. X-rays from Chandra are blue and reveal hot gas, mostly from supernova debris from the destroyed star, and include elements like silicon and iron. X-rays are also present as thin arcs in the outer regions of the remnant. Infrared data from Webb is red, green, and blue. Webb highlights infrared emission from dust that is warmed up because it is embedded in the hot gas seen by Chandra, and from much cooler supernova debris. Hubble data shows a multitude of stars that permeate the field of view. The image on the bottom is 30 Doradus. This release features a composite image of 30 Doradus, otherwise known as the Tarantula Nebula, a region of active star formation in a neighboring galaxy. In the image, royal blue and purple gas clouds interact with red and orange gas clouds. Specks of light and large gleaming stars peek through the colourful clouds. The patches of royal blue and purple gas clouds represent X-ray data collected by the Chandra Observatory. The brightest and most prominent blue cloud appears at the center of the image, roughly shaped like an upward pointing triangle. Darker X-ray clouds can be found near the right and left edges of the image. The red and orange gas clouds represent infrared data from the James Webb Space Telescope. These patches resemble clouds of roiling fire. The brightest and most prominent infrared cloud appears at our upper left, roughly shaped like a downward pointing triangle. Wispy white clouds outline the upward pointing bright blue triangle in the center of the image. Inside this frame is a brilliant gleaming star with six long, thin, diffraction spikes. Beside it is a cluster of smaller bright specks showing young stars in the nebula. The final image is NGC 6872. In this composite image, a large spiral galaxy has some of its superheated gas stolen by a smaller, nearby neighbor. Centered in the frame, NGC 6872 is a large spiral galaxy with two elongated arms that stretch toward our upper right and lower left. Near the white dot at the heart of the galaxy, a cloud of neon purple tints the arms, which appear steel blue at the tips. The purple represents hot gas detected by Chandra. Just to the upper left of NGC 6872 is a second spiral galaxy. Its spiraling arms are much smaller, but the bright white dot at its core is quite large, suggesting a supermassive black hole. 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The headshot image of NASA NASA Jun 19, 2019 Article * * * * Contents * Why do we use clocks to navigate in space? * What do atoms have to do with clocks? * What's unique about the Deep Space Atomic Clock? [dsac-16b] The clock is ticking: A technology demonstration that could transform the way humans explore space is nearing its target launch date of June 24, 2019. Developed by NASA's Jet Propulsion Laboratory in Pasadena, California, the Deep Space Atomic Clock is a serious upgrade to the satellite-based atomic clocks that, for example, enable the GPS on your phone. Ultimately, this new technology could make spacecraft navigation to distant locations like Mars more autonomous. But what is an atomic clock? How are they used in space navigation, and what makes the Deep Space Atomic Clock different? Read on to get all the answers. Read more: Five Things to Know About NASA's Deep Space Atomic Clock Why do we use clocks to navigate in space? To determine a spacecraft's distance from Earth, navigators send a signal to the spacecraft, which then returns it to Earth. The time the signal requires to make that two-way journey reveals the spacecraft's distance from Earth, because the signal travels at a known speed (the speed of light). While it may sound complicated, most of us use this concept every day. The grocery store might be a 30-minute walk from your house. If you know you can walk about a mile in 20 minutes, then you can calculate the distance to the store. By sending multiple signals and taking many measurements over time, navigators can calculate a spacecraft's trajectory: where it is and where it's headed. Most modern clocks, from wristwatches to those used on satellites, keep time using a quartz crystal oscillator. These devices take advantage of the fact that quartz crystals vibrate at a precise frequency when voltage is applied to them. The vibrations of the crystal act like the pendulum of a grandfather clock, ticking off how much time has passed. To know the spacecraft's position within a meter, navigators need clocks with precision time resolution -- clocks that can measure billionths of a second. Navigators also need clocks that are extremely stable. "Stability" refers to how consistently a clock measures a unit of time; its measurement of the length of a second, for example, needs to be the same (to better than a billionth of a second) over days and weeks. Read more: NASA Navigation Tech Shows Timing Really Is Everything What do atoms have to do with clocks? By space navigation standards, quartz crystal clocks aren't very stable. After only an hour, even the best-performing quartz oscillators can be off by a nanosecond (one billionth of a second). After six weeks, they may be off by a full millisecond (one thousandth of a second), or a distance error of 185 miles (300 kilometers). That would have a huge impact on measuring the position of a fast-moving spacecraft. Atomic clocks combine a quartz crystal oscillator with an ensemble of atoms to achieve greater stability. NASA's Deep Space Atomic Clock will be off by less than a nanosecond after four days and less than a microsecond (one millionth of a second) after 10 years. This is equivalent to being off by only one second every 10 million years. Atoms are composed of a nucleus (consisting of protons and neutrons) surrounded by electrons. Each element on the periodic table represents an atom with a certain number of protons in its nucleus. The number of electrons swarming around the nucleus can vary, but they must occupy discreet energy levels, or orbits. A jolt of energy -- in the form of microwaves -- can cause an electron to rise to a higher orbit around the nucleus. The electron must receive exactly the right amount of energy -- meaning the microwaves must have a very specific frequency -- in order to make this jump. The energy required to make electrons change orbits is unique in each element and consistent throughout the universe for all atoms of a given element. For instance, the frequency necessary to make electrons in a carbon atom change energy levels is the same for every carbon atom in the universe. The Deep Space Atomic Clock uses mercury atoms; a different frequency is necessary to make those electrons change levels, and that frequency will be consistent for all mercury atoms. "The fact that the energy difference between these orbits is such a precise and stable value is really the key ingredient for atomic clocks," said Eric Burt, an atomic clock physicist at JPL. "It's the reason atomic clocks can reach a performance level beyond mechanical clocks." Being able to measure this unchangeable frequency in a particular atom offers science a universal, standardized measurement of time. ("Frequency" refers to the number of waves that pass a particular point in space in a given unit of time. So, by counting waves, it's possible to measure time.) In fact, the official measurement of the length of a second is determined by the frequency needed to make electrons jump between two specific energy levels in a cesium atom. In an atomic clock, the frequency of the quartz oscillator is transformed into a frequency that is applied to a collection of atoms. If the derived frequency is correct, it will cause many electrons in the atoms to change energy levels. If the frequency is incorrect, far fewer electrons will jump. This will determine if the quartz oscillator is off-frequency and by how much. A "correction" determined by the atoms can then be applied to the quartz oscillator to steer it back to the correct frequency. This type of correction is calculated and applied to the quartz oscillator every few seconds in the Deep Space Atomic Clock. What's unique about the Deep Space Atomic Clock? Atomic clocks are used onboard GPS satellites that orbit the Earth, but even they must be sent updates two times per day to correct the clocks' natural drift. Those updates come from more stable atomic clocks on the ground that are large (often the size of a refrigerator) and not designed to survive the physical demands of going to space. Up to 50 times more stable than the atomic clocks on GPS satellites, NASA's Deep Space Atomic Clock is intended to be the most stable atomic clock ever flown in space. It achieves this stability by using mercury ions. Ions are atoms that have a net electric charge, rather than being electrically neutral. In any atomic clock, the atoms are contained in a vacuum chamber, and in some of those clocks, atoms interact with the vacuum chamber walls. Environmental changes such as temperature will then cause similar changes in the atoms and lead to frequency errors. Many atomic clocks use neutral atoms, but because the mercury ions have an electric charge, they can be contained in an electromagnetic "trap" to prevent this interaction from happening, allowing the Deep Space Atomic Clock to achieve a new level of precision. For missions going to distant destinations like Mars or other planets, such precision makes autonomous navigation possible with minimal communication to and from Earth -- a huge improvement in how spacecraft are currently navigated. Read more: How an Atomic Clock Will Get Humans to Mars on Time The Deep Space Atomic Clock is hosted on a spacecraft provided by General Atomics Electromagnetic Systems of Englewood, Colorado. It is sponsored by the Technology Demonstration Missions program within NASA's Space Technology Mission Directorate and the Space Communications and Navigations program within NASA's Human Exploration and Operations Mission Directorate. JPL manages the project. Video File for Media Click to download the posters Arielle Samuelson Jet Propulsion Laboratory, Pasadena, Calif. 818-354-0307 arielle.a.samuelson@jpl.nasa.gov NASA Logo National Aeronautics and Space Administration NASA explores the unknown in air and space, innovates for the benefit of humanity, and inspires the world through discovery. * About NASA's Mission Join Us * Home * News & Events * Multimedia * NASA+ * Missions * Humans in Space * Earth & Climate * The Solar System * The Universe * Science * Aeronautics * Technology * Learning Resources * About NASA * NASA en Espanol Follow NASA * * * * * More NASA Social Accounts * NASA Newsletters * Sitemap * For Media * Privacy Policy * FOIA * No FEAR Act * Office of the IG * Budget & Annual Reports * Agency Financial Reports * Contact NASA * Accessibility * Page Last Updated: Aug 16, 2023 * Page Editor: Naomi Hartono * Responsible NASA Official: Abigail Bowman