Results for “transit method”
TESS Mission
** The Transiting Exoplanet Survey Satellite (TESS) is NASA’s wide‑field space telescope that, since 2018, has been scanning nearly the entire sky to discover thousands of nearby exoplanets using the transit method. **CONTENT:** ## Overview The **Transiting Exoplanet Survey Satellite (TESS)** is a small, highly capable space telescope built under NASA’s Explorer program. Unlike its predecessor Kepler, which stared at a single patch of the Milky Way, TESS is designed to monitor almost the whole celestial sphere, covering an area **about 400 times larger** than Kepler’s field of view. Its four wide‑angle cameras continuously record the brightness of millions of stars, searching for the tell‑tale dip that occurs when a planet passes in front of its host star. By focusing on bright, nearby stars, TESS enables rapid follow‑up observations with ground‑based telescopes and larger space observatories such as the James Webb Space Telescope (JWST), opening a path toward detailed atmospheric characterization. TESS operates in a **highly elliptical 13.70‑day orbit** known as a “high‑elliptical lunar‑synchronous orbit,” which keeps the spacecraft well away from Earth’s radiation belts while providing a stable thermal environment and continuous sky coverage. The satellite’s four identical lenses each have a 24° × 24° field of view, together delivering a combined 24° × 96° swath that sweeps across the sky in 27‑day sectors. Over its primary two‑year mission, TESS completed a full‑sky survey, and an extended mission continues to refine planet catalogs and explore additional astrophysical phenomena such as stellar flares, asteroseismology, and solar system objects. ## History/Background The concept for a wide‑field exoplanet hunter originated in the early 2000s, when astronomers recognized the need for a mission that could complement Kepler’s deep but narrow survey. In 2013, NASA selected TESS as an **Explorer-class mission** after a competitive proposal process led by the Massachusetts Institute of Technology’s (MIT) Kavli Institute for Astrophysics and Space Research. The spacecraft was built by **Ball Aerospace**, with the four cameras supplied by **MIT Lincoln Laboratory**. Key milestones include: - **June 2017:** Completion of spacecraft integration and testing. - **18 April 2018:** Launch aboard a **SpaceX Falcon 9** from Cape Canaveral. - **7 August 2018:** First light image captured, showcasing the full‑frame view of the Large Magellanic Cloud. - **17 September 2018:** Public release of the first light image, confirming instrument performance. - **July 2019:** Announcement of the first batch of TESS exoplanet candidates, including the notable super‑Earth **π Mensae b**. Following the successful primary mission (July 2018 – July 2020), NASA approved an extended mission that began in 2021, allowing TESS to revisit previously observed sectors, improve detection sensitivity, and target the ecliptic poles for continuous monitoring. ## Key Information - **Orbit:** 13.70‑day highly elliptical, 108,000 km apogee, 17,000 km perigee; 2:1 resonance with the Moon. - **Cameras:** Four identical f/1.4 refractive optics, each with a 10‑cm aperture and a 100‑megapixel CCD array. - **Survey Strategy:** 27‑day observation per sector; 13‑month full‑sky coverage; 2‑minute cadence for pre‑selected target stars, 30‑minute full‑frame images. - **Data Yield:** Over **5,000** planet candidates identified to date; more than **2,800** confirmed exoplanets, many of them **Earth‑size to sub‑Neptune** in size and orbiting bright (V < 12) stars. - **Notable Discoveries:** The ultra‑short‑period planet **TOI‑700 e** (Earth‑size in the habitable zone), the multi‑planet system **L 98‑59**, and the first transiting exoplanet around a **white dwarf** (WD 1856 b). - **Community Involvement:** TESS data are released to the public within weeks, enabling citizen‑science projects like **Planet Hunters TESS** and fostering rapid follow‑up by the global astronomical community. ## Significance TESS has transformed exoplanet science by shifting the focus from distant, faint stars to **nearby, bright hosts** that are amenable to detailed spectroscopic study. This strategic pivot accelerates the search for potentially habitable worlds and the characterization of planetary atmospheres, a prerequisite for assessing biosignatures. Moreover, TESS’s all‑sky approach has democratized exoplanet discovery, allowing observatories of all sizes to contribute to validation and mass measurement campaigns. The mission also serves as a technological testbed for future wide‑field space telescopes, informing design choices for concepts such as the **Habitable Exoplanet Imaging Mission (HabEx)** and the **Large UV/Optical/IR Surveyor (LUVOIR)**. In a broader sense, TESS’s success underscores the power of modest‑cost, high‑impact Explorer missions to address fundamental questions about our place in the cosmos. **INFOBOX:** - Name: Transiting Exoplanet Survey Satellite - Type: Space telescope (NASA Explorer mission) - Date: Launched 18 April 2018 - Location: Highly elliptical 13.70‑day Earth‑Moon resonant orbit - Known For: Discovering thousands of exoplanets around bright, nearby stars **TAGS:** exoplanets, transit method, NASA, space telescope, TESS, astrophysics, planetary science, Kepler successor
Space & AstronomyTRAPPIST-1e
TRAPPIST-1e is a close-to-Earth-sized exoplanet orbiting within the habitable zone of the ultracool dwarf star TRAPPIST-1, located 40.7 light-years away from Earth in the constellation of Aquarius. ## Overview TRAPPIST-1e is one of seven Earth-sized planets discovered orbiting the ultracool dwarf star TRAPPIST-1, located in the constellation of Aquarius. The star, a type of **M-dwarf**, is about 8% the mass of the Sun and has a surface temperature of around 2,500 Kelvin (4,000°F). The TRAPPIST-1 system is of great interest to astronomers due to its proximity to Earth and the presence of multiple planets in the habitable zone, where liquid water could exist on their surfaces. The discovery of TRAPPIST-1e and its siblings was announced in 2017 by a team of astronomers using the **Spitzer Space Telescope**. The team used the transit method to detect the planets, which involves measuring the dimming of a star as a planet passes in front of it. This technique allows astronomers to infer the presence of a planet and its size, but not its mass or composition. ## History/Background The discovery of TRAPPIST-1e is a result of a long-term monitoring campaign of the TRAPPIST-1 star by the Spitzer Space Telescope. The telescope was designed to study the infrared radiation emitted by cool stars, and it was used to search for planets orbiting TRAPPIST-1. The team of astronomers, led by Dr. Michaël Gillon, used a technique called the "transit method" to detect the planets. This method involves measuring the dimming of a star as a planet passes in front of it, which allows astronomers to infer the presence of a planet and its size. ## Key Information - **Size**: TRAPPIST-1e is approximately 0.92 times the size of Earth, making it a close-to-Earth-sized exoplanet. - **Mass**: The mass of TRAPPIST-1e is not directly known, but it is estimated to be around 0.9 times the mass of Earth. - **Orbital Period**: TRAPPIST-1e orbits its star every 6.1 days, which is relatively close to the star. - **Surface Temperature**: The surface temperature of TRAPPIST-1e is estimated to be around 0°C (32°F), which is close to the freezing point of water. - **Habitability**: TRAPPIST-1e is considered a potentially habitable exoplanet due to its location in the habitable zone and its size, which suggests that it may have a solid surface. ## Significance The discovery of TRAPPIST-1e and its siblings has significant implications for the search for life beyond Earth. The presence of multiple planets in the habitable zone of TRAPPIST-1 increases the likelihood of finding life on one of these planets. Additionally, the study of TRAPPIST-1e and its siblings provides valuable insights into the formation and evolution of planetary systems. INFOBOX: - Name: TRAPPIST-1e - Type: Rocky exoplanet - Date: Announced in 2017 - Location: TRAPPIST-1 system, 40.7 light-years away from Earth in the constellation of Aquarius - Known For: Potentially habitable exoplanet in the TRAPPIST-1 system TAGS: TRAPPIST-1, exoplanet, habitable zone, rocky planet, Spitzer Space Telescope, transit method, ultracool dwarf star, M-dwarf, planetary system, astrobiology, astronomy.