Possible dwarf planets

Dwarf planets are celestial bodies that orbit the Sun and are similar to planets but do not meet all the criteria to be classified as such. The International Astronomical Union (IAU) defines a dwarf planet as a body that: 1. Orbits the Sun 2. Is not a satellite (i.e., it is not a moon of another body) 3.

Former dwarf planet candidates refer to celestial bodies in the solar system that were considered for classification as dwarf planets but ultimately were not designated as such, either due to lack of sufficient evidence or because they did not meet all the criteria established by the International Astronomical Union (IAU) for dwarf planet status. To be classified as a dwarf planet, a celestial body must: 1. Orbit the Sun.

(119951) 2002 KX14 is a trans-Neptunian object, classified as a centaur or a scattered disc object. It was discovered in May 2002 and is part of a group of icy bodies located beyond the orbit of Neptune in the outer solar system. Due to its size and characteristics, it falls under the category of minor planets or asteroids. These types of objects can offer valuable insights into the early solar system and the formation of planetary bodies.

(119979) 2002 WC19 is an asteroid that belongs to the outer region of the asteroid belt. It was discovered on November 24, 2002. Like many asteroids in this belt, it orbits the Sun between Mars and Jupiter. The specific label "(119979)" is its provisional designation, indicating it has been assigned a number in the astronomical catalog of discovered asteroids.

The notation (120132) 2003 FY128 appears to be a reference to a specific number or identifier, but its exact meaning is not clear without additional context. It could represent a variety of things depending on the field it pertains to, such as a code for a product, a financial year designation, or even a specific document or case number. - **120132** might be a part number, client ID, or some other identifier.

(120348) 2004 TY364 is a trans-Neptunian object (TNO) located in the Kuiper Belt, a region of the Solar System beyond the orbit of Neptune that is populated with many small celestial bodies. It was discovered on October 6, 2004, and is classified as a scattered disk object, which means it has an orbit that is more eccentric and inclined compared to those of other Kuiper Belt objects.

(144897) 2004 UX10 is a near-Earth object (NEO) classified as an asteroid. Specifically, it is part of the Apollo group of asteroids, which are characterized by their orbits that cross Earth's orbit. Discovered in 2004, it is an example of a potentially hazardous asteroid due to its size and proximity to Earth's orbit.

(145451) 2005 RM43 is a numbered asteroid that belongs to the asteroid belt between Mars and Jupiter. It was discovered in 2005 and classified as a member of the Hilda family of asteroids. These asteroids are characterized by their stable orbits that are located in a 3:2 resonance with Jupiter. Asteroids like (145451) 2005 RM43 provide valuable insights into the formation and evolution of our solar system.

(145452) 2005 RN43 is a minor planet or asteroid that is part of the asteroid belt in our solar system. It was discovered on September 8, 2005. Like other asteroids, it is composed of rock and metal and orbits the Sun. The designation "145452" refers to its number in the sequential list of discovered minor planets, while "2005 RN43" is its provisional designation, indicating it was discovered in the year 2005.

(145480) 2005 TB190 is a near-Earth object (NEO) that belongs to the category of asteroids. Specifically, it is classified as an Apollo asteroid, which means that its orbit crosses Earth's orbit. The object was discovered in 2005, as indicated by its designation. Like other NEOs, (145480) 2005 TB190 is of interest to astronomers and planetary scientists.

(15874) 1996 TL66 is an asteroid located in the asteroid belt between Mars and Jupiter. It was discovered on October 6, 1996, and assigned the provisional designation 1996 TL66. The number 15874 indicates that it is the 15,874th asteroid to be assigned a permanent number by the International Astronomical Union (IAU).

(202421) 2005 UQ513 is designated as a trans-Neptunian object, specifically a centaur, that resides in the outer region of our solar system. It was discovered in 2005 and is part of a group of icy bodies that exist beyond the orbit of Neptune. Centaur objects typically exhibit characteristics of both asteroids and comets, and they are thought to be remnants from the early solar system.

(208996) 2003 AZ84 is an asteroid that belongs to the Asteroid Belt, which is situated between the orbits of Mars and Jupiter. It was discovered on January 12, 2003, as part of an ongoing survey of near-Earth objects and asteroids.

(230965) 2004 XA192 is an asteroid that is part of the asteroid belt located between Mars and Jupiter. It was discovered in 2004 and is classified as a near-Earth object (NEO) due to its orbit bringing it relatively close to Earth's path around the Sun.

(24835) 1995 SM55 is a numbered asteroid that is part of the main asteroid belt in our solar system. It was discovered on September 23, 1995, and is classified as an Apollo-type near-Earth asteroid, which means it has an orbit that brings it close to Earth's orbit. The asteroid is a subject of interest for astronomers and researchers due to its potential for studying the properties of asteroids and their orbits.

(26375) 1999 DE9 is an asteroid that is part of the asteroid belt between Mars and Jupiter. It was discovered on February 23, 1999, and is classified as a Near-Earth Object (NEO). The object belongs to the Apollo group of asteroids, which are characterized by their orbits that cross Earth's orbit.

(278361) 2007 JJ43 is an asteroid that is part of the asteroid belt located between Mars and Jupiter. It was discovered on May 8, 2007, and is classified as a member of the main belt asteroids. The designation "278361" refers to its specific catalog number, while "2007 JJ43" is the provisional designation given upon its discovery. Like many asteroids, it provides valuable information about the early solar system and the formation of planetary bodies.

(303775) 2005 QU182 is a minor planet located in the outer region of the solar system, specifically classified as a centaur. Centaurs are small celestial bodies that have characteristics of both asteroids and comets, typically orbiting between the orbits of Jupiter and Neptune. This specific object was discovered in 2005.

(307261) 2002 MS4 is an asteroid that is part of the main belt, which is the region of space between the orbits of Mars and Jupiter where a majority of the solar system's asteroids are found. This particular asteroid was discovered in June 2002 and is classified as a "main-belt asteroid" in the asteroid catalog.

(309239) 2007 RW10 is a trans-Neptunian object (TNO) located in the Kuiper Belt, which is a region of the solar system beyond the orbit of Neptune that contains many small icy bodies. It was discovered in September 2007 and is classified as a member of the scattered disk, a group of TNOs that have highly elliptical orbits.

(315530) 2008 AP129 is a near-Earth object classified as an asteroid. It belongs to the group of asteroids known as Apollo asteroids, which are characterized by orbits that cross Earth's orbit. This specific asteroid was discovered in January 2008 and has been monitored due to its close proximity to Earth.

(35671) 1998 SN165 is an asteroid that is part of the main asteroid belt, which lies between the orbits of Mars and Jupiter. It was discovered on September 24, 1998, and is classified as a near-Earth object (NEO). The asteroid is named following the convention of minor planet naming, often based on various themes including characters, events, or places of significance.

(386723) 2009 YE7 is classified as a trans-Neptunian object (TNO) and is a member of the Kuiper Belt, which is a region of the Solar System beyond the orbit of Neptune filled with numerous small celestial bodies. It was discovered in 2009 and has been designated with the provisional designation 2009 YE7 before being assigned a permanent number.

(416400) 2003 UZ117 is a centaur, which is a type of small celestial body that orbits the Sun between the main asteroid belt and the outer planets, primarily the gas giants. Discovered in 2003, it has characteristics typical of both asteroids and comets. Centaurs are thought to be composed of frozen gases, similar to comets, but they also have a more solid structure, like asteroids.

(42301) 2001 UR163 is a small celestial body classified as a centaur, which is a type of object located between the orbits of Jupiter and Neptune. Centaurs are considered transitional objects because they share characteristics of both asteroids and comets. Discovered in 2001, (42301) 2001 UR163 has an irregular orbit and is believed to be composed of ice and rock.

(444030) 2004 NT33 is an asteroid that belongs to the main belt of asteroids, which is located between the orbits of Mars and Jupiter. The asteroid was discovered in 2004 and has been designated with the numerical identifier 444030. Like many asteroids in the main belt, it is composed primarily of rock and metal. Asteroids are classified based on their size, composition, and orbit, and many of them have their own unique characteristics and histories.

(445473) 2010 VZ98 is a minor planet, specifically classified as a trans-Neptunian object (TNO) in the Kuiper Belt. These objects are located beyond the orbit of Neptune and often have elongated orbits that can take them far from the Sun. Discovered in 2010, this object is part of a population that includes many icy bodies that are remnants from the early solar system.

(455502) 2003 UZ413 is a trans-Neptunian object (TNO) and a member of the Kuiper Belt, which is a region of the Solar System beyond the orbit of Neptune that is populated with many small icy bodies. This specific object was discovered in 2003 and is classified as a centaur due to its size and characteristics.

(469372) 2001 QF298 is classified as a trans-Neptunian object (TNO), specifically a centaur. Centaurs are celestial bodies that orbit between the orbits of Jupiter and Neptune. This particular object was discovered in 2001 and is part of the larger population of icy bodies located in the outer Solar System. You can typically find information on its orbital characteristics, size, and any significant studies conducted about it in astronomical databases or publications.

(470308) 2007 JH43 is an asteroid in the main belt, a region of space between the orbits of Mars and Jupiter where most of the solar system's asteroids are found. The designation "470308" refers to its catalog number assigned by the Minor Planet Center, while "2007 JH43" is the specific provisional designation given to the asteroid when it was first observed. This designation indicates that it was discovered in the year 2007.

(470599) 2008 OG19 is a near-Earth object (NEO) that is classified as an asteroid. It was discovered in 2008 and is part of the Apollo group of asteroids, which have orbits that cross Earth's path. The specific characteristics of 2008 OG19, such as its size, composition, and trajectory, are determined by observations made by astronomers and are subject to updates as new data is collected.

(471288) 2011 GM27 is a small asteroid that belongs to the main asteroid belt, which is located between the orbits of Mars and Jupiter. It was discovered on April 9, 2011, and is classified as a member of the Apollo group of asteroids, which are characterized by having orbits that bring them close to Earth's orbit.

(472271) 2014 UM33 is an asteroid that belongs to the main belt of asteroids in our solar system. It was discovered in October 2014, and it is classified as a member of the "Jupiter trojans" due to its orbital characteristics. Asteroids like 2014 UM33 are of interest to scientists because they can provide insights into the early solar system's conditions and the formation of planetary bodies.

(495603) 2015 AM281 is a designation for a specific near-Earth object (NEO), which is classified as an astroid. The number "495603" is its sequential designation indicating it is the 495,603rd NEO to be cataloged.

(496315) 2013 GP136 is an asteroid in the asteroid belt, which is located between the orbits of Mars and Jupiter. It was discovered on April 10, 2013. The asteroid is part of the larger population of objects that orbit the Sun and can vary widely in size, shape, and composition. Specific information about this asteroid's size, composition, and orbital characteristics would typically be available from astronomical databases and observatories that track such objects.

(501546) 2014 JJ80 is a minor planet, specifically classified as a trans-Neptunian object (TNO). It was discovered in 2014 and is part of the larger population of objects in the Kuiper Belt, which is a region of the solar system located beyond the orbit of Neptune. Minor planets like (501546) 2014 JJ80 are often of interest to astronomers studying the formation and evolution of the solar system.

(501581) 2014 OB394 is an asteroid belonging to the asteroid belt, which lies between the orbits of Mars and Jupiter. It was discovered in 2014 and has since been assigned the number 501581. Objects like this are typically categorized based on their size, orbit, and composition.

(505448) 2013 SA100 is a designation for a specific asteroid discovered in the asteroid belt. It is classified as a "trans-Neptunian object" (TNO), which generally refers to objects located beyond the orbit of Neptune. The asteroid was identified in 2013, and its numbering (505448) indicates that it has been officially cataloged.

(505624) 2014 GU53 is classified as a trans-Neptunian object (TNO), which means it orbits the Sun at a distance greater than that of Neptune. Specifically, it is part of the scattered disk, a distant region of the solar system populated by icy bodies. Objects like 2014 GU53 can provide valuable insights into the early solar system's formation and the processes that shaped it.

(523635) 2010 DN93 is a near-Earth object (NEO), specifically an asteroid that was discovered in 2010. Like other NEOs, it orbits the sun and has the potential to come close to Earth's orbit. The designation "523635" indicates that it is the 523,635th object that has been given a number in the sequential catalog of minor planets.

(523639) 2010 RE64 is a trans-Neptunian object (TNO) that is part of the Kuiper Belt, a region of the solar system beyond the orbit of Neptune filled with many small and icy bodies. This particular object was discovered in 2010 and has characteristics typical of other Kuiper Belt objects, such as being relatively small and composed mainly of frozen materials.

(523643) 2010 TY53 is a classified asteroids and part of the larger category of near-Earth objects (NEOs). Specifically, it is a member of the Apollo group of asteroids, which are known for their orbits that bring them close to Earth's orbit.

(523645) 2010 VK201 is the designation of a significant asteroid that is part of the asteroid belt. It was discovered in November 2010. It's categorized as a near-Earth object (NEO), specifically an Atira asteroid, meaning its orbit lies entirely within that of Earth's orbit.

(523671) 2013 FZ27 is a minor planet or asteroid that is part of the solar system. Specifically, it is classified as a near-Earth object (NEO), which means it has an orbit that brings it close to Earth's orbit. Discovered on March 18, 2013, it belongs to the Apollo group of asteroids, which are characterized by their orbits that cross Earth's orbit.

(523674) 2013 MA12 is a near-Earth object (NEO), specifically categorized as an asteroid. It is part of the Apollo group of asteroids, which have orbits that cross Earth's orbit. The designation includes the year of its discovery (2013) and a unique numerical identifier (MA12) assigned during the cataloging process.

(523683) 2014 CP23 is a designation for a specific asteroid, which is part of the larger category of near-Earth objects (NEOs). This designation indicates that it was discovered in 2014. The number 523683 represents its unique identifier in the catalogue of minor planets, while the letters 'CP' denote the spectroscopic class. Asteroids like 2014 CP23 can vary in size, composition, and orbit.

(523684) 2014 CQ23 is classified as a near-Earth object (NEO) and an Apollo asteroid. It was discovered on February 12, 2014. Near-Earth objects are asteroids or comets that have been nudged by the gravitational attraction of nearby planets into orbits that bring them into the Earth's neighborhood.

(523687) 2014 DF143 is a trans-Neptunian object, specifically classified as a further-out object in the Kuiper Belt. Discovered in 2014, it is categorized as a "cubewano," a type of classical Kuiper Belt object that has an orbit that is not significantly affected by the gravitational influence of Neptune.

(523692) 2014 EZ51 is classified as a near-Earth object (NEO) and more specifically, it is an Apollo-type asteroid. Apollo asteroids are a group of near-Earth asteroids whose orbits cross that of Earth's. The designation "523692" is its number in the minor planet catalog, and "2014 EZ51" refers to the specific designation given to it when it was discovered, indicating that it was identified in the year 2014.

(523702) 2014 HW199 is an asteroid that belongs to the Kuiper Belt, which is a region of the Solar System beyond the orbit of Neptune populated with many small icy bodies. It was discovered in April 2014 and is classified as a Trans-Neptunian Object (TNO). Characteristics such as its size, orbit, and specific details about its composition may evolve with further observations and research.

(523706) 2014 HF200 is a designated asteroidal object within our solar system. It is classified as a near-Earth object (NEO), specifically an Apollo-type asteroid, which means its orbit crosses that of Earth. Discovered in 2014, it has been studied for its physical characteristics, orbital parameters, and potential impact risks. As a small Solar System body, 2014 HF200 may provide insights into the formation and evolution of our solar system.

(523727) 2014 NW65 is a designation for a trans-Neptunian object (TNO) that was discovered in 2014. It is classified as a cubewano, which is a type of icy body located in the Kuiper Belt that does not have significant gravitational influences from Neptune. These objects often have stable orbits and are sometimes referred to as "classical" Kuiper Belt Objects (KBOs).

(523759) 2014 WK509 is an asteroid that is part of the Apollo group of near-Earth objects. Discovered in 2014, it is notable for its relatively close approach to Earth and is classified as a potentially hazardous asteroid (PHA) due to its size and orbit.

(523794) 2015 RR245 is a trans-Neptunian object (TNO) located in the outer region of the Solar System, specifically in the Kuiper Belt. It is classified as a dwarf planet candidate due to its size and characteristics.

(524435) 2002 CY248 is a trans-Neptunian object (TNO) and a centaur, which is a class of small celestial bodies located in the outer Solar System, often between the orbits of Jupiter and Neptune. This specific object was discovered in 2002 and is known for its properties as a detached object, meaning its orbit does not interact significantly with Neptune.

(527603) 2007 VJ305 is a classified asteroid that is part of the main belt of asteroids in our solar system. Identified by the Minor Planet Center, it was discovered in 2007. Like many asteroids, it can provide valuable information about the early solar system since they are considered remnants from the formation of the solar system approximately 4.6 billion years ago.

(528381) 2008 ST291 is a centaur—a type of minor planet that is situated between the asteroid and comet categories. Centaurs are typically found in the outer Solar System, between the orbits of Jupiter and Neptune. They are characterized by unstable orbits and exhibit characteristics of both asteroids and comets.

(532037) 2013 FY27 is an asteroid that orbits the Sun. It was discovered on March 22, 2013, and is classified as a member of the main belt of asteroids between Mars and Jupiter. Like many asteroids, it has a specific designation assigned by the Minor Planet Center.

(533560) 2014 JM80 is a designation for a specific asteroid that is part of the main asteroid belt in our solar system. It was discovered in 2014 and is categorized as a member of the "Hilda" group of asteroids, which are known for their stable orbits that share similarities with Jupiter’s orbit. Asteroids like 2014 JM80 are typically small, and their characteristics can include size, orbit, and composition.

(543354) 2014 AN55 is classified as a near-Earth object (NEO) and is specifically categorized as an asteroid. It was discovered in January 2014 and is part of the Apollo group of asteroids, which are known for having orbits that cross Earth's orbit. The designation indicates the year of discovery (2014) and the specific number assigned to it by the Central Bureau for Astronomical Telegrams (CBAT) following its discovery.

(55565) 2002 AW197 is a minor planet, specifically an asteroidal body located in the asteroid belt. It was discovered on January 5, 2002. The designation indicates it is the 55,565th numbered asteroid in the sequence of discoveries.

(55637) 2002 UX25 is a way to refer to a specific trans-Neptunian object, which is a minor planet located in the Kuiper Belt. It was discovered in 2002 and is classified as a "distant" object in the Solar System, falling under the category of centaurs or scattered disk objects.

(556416) 2014 OE394 is a minor planet or asteroid located in the asteroid belt between Mars and Jupiter. It was discovered on July 19, 2014, and is classified as a member of the Apollo group of asteroids, which are known for their orbits crossing that of Earth.

(574372) 2010 JO179 is a trans-Neptunian object (TNO) located in the Kuiper Belt, which is a region of the solar system beyond the orbit of Neptune. It was discovered on May 12, 2010, and is classified as a detached object, meaning its orbit is significantly influenced by gravitational interactions with nearby planets, particularly Neptune.

(589683) 2010 RF43 is an asteroid that is part of the asteroid belt. It was discovered on September 5, 2010, and is classified under the category of near-Earth objects (NEOs). The designation "2010 RF43" indicates the year of its discovery (2010) and the order of its identification during that year (RF43).

(612533) 2002 XV93 is a designation for a trans-Neptunian object (TNO) located in the outer solar system, specifically in the Kuiper Belt. TNOs are celestial bodies that orbit the Sun beyond Neptune.

(612584) 2003 QX113 is a trans-Neptunian object located in the Kuiper Belt. It is classified as a centaur, which is a type of minor planet that orbits between the asteroid belt and the outer planets, specifically between Jupiter and Neptune. This designation indicates that it exhibits characteristics of both asteroids and comets.

(612911) 2004 XR190 is a trans-Neptunian object (TNO) that is part of the Kuiper Belt, a region of the solar system beyond the orbit of Neptune that is populated with many small icy bodies. Discovered in December 2004, it is classified as a centaur, which is a type of celestial object that has characteristics of both asteroids and comets.

(620074) 2013 AT183 is the designation for a near-Earth asteroid that was discovered on January 3, 2013. It is part of the Apollo group of asteroids, which are characterized by their orbits that cross Earth's orbit. The "620074" part is the numerical designation assigned to the asteroid, while "2013 AT183" is its provisional designation reflecting the year of discovery and the order in which it was discovered that year.

(78799) 2002 XW93 is a numerical designation for a specific asteroid that is part of the asteroid belt, which is located between the orbits of Mars and Jupiter. This asteroid was discovered in 2002 and received a provisional designation before being assigned a permanent number, 78799. Asteroids like 2002 XW93 are studied for various reasons, including their composition, size, and potential risk they might pose to Earth.

(84522) 2002 TC302 is a near-Earth asteroid discovered on October 1, 2002. It is classified as an Apollo-type asteroid, which means it has an orbit that crosses Earth's orbit. These types of asteroids can come quite close to Earth but are not necessarily on a collision course with our planet.

(84719) 2002 VR128 is a near-Earth object (NEO) and classified as an asteroid. It is part of the Apollo group of asteroids, which have orbits that bring them close to Earth's orbit. The designation "84719" is its official permanent number, while "2002 VR128" refers to the year of its discovery (2002) and its provisional designation.

(84922) 2003 VS2 is a near-Earth asteroid that was discovered in 2003. It is categorized as a member of the Apollo group of asteroids, which are characterized by their orbits crossing Earth's orbit. As a near-Earth object (NEO), it has the potential to come close to Earth at certain times, although it does not pose a significant threat.

(90568) 2004 GV9 is a minor planet or asteroid that belongs to the Main Belt, which is the region of space between the orbits of Mars and Jupiter where most asteroids are found. This particular asteroid was discovered in 2004. The designation "90568" refers to its number in the sequential list of asteroids, while "2004 GV9" indicates the year of its discovery (2004) and a specific code used for identification purposes.

10199 Chariklo is a centaur, which is a type of small celestial body that orbits the Sun between the orbits of Jupiter and Neptune. Discovered in 1997, Chariklo is notable for being one of the largest centaurs, with an estimated diameter of about 250 kilometers (around 155 miles).

10 Hygiea is the largest asteroid in the asteroid belt, located between the orbits of Mars and Jupiter. It is classified as a C-type (carbonaceous) asteroid, which means it has a composition that is rich in carbon, similar to that of comets.

120347 Salacia is a trans-Neptunian object located in the Kuiper Belt, which is a region of the solar system beyond the orbit of Neptune filled with icy bodies and dwarf planets. Discovered in 2003, Salacia is categorized as a "dwarf planet" candidate and is one of the larger objects of its kind. Its diameter is estimated to be around 800 kilometers (approximately 500 miles), though measurements may vary.

15760 Albion could refer to a specific address, location, or property. Without additional context, it's difficult to pinpoint exactly what you are referring to. If you can provide more details—such as the city, state, or type of establishment (residential, commercial, etc.

15810 Arawn is a small asteroid that is part of the asteroid belt in our solar system. Discovered on February 1, 1991, by the astronomer David C. Jewitt and his team, it is named after Arawn, a figure from Welsh mythology, who is associated with the otherworld.

174567 Varda is a trans-Neptunian object, specifically classified as a centaur. It was discovered on November 24, 2003, and is named after Varda, a character from J.R.R. Tolkien's Middle-earth legendarium. Varda is known as the queen of the stars and is associated with light and beauty. In terms of its physical characteristics, Varda has an estimated diameter of around 30 kilometers (19 miles).

19521 Chaos refers to a specific numerical value associated with a particular chaotic dynamical system or a mathematical phenomenon known as "chaos theory." However, without more context, it’s difficult to determine the precise significance of "19521 Chaos." In mathematics and physics, chaos theory studies systems that appear to be disordered or random, but are actually governed by underlying patterns and deterministic laws. These systems are sensitive to initial conditions, which is often illustrated with examples like the butterfly effect.

20000 Varuna is a trans-Neptunian object and a Centaur, which means it is located in the outer region of the Solar System, beyond the orbit of Neptune. It was discovered in 1978 and is named after Varuna, a deity in Hindu mythology associated with the sky and the oceans.

2006 QH181 is an asteroid that belongs to the Apollo group of near-Earth objects. Discovered on August 24, 2006, it is classified as a potentially hazardous asteroid due to its size and orbit, which brings it close to Earth's orbit. Asteroids like 2006 QH181 are of interest to astronomers and planetary scientists because studying them can provide insights into the early solar system and the formation of planetary bodies.

The term "2010 FX86" could refer to a few different things, depending on the context. However, it seems most likely that you are referring to the **2010 Nissan FX86**, a model of car produced by Nissan, known for its sporty characteristics and performance-oriented design. Alternatively, "FX86" could also refer to something specific within a different domain, like technology or gaming, but without additional context, it's hard to pinpoint.

2010 KZ39 is a near-Earth object (NEO) categorized as an asteroid. It was discovered in 2010 and is part of the Apollo group of asteroids, which are characterized by orbits that cross Earth's. Near-Earth objects like 2010 KZ39 are of interest to astronomers and planetary scientists because they can potentially pose a risk to Earth, and studying them can provide insights into the early solar system.

The designation "2010 TJ" refers to a specific model of the Jeep Wrangler, which was produced from 1996 to 2006. The "TJ" signifies the second generation of the Wrangler. This generation is known for its solid front and rear axles, improved handling, and an overall more refined design compared to its predecessor, the YJ.

The term "2010 VR11" could refer to various concepts depending on the context, but it is most commonly associated with a few different areas: 1. **Astronomy**: It might refer to an astronomical object or event, such as an asteroid or a comet, discovered or designated with this label. Astronomers often use nomenclature like this to identify and catalog celestial bodies.

2012 VP113 is a trans-Neptunian object (TNO) that was discovered in November 2012. It is classified as a candidate for a part of the scattered disk, a distant region of the Solar System populated by icy bodies. 2012 VP113 is of particular interest because its orbit suggests that it might be influenced by the gravitational pull of a massive, yet unseen object in the outer Solar System, often referred to as "Planet Nine.

2013 FQ28 is an asteroid that belongs to the Apollo group of near-Earth asteroids. It was discovered on March 19, 2013, and it has a diameter of approximately 45 to 100 meters. Like many near-Earth objects (NEOs), its orbit brings it close to Earth, and its characteristics are of interest to astronomers who study potential impact threats as well as resources for future space exploration.

2013 FS28 is a near-Earth object (NEO) categorized as an asteroid. It was discovered on March 30, 2013, and belongs to the Apollo group of asteroids, which are characterized by their orbits that cross that of Earth's. It has gained attention due to its close approaches to Earth. Asteroids like 2013 FS28 are monitored closely by astronomers to assess any potential impacts with Earth in the future.

2014 FC69 is classified as a small near-Earth object (NEO) and more specifically, it is an Apollo-type asteroid. It was discovered in March 2014 and orbits the Sun. Asteroids like 2014 FC69 are of interest to astronomers because they have orbits that bring them close to Earth and can offer insights into the history of our solar system.

2014 FC72 is a specific fluid used in various applications, primarily known for its properties as a coolant and dielectric fluid. It is a perfluorinated compound, which means it consists of carbon and fluorine atoms. FC72 is often utilized in electronics cooling, particularly in applications where traditional cooling methods (like water cooling) may not be suitable. FC72 offers several advantages, such as excellent thermal conductivity, high chemical stability, and low toxicity.

2014 FE72 is an asteroid that is classified as a near-Earth object (NEO). It was discovered in March 2014 and is part of the Apollo group of asteroids, which have orbits that cross the Earth's orbit. The designation "2014 FE72" indicates the year of its discovery (2014) and the order in which it was discovered in that year (72nd object).

2014 ST373 is an asteroid that belongs to the Asteroid Belt, which is between the orbits of Mars and Jupiter. It was discovered on September 27, 2014, by the Pan-STARRS 1 survey, based in Hawaii. This particular asteroid is classified as a member of the "Stype" or "Sub-Kentaur" group, and it has an orbital period of approximately 3.26 years.

2014 SV349 is a trans-Neptunian object (TNO) located in the outer regions of our Solar System. It was discovered on September 22, 2014, during the Pan-STARRS survey. This object is classified as a "distant" Kuiper Belt Object (KBO), which means it orbits the Sun at a significant distance beyond the orbit of Neptune.

2014 UZ224 is a trans-Neptunian object (TNO) that was discovered in 2014. It is part of the Kuiper Belt, a region of the solar system beyond the orbit of Neptune that contains many small icy bodies. 2014 UZ224 is classified as a scattered disk object, which means it has an elliptical and tilted orbit that can be influenced by the gravitational pull of the giant planets, particularly Neptune.

2015 BP519 is a trans-Neptunian object (TNO) located in the Kuiper Belt, which is a region of the solar system beyond the orbit of Neptune that contains many small icy bodies. Specifically, 2015 BP519 is classified as a detached object, meaning it has an orbit that is not significantly influenced by the gravitational pull of Neptune.

The 2015 GT350 is a high-performance variant of the Ford Mustang, specifically part of the Mustang lineup produced by Ford Motor Company. The GT350 was designed for enthusiasts who sought a track-ready car with enhanced performance features compared to the standard Mustang models. Key features of the 2015 Ford Mustang GT350 include: 1. **Engine**: The 2015 GT350 is equipped with a naturally aspirated 5.

2015 KH162 is classified as a near-Earth asteroid. It was discovered in 2015 during a survey of near-Earth objects. This asteroid is particularly interesting to astronomers and researchers due to its orbit, size, and potential implications for planetary defense. Though specific details about its size and exact orbital characteristics may vary, it generally falls within the category of asteroids that come close to Earth's orbit, and it is monitored for any potential future close approaches to our planet.

2017 FO161 is a trans-Neptunian object (TNO) located in the Kuiper Belt, which is a region of the solar system beyond the orbit of Neptune. It was designated as a centaur, which typically refers to icy bodies that exhibit characteristics of both asteroids and comets. This object is of interest to astronomers because it is part of a class of bodies that can provide insights into the early solar system's formation and evolution.

2017 OF69 is an asteroid that was discovered in 2017. It belongs to the Apollo group of near-Earth objects and is categorized as a potentially hazardous asteroid due to its size and close approaches to Earth's orbit. The designation "2017 OF69" is based on the date of its discovery (July 19, 2017) and follows the naming convention used by astronomers for new celestial objects.