3428 Roberts, the Glossary
3428 Roberts (''prov. designation'') is a background asteroid from the central regions of the asteroid belt, approximately in diameter.[1]
Table of Contents
37 relations: Absolute magnitude, Akari (satellite), Albedo, Asteroid belt, Asteroid family, Asteroid spectral types, Astronomical unit, C-type asteroid, Coronagraph, Degree (angle), Ecliptic, Ecliptic coordinate system, Goethe Link Observatory, Indiana Asteroid Program, Indiana University Bloomington, Jet Propulsion Laboratory, Julian day, Julian year (astronomy), Kirkwood gap, Light curve, List of observatory codes, Magnitude (astronomy), Minor planet, Minor Planet Center, National Center for Atmospheric Research, Observation arc, Orbital eccentricity, Orbital inclination, Photometry (astronomy), Poles of astronomical bodies, Proper orbital elements, Provisional designation in astronomy, Rotation period (astronomy), S-type asteroid, Semi-major and semi-minor axes, Walter Orr Roberts, Wide-field Infrared Survey Explorer.
- Astronomical objects discovered in 1952
Absolute magnitude
In astronomy, absolute magnitude is a measure of the luminosity of a celestial object on an inverse logarithmic astronomical magnitude scale.
See 3428 Roberts and Absolute magnitude
Akari (satellite)
AKARI (ASTRO-F) was an infrared astronomy satellite developed by Japan Aerospace Exploration Agency, in cooperation with institutes of Europe and Korea.
See 3428 Roberts and Akari (satellite)
Albedo
Albedo is the fraction of sunlight that is diffusely reflected by a body.
Asteroid belt
The asteroid belt is a torus-shaped region in the Solar System, centered on the Sun and roughly spanning the space between the orbits of the planets Jupiter and Mars.
See 3428 Roberts and Asteroid belt
Asteroid family
An asteroid family is a population of asteroids that share similar proper orbital elements, such as semimajor axis, eccentricity, and orbital inclination.
See 3428 Roberts and Asteroid family
Asteroid spectral types
An asteroid spectral type is assigned to asteroids based on their reflectance spectrum, color, and sometimes albedo.
See 3428 Roberts and Asteroid spectral types
Astronomical unit
The astronomical unit (symbol: au, or AU) is a unit of length defined to be exactly equal to.
See 3428 Roberts and Astronomical unit
C-type asteroid
C-type (carbonaceous) asteroids are the most common variety, forming around 75% of known asteroids.
See 3428 Roberts and C-type asteroid
Coronagraph
A coronagraph is a telescopic attachment designed to block out the direct light from a star or other bright object so that nearby objects – which otherwise would be hidden in the object's bright glare – can be resolved.
See 3428 Roberts and Coronagraph
Degree (angle)
A degree (in full, a degree of arc, arc degree, or arcdegree), usually denoted by ° (the degree symbol), is a measurement of a plane angle in which one full rotation is 360 degrees.
See 3428 Roberts and Degree (angle)
Ecliptic
The ecliptic or ecliptic plane is the orbital plane of Earth around the Sun.
Ecliptic coordinate system
In astronomy, the ecliptic coordinate system is a celestial coordinate system commonly used for representing the apparent positions, orbits, and pole orientations of Solar System objects.
See 3428 Roberts and Ecliptic coordinate system
Goethe Link Observatory
The Goethe Link Observatory, observatory code 760, is an astronomical observatory near Brooklyn, Indiana, United States. 3428 Roberts and Goethe Link Observatory are Discoveries by Indiana University (Indiana Asteroid Program).
See 3428 Roberts and Goethe Link Observatory
Indiana Asteroid Program
The Indiana Asteroid Program was a photographic astronomical survey of asteroids during 1949–1967, at the U.S. Goethe Link Observatory near Brooklyn, Indiana. 3428 Roberts and Indiana Asteroid Program are Discoveries by Indiana University (Indiana Asteroid Program).
See 3428 Roberts and Indiana Asteroid Program
Indiana University Bloomington
Indiana University Bloomington (IU Bloomington, Indiana University, IU, or simply Indiana) is a public research university in Bloomington, Indiana.
See 3428 Roberts and Indiana University Bloomington
Jet Propulsion Laboratory
Jet Propulsion Laboratory (JPL) is a Federally Funded Research and Development Center (FFRDC) in La Cañada Flintridge, California, Crescenta Valley, United States.
See 3428 Roberts and Jet Propulsion Laboratory
Julian day
The Julian day is the continuous count of days since the beginning of the Julian period, and is used primarily by astronomers, and in software for easily calculating elapsed days between two events (e.g. food production date and sell by date).
See 3428 Roberts and Julian day
Julian year (astronomy)
In astronomy, a Julian year (symbol: a or aj) is a unit of measurement of time defined as exactly 365.25 days of SI seconds each.
See 3428 Roberts and Julian year (astronomy)
Kirkwood gap
A Kirkwood gap is a gap or dip in the distribution of the semi-major axes (or equivalently of the orbital periods) of the orbits of main-belt asteroids.
See 3428 Roberts and Kirkwood gap
Light curve
In astronomy, a light curve is a graph of the light intensity of a celestial object or region as a function of time, typically with the magnitude of light received on the y-axis and with time on the x-axis.
See 3428 Roberts and Light curve
List of observatory codes
This is a list of observatory codes (IAU codes or MPC codes) published by the Minor Planet Center.
See 3428 Roberts and List of observatory codes
Magnitude (astronomy)
In astronomy, magnitude is measure of the brightness of an object, usually in a defined passband.
See 3428 Roberts and Magnitude (astronomy)
Minor planet
According to the International Astronomical Union (IAU), a minor planet is an astronomical object in direct orbit around the Sun that is exclusively classified as neither a planet nor a comet.
See 3428 Roberts and Minor planet
Minor Planet Center
The Minor Planet Center (MPC) is the official body for observing and reporting on minor planets under the auspices of the International Astronomical Union (IAU).
See 3428 Roberts and Minor Planet Center
National Center for Atmospheric Research
The US National Center for Atmospheric Research (NCAR) is a US federally funded research and development center (FFRDC) managed by the nonprofit University Corporation for Atmospheric Research (UCAR) and funded by the National Science Foundation (NSF).
See 3428 Roberts and National Center for Atmospheric Research
Observation arc
In observational astronomy, the observation arc (or arc length) of a Solar System body is the time period between its earliest and latest observations, used for tracing the body's path.
See 3428 Roberts and Observation arc
Orbital eccentricity
In astrodynamics, the orbital eccentricity of an astronomical object is a dimensionless parameter that determines the amount by which its orbit around another body deviates from a perfect circle.
See 3428 Roberts and Orbital eccentricity
Orbital inclination
Orbital inclination measures the tilt of an object's orbit around a celestial body.
See 3428 Roberts and Orbital inclination
Photometry (astronomy)
In astronomy, photometry, from Greek photo- ("light") and -metry ("measure"), is a technique used in astronomy that is concerned with measuring the flux or intensity of light radiated by astronomical objects.
See 3428 Roberts and Photometry (astronomy)
Poles of astronomical bodies
The poles of astronomical bodies are determined based on their axis of rotation in relation to the celestial poles of the celestial sphere.
See 3428 Roberts and Poles of astronomical bodies
Proper orbital elements
The proper orbital elements or proper elements of an orbit are constants of motion of an object in space that remain practically unchanged over an astronomically long timescale.
See 3428 Roberts and Proper orbital elements
Provisional designation in astronomy
Provisional designation in astronomy is the naming convention applied to astronomical objects immediately following their discovery.
See 3428 Roberts and Provisional designation in astronomy
Rotation period (astronomy)
In astronomy, the rotation period or spin period of a celestial object (e.g., star, planet, moon, asteroid) has two definitions.
See 3428 Roberts and Rotation period (astronomy)
S-type asteroid
S-type asteroids are asteroids with a spectral type that is indicative of a siliceous (i.e. stony) mineralogical composition, hence the name.
See 3428 Roberts and S-type asteroid
Semi-major and semi-minor axes
In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the two most widely separated points of the perimeter.
See 3428 Roberts and Semi-major and semi-minor axes
Walter Orr Roberts
Walter Orr Roberts (August 20, 1915 – March 12, 1990) was an American astronomer and atmospheric physicist, as well as an educator, philanthropist, and builder.
See 3428 Roberts and Walter Orr Roberts
Wide-field Infrared Survey Explorer
Wide-field Infrared Survey Explorer (WISE, observatory code C51, Explorer 92 and MIDEX-6) is a NASA infrared astronomy space telescope in the Explorers Program launched in December 2009.
See 3428 Roberts and Wide-field Infrared Survey Explorer
See also
Astronomical objects discovered in 1952
- 1617 Alschmitt
- 1622 Chacornac
- 1761 Edmondson
- 1788 Kiess
- 1801 Titicaca
- 1824 Haworth
- 1954 Kukarkin
- 1987 Kaplan
- 1988 Delores
- 2023 Asaph
- 2024 McLaughlin
- 2244 Tesla
- 3428 Roberts
- Simeis 147