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Dawn Dictionary
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Achondrite - A meteorite consisting of igneous
minerals and no chondrules, very similar to terrestrial igneous rocks
Albedo - The ratio of the amount of light
reflected from a surface to the amount of incident light
Aperture - The effective diameter of the
primary mirror or lens of a telescope
Aphelion - The point in a planetary orbit
that is at the greatest distance from the Sun
Apparent Magnitude - The
brightness of a star as it appears to the eye or to the telescope,
as measured in units of magnitude—the brighter the star,
the smaller the apparent magnitude.
Asteroid - (also called a “minor planet”) A small solar system object in orbit around the
sun composed mostly of rock. Many of these objects orbit the
sun between Mars and Jupiter. Their size can range anywhere
from 100 meters in diameter to almost 1000 kilometers.
Principal asteroids – Ceres, Pallas, Juno and Vesta
C-type asteroids are carbon-rich, very dark, reflect on 3%-9%
of sunlight.
S-type asteroids are comprised of metallic nickel-iron mixed
with iron- and magnesium-silicates.
V-type asteroids contain more pyroxene than S-type asteroids.
Asteroid belt - A region of space lying between
Mars (1.5 AU) and Jupiter (5.2 AU), where the great majority
of the asteroids are found
Astronomical Unit (AU) -
The mean distance between the Earth and the Sun: 149,598,500km; the preferred unit for distances within the Solar System
Axis of rotation - The theoretical straight
line through a celestial body, around which it rotates
Bode’s Law - This law describes a mathematical
method for calculating planetary distances which states that
the distance to the nth planet is 0.4 + (0.3)n Astronomical
Units. Bodes law works surprisingly well out to Uranus.
Brightness magnitude - The
apparent brightness of a star is called the apparent magnitude
and that is what is measured by a telescope: how much energy
the star puts into the telescope's collecting area per
second.
Brightness - Refers to the
amount of light coming from an object
Canon law - The body of ecclesiastical law
by which a Christian church is governed.
Celestial body - A solid object found in
space; in the heavens
Celestial Police - A group of astronomers
looking for Kepler’s missing planet between Jupiter
and Mars
Ceres - Largest of the known asteroids, and
the first to be discovered (by Piazzi in 1801)
Chondrite - A meteorite containing chondrules,
which are small, spherical silicate objects on the order of
a millimeter in size that formed in the solar nebula before
the asteroids were formed
Chondrules -A crystallized sphere of rocky material found in chondrite meteorites. Named after the Greek for seeds, they are essentially tiny igneous rocks that formed in the solar nebula.
Circumscribe - To draw a line around; to
encircle
Classical planets - Mercury, Venus, Mars,
Jupiter and Saturn are known as “the classical planets
Collodian - A viscous solution used in coating
photographic films; the wet collodion process produced plates
that had a much higher sensitivity than was previously available
Comet - A small solar system object orbiting
the Sun consisting of ice, dust and gas that form a coma and
sometimes a visible tail whenever they orbit close to the
Sun
Comet debris - Clumps of dust, ice and rocky
material that are released from comets as they approach the
sun
Concave - Hollowed or rounded inward like the inside of a bowl
Concave lens - A lens whose interior surface
in hollowed or curved inward, away from the viewpoint, making
the interior of the lens thinner than the outer edges
Convex - Curved or rounded outward like the exterior of a sphere or circle
Convex lens - A lens whose interior surface
is curved outward, toward viewpoint, making the interior of
the lens thicker than the outer edges
Convex-profile inversion -
A modeling technique for producing a three-dimensional shape
from a two-dimension convex profile
Copernican system - A heliocentric
model of the universe; the hypothesis that the earth and the
other planets orbit the sun
Coulomb - A measure of the amount of electric
current, being the quantity transferred in one second by a
current of one ampere. 1 coulomb = 1 A s.
Crust - The outer part of a planet, moon, or asteroid composed essentially of crystalline rocks—generally the crustal composition is different from the bulk composition of the planet (adapted from Merriam-Webster.com).
Cyclic - Moving or recurring in cycles or
periods
Dawn Discovery Mission - The ninth of NASA’s
Discovery Program missions will investigate two of the largest protoplanets in the main asteroid belt, Vesta and Ceres.
Declination (DEC) - Declination is measured in degrees, and refers to how far above the imaginary"celestial equator" an object is (like latitude on the Earth).
Ecliptic - The mean plane of the Earth's
orbit around the Sun
Elastic Collision - A collision between two
particles which conserves the total kinetic energy and momentum
of the system
Electromagnetic Radiation - "Waves"
of electrical and magnetic "disturbance", radiated
as visible light, radio waves, or any other manifestation
of the electromagnetic spectrum
Electron Volt (eV) - A unit of energy used
to indicate the energy of a charged particle. 1 eV is the
energy gained when an electron is accelerated by a potential
of one volt. 1 electron volt = 1.6 x 10-12 ergs
Elliptical - Shaped like an ellipse, a plane
curve in which the sum of the distances of each point along
its periphery from two points - its "foci" - are
equal
Emission spectrum - A spectrum of energy released from a source, usually in the form of electromagnetic radiation
Emit (also see Light) - To send forth or
to send out electromagnetic radiation
Emulsion - A suspension of sensitive silver
salt in a viscous medium, used for coating plates or films
Ephemeris (Ephemerides; plural) - A table that gives the positions of objects in the sky at various times
Epicycle - Circular orbit of a body round
a point that is itself in a circular orbit round a parent
body—such a system was formulated to explain some planetary
orbits in the Solar System before they were known to be elliptical
Epithermal Neutron - A neutron that has undergone energy loss due to scattering collisions, but is not in thermalequilibrium with the regolith (E = ~0.3 eV to ~600 keV)
Evolutionary path - In astronomy, the theory
that more complex and varied bodies develop from simpler ones
Exposure - To lay open to the influences
of climate or other external forces
Fast Neutron—A neutron ejected at high kinetic energy in a nuclear reaction (E = ~103 eV to 6 MeV)
Fusion Crust -Fusion crust is the outer covering that a meteorite has acquired as a result of the melting of its surface layer as it passes through the atmosphere. The compression of the Earth's atmosphere heats the surface of the meteoroid to its melting point. Most of the melted material is ablated (removed): what remains resolidifies as the fusion crust. The thickness of these crusts can range from less than one millimeter up to several millimeters. Typically, the leading side of the meteoroid will have a thinner crust than the trailing side. Fusion crusts can be light or dark in color depending on the amount of iron in the meteorite minerals.
Gamma rays - Very energetic EMR photons with energies between 1 MeV–¬10 GeV
Inelastic collision; a collision between two particles in which part of their kinetic energy is transformed into another form of energy (gamma rays)—the total amount of energy remains the same
Geocentric - Having the Earth at the center.
Heliocentric - Having the Sun at the center.
Hubble Space Telescope (HST) - NASA launched
the Hubble Space Telescope in 1990. It orbits around the Earth
every 97 minutes about 600 kilometers above the Earth, above
the distorting effects of the atmosphere. Hubble’s instruments
include cameras and spectrographs, using mirrors to focus
and magnify light.
Igneous - In the case of meteorites the term
“igneous” refers to a rock formed by solidification
of a molten rock or metal. Examples of igneous meteorites
include the iron meteorites, and basaltic meteorites (Howardites
and Eucrites) thought to come from the asteroid Vesta.
Impact basin (also impact crater) -
A circular depression on the surface of a planet,
moon, asteroid, or other celestial body. Craters are typically
caused by meteorite impacts. In the center of craters on Earth
a crater lake often accumulates, and in craters formed by
meteorites a central island (caused by rebounding crustal
rock after the impact) is usually a prominent feature in the
lake.
Inclination - In astronomy,
the angle between one plane and another. The (equatorial)
inclination of a planet is the angle between the plane of
its equator and that of its orbit. The inclination of the
orbit of a planet in the Solar System other than Earth is
the angle between the plane of that orbit and the ecliptic.
Inelastic Collision - A reaction involving
a change in the kinetic energy of the system, as in ionization,
excitation, or capture; or a process which changes the energy
level of the system.
Ion - A charged particle consisting of an
atom, or group of atoms, that has either lost or gained electrons.
Ionization - Loss or gain by an atom of one
or more electrons, by which process the atom becomes an ion
and instead of being neutral, has a charge: positive if it
has lost an electron, negative if it has gained one.
Ion jet propulsion - Any device in which
an ionized propellant stream is accelerated by interactions
of external and internal magnetic fields with electric currents
driven through the stream, thereby imparting thrust to a spacecraft
on which is it mounted.
IPS - Acronymn for Ion Propulsion System. (See ion jet propulsion above.)
Inscribe - To draw on figure within another
so as to have as many incidences as possible.
Light - The radiant energy that enables organs
of vision to perform the function of sight; more accurately
called luminous energy. (see also Electromagnetic Radiation).
Visible - Electromagnetic radiation with wavelengths
of or close to those detectable by the eye.
Emitted - An emanation of light from a light-giving
body, such as the Sun
Infrared - Electromagnetic radiation with wavelengths
too long to be detectable by the eye.
Reflected - Light that is bent back from an
object.
Light Curve - A plot of the amount of light
detected from an object (i.e. the apparent magnitude) as a
function of time. Light curves provide evidence of eclipsing
binaries, variable stars, and track the progress of nova and
supernova explosions.
Magnification - The effect of an optical
system on the apparent angular size of an object—an increase
in angular size occurs if the magnification factor is greater
than 1
Magma - Molten rock material
within a melted planet or asteroid from which igneous rock
results by cooling (adapted from Merriam-Webster.com)
Magnitude - An astronomical unit of brightness—originally corresponding to the eye's response to starlight—the magnitude system is logarithmic, with 5 magnitudes corresponding
to a factor of 100 in brightness. To further confuse things
larger magnitudes correspond to fainter objects.
Mantle - The part of a planet or asteroid
between the crust and the core
Metamorphic - In the case of meteorites the
term “metamorphic” refers to a rock containing
minerals that have recrystallized due to heat in a parent
body asteroid.
Meteor - The flash and trail of light that
we see in the night sky caused by a meteoroid
passing through the atmosphere
Meteorite - An object that passes through the Earth's
atmosphere and is too large to be destroyed before it hits the surface—meteorites may in some way be
connected with asteroids.
Meteoroid - An interplanetary piece of matter larger than dust, but smaller than an asteroid or dwarf planet
Minor planet - (see Asteroid)
Nebulosity - A hazy, cloudy, or misty characteristic
of matter in a gaseous or finely divided state
Neutron capture - A process in which a neutron is absorbed by a nucleus to produce an excited nucleus that transitions to ground state by emission of one or more gamma rays
Observatory - A building equipped for observation
of natural phenomena, as in meteorology or astronomy
Opposition - A configuration of the Sun,
Earth and a planet or asteroid in which the apparent geocentric
longitude of the planet or asteroid differs by 180 degrees
from the apparent geocentric longitude of the Sun
Orbit - The path in space followed by a celestial
body
Patent - A writing securing to an inventor
the exclusive right to make, use, and vend his invention
Period of revolution - The interval of time
required to complete one revolution in an orbit
Photochemical - Materials in which the absorption
of light leads to a chemical reaction
Photographic plate - The flat surface on
which the emulsion containing light-sensitive chemicals is
placed; after exposing to light, the emulsion forms a negative
of the object photographed.
Photometry - The measurement of light. Specifically
refers to the procedure of highly accurate measuring of the
apparent magnitudes of astronomical objects. In general, astronomers
measure only a portion of the wavelength spectrum when they
do photometry. Different types of photometry are defined by
the portion of the wavelength that they examine. Differential
photometry, or "UBV Photometry", measures the light
within three standard regions defined by filters. These are
Ultraviolet, Blue and Visual (hence UBV). There are many different
photometry systems and standards.
Photomultiplier tube - A vacuum encapsulated
photocathode from which electrons are ejected by the photoelectric
effect followed by multiple cathodes from which many additional
electrons are emitted in a cascade—when finally collected,
the original single electron may have generated a pulse of
over one million electrons; first used in astronomy in the
early 1950s in a process known as differential photometry
Planetary orbit - The path in space followed
by a planet
Planet - An object that
formed in the disk surrounding a star—to be called a planet,
an object must be more massive than Pluto (1/500 the Earth's
mass) and less massive than ten times Jupiter's mass
Planetoids - (see Asteroids)
Power - The magnifying capacity of a lens,
expressed as the number of times it multiplies the diameter
of an object
Protoplanets - Early stage in the formation
of planets according to the theory by which planetary systems
evolve through the condensation of gas clouds surrounding
a young star
Ptolemaic system or Ptolemaic Model of the Universe
- A geocentric model in which the Earth remained
stationary as the other planets the Sun, the Moon and the
stars orbited it on their spheres— was eventually replaced
by the Copernican model
Pyroxene - A common metasilicate, chiefly
of calcium and magnesium, usually in short, thick, prismatic
crystals; next to feldspar the most frequent constituent of
igneous rocks
Reciprocity failure - The tendency for film
emulsions to suffer a rapid fall-off in their ability to gather
data after an initial surge of light
Reflection - The return of light or sound waves from a surface
Reflecting telescope - Telescope
that uses mirrors to magnify and focus an image onto an eyepiece
Refraction - The bending of light as it passes from one medium to another
Refracting Telescope - Telescope
that uses lenses to magnify and focus an image onto an eyepiece
Regmaglypts -Thumbprint-like indentations that are caused by parts of the meteorite melting and being sloughed off in its descent through Earth’s atmosphere
Regolith - The layer of rocky or icy debris and dust made by meteoritic impact that forms the uppermost surface of planets, moons and asteroids
Retina - The sensitive membrane of specialized
cells in the eye which receives the image formed by the lens
and is connected with the brain by the optic nerve
Right ascension (RA) - Right ascension is measured in hours of time. It is similar to longitude on the Earth. Astronomers have chosen the Vernal Equinox to define the starting point for the measurement of right ascension. The Vernal Equinox is the point where the Sun appears to cross the Celestial Equator at the beginning of spring. It is therefore one of the two points where the Ecliptic intersects the Celestial Equator.
Rotation - Of a single body
in space, spinning on an axis; of a planetary system, rotation
is generally planar in relation to the parent star
Rotation axis - (see Axis of rotation)
Scintillator - A phosphor-containing radiation detector that absorbs a photon or ionizing particle
Semiconductor - A substance or material, typically crystalline, that conducts electricity better than an insulator, but not as well as a conductor, because it allows current to flow only under certain condictions—common semiconductors are silicon, germanium, gallium, and arsenide
Semi-major axis - Half the length of the
major axis of an ellipse; a standard element used to describe
an elliptical orbit
Sensitivity - The capacity to respond to
stimulation
Serendipity - Finding without seeking
Silver bromide - A yellowish,
odorless powder that darkens on exposure to light; is used
in photographic colloids
Silver iodide - A light yellow, odorless
power that slowly darkens by light; is used in photographic
colloids
Solar Nebula - The cloud of gas and dust that condensed and accumulated to form the Solar System.
Solar System - The complex of planets, asteroids,
comets, debris gravitationally bound to the Sun and including
the particles and fields emitted from the sun and interacting
with its components
Spacecraft - A vehicle that can travel in
outer space
Speckle interferometry - A process that uses
ground-based telescopes and computer technology to make highly
detailed or high-resolution images of asteroids by clustering
together loads of tiny “specks” to form a clearer
picture
Spectra - The energies of
the photons emitted or absorbed by one atom are different
from those of all other atoms. The photon energies are directly
related to their frequencies, which set their colors in the
spectrum, so by observing the colors of the photons, it is
possible to determine which atoms are being observed. This
can be done in a laboratory, and it can also be done with
the light reaching us from stars, near or distant, which enables
us to identify the atoms that stars are made of.
Spectroscope - An optical
instrument used for producing and observing spectra of light
or other radiation
Spectroscopy - Spectroscopy is the study
of the detailed features of a star's spectrum, done by measuring
the intensity of the star's light at as many different wavelengths
as possible. The resulting spectrum of light allows one to
locate the emission and absorption lines, determine the composition
of the star, its doppler shift, its spectral type, and its
luminosity class.
Telescope - An optical instrument for making
distant objects appear closer or larger
Theory - In science a theory is a verified
hypothesis applicable to many related phenomena.
Thermal Neutron - A neutron produced by fission and slowed by a moderator, so that it is in thermal equilibrium with its surrounding medium; (E< ~0.3 eV)
Titius-Bode Law - The Titius-Bode
Rule was first devised in 1772 and comprised the series 0
+ 4/10, 3 + 4/10, 6 + 4/10, 12 + 4/10, 24 + 4/10 and so on.
It was found to describe fairly accurately the distance in
astronomical units of the then known planets from the Sun.
Vesta - The brightest of all minor planets,
at times approaching naked-eye visibility, was discovered
by Olbers in 1807.
Volatiles - Substances that change into a vapor at relatively low temperatures | | |