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Possible Answers:
UMP.
Last seen on: Eugene Sheffer – King Feature Syndicate Crossword – Nov 24 2022
Random information on the term “Ballpark figure”:
In physics and mathematics, an ansatz (/ˈænsæts/; German: [ˈʔanzats], meaning: “initial placement of a tool at a work piece”, plural Ansätze /ˈænsɛtsə/; German: [ˈʔanzɛtsə]) is an educated guess or an additional assumption made to help solve a problem, and which may later be verified to be part of the solution by its results.
An ansatz is the establishment of the starting equation(s), the theorem(s), or the value(s) describing a mathematical or physical problem or solution. It typically provides an initial estimate or framework to the solution of a mathematical problem, and can also take into consideration the boundary conditions (in fact, an ansatz is sometimes thought of as a “trial answer” and an important technique in solving differential equations).
After an ansatz, which constitutes nothing more than an assumption, has been established, the equations are solved more precisely for the general function of interest, which then constitutes a confirmation of the assumption. In essence, an ansatz makes assumptions about the form of the solution to a problem so as to make the solution easier to find.
Random information on the term “UMP”:
During 1944, Walter Baade categorized groups of stars within the Milky Way into stellar populations.In the abstract of the article by Baade, he recognizes that Jan Oort originally conceived this type of classification in 1926:
The two types of stellar populations had been recognized among the stars of our own galaxy by Oort as early as 1926.
Baade noticed that bluer stars were strongly associated with the spiral arms, and yellow stars dominated near the central galactic bulge and within globular star clusters. Two main divisions were defined as
with another newer, hypothetical division called
added in 1978; they are often simply abbreviated as Pop. I, Pop. II, and Pop. III.
Among the population types, significant differences were found with their individual observed stellar spectra. These were later shown to be very important and were possibly related to star formation, observed kinematics, stellar age, and even galaxy evolution in both spiral and elliptical galaxies. These three simple population classes usefully divided stars by their chemical composition or metallicity.