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Detection of Black Holes01:10

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Although black holes were theoretically postulated in the 1920s, they remained outside the domain of observational astronomy until the 1970s.
Their closest cousins are neutron stars, which are composed almost entirely of neutrons packed against each other, making them extremely dense. A neutron star has the same mass as the Sun but its diameter is only a few kilometers. Therefore, the escape velocity from their surface is close to the speed of light.
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Reduced Mass Coordinates: Isolated Two-body Problem01:12

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In classical mechanics, the two-body problem is one of the fundamental problems describing the motion of two interacting bodies under gravity or any other central force. When considering the motion of two bodies, one of the most important concepts is the reduced mass coordinates, a quantity that allows the two-body problem to be solved like a single-body problem. In these circumstances, it is assumed that a single body with reduced mass revolves around another body fixed in a position with an...
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Nomenclature of Aryl and Heterocyclic Amines01:10

Nomenclature of Aryl and Heterocyclic Amines

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The simplest aromatic amine is phenylamine, which contains an –NH2 functionality directly attached to an aromatic ring. The name aniline is designated for this skeleton. As shown in Figure 1, the common names of the functionalized anilines involve prefixes ortho-, meta-, and para- to indicate the substitution position. Different functionalized aniline derivatives also have notable trivial names.
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Criteria for Aromaticity and the Hückel 4n + 2 Rule01:20

Criteria for Aromaticity and the Hückel 4n + 2 Rule

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Like benzene, cyclobutadiene and cyclooctatetraene are cyclic compounds with alternate single and double bonds. However, their chemical behavior differs from benzene, as they are unstable and not aromatic. So, what are the structural characteristics of unsaturated compounds categorized as aromatic?  
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Types of Hypothesis Testing01:11

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There are three types of hypothesis tests: right-tailed, left-tailed, and two-tailed.
When the null and alternative hypotheses are stated, it is observed that the null hypothesis is a neutral statement against which the alternative hypothesis is tested. The alternative hypothesis is a claim that instead has a certain direction. If the null hypothesis claims that p = 0.5, the alternative hypothesis would be an opposing statement to this and can be put either p > 0.5, p < 0.5, or p...
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Preparation of 1&deg; Amines: Hofmann and Curtius Rearrangement Overview01:07

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In the presence of an aqueous base and a halogen, primary amides can lose the carbonyl (as carbon dioxide) and undergo rearrangement to form primary amines. This reaction, called the Hofmann rearrangement, can produce primary amines (aryl and alkyl) in high yields without contamination by secondary and tertiary amines.
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ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2014 DECEMBER - 2015 MARCH.

The Minor planet bulletin·2020
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ASTEROID LIGHTCURVE ANALYSIS AT CS3-PALMER DIVIDE STATION: 2013 SEPTEMBER-DECEMBER.

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LIGHTCURVE PHOTOMETRY OPPORTUNITIES: 2015 JULY-SEPTEMBER.

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Updated: Dec 20, 2025

Scattering And Absorption of Light in Planetary Regoliths
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Scattering And Absorption of Light in Planetary Regoliths

Published on: July 1, 2019

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ONE NEW AND ONE SUSPECTED HUNGARIA BINARY ASTEROID.

Brian D Warner1, Robert D Stephens2

  • 1Center for Solar System Studies - Palmer Divide Station, 17995 Bakers Farm Rd., Colorado Springs, CO 80908 USA.

The Minor Planet Bulletin
|May 28, 2020
PubMed
Summary
This summary is machine-generated.

Astronomers discovered a new binary asteroid, 4765 Wasserburg, which is part of an asteroid pair. Another Hungaria asteroid, 1994 WB1, shows potential but inconclusive evidence of being a binary system.

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Area of Science:

  • Asteroid Science
  • Photometry
  • Binary Systems

Background:

  • Hungaria asteroids are a population of small Solar System bodies located beyond the main asteroid belt.
  • Asteroid pairs are groups of asteroids thought to originate from a single parent body.
  • Understanding asteroid binaries provides insights into their formation and evolution.

Purpose of the Study:

  • To conduct CCD photometry observations of two Hungaria asteroids.
  • To investigate the potential binary nature of asteroids 4765 Wasserburg and 1994 WB1.
  • To determine the rotational and orbital periods of any discovered satellites.

Main Methods:

  • Utilized CCD photometry for observational data acquisition.
  • Analyzed light curves to identify periodic variations indicative of rotation and orbital motion.
  • Applied data analysis techniques to determine primary and satellite periods.

Main Results:

  • Discovered 4765 Wasserburg as a previously unknown binary asteroid with a primary period of 3.6231 ± 0.0005 hours and a satellite orbital period of 15.97 ± 0.02 hours.
  • Identified 4765 Wasserburg as a member of an asteroid pair, adding significance to the discovery.
  • Observed 1994 WB1 with tentative evidence for a satellite (orbital period 15.94 h) and a primary rotation period of 2.462 h in 2013 data, but conflicting results from 2008 data.

Conclusions:

  • 4765 Wasserburg is confirmed as a binary asteroid and a member of an asteroid pair.
  • The binary status of 1994 WB1 remains uncertain, classifying it as an 'asteroid of interest'.
  • Further observations are needed to confirm the binary nature of 1994 WB1.