1) Astronomy is the scientific study of celestial objects like stars, planets, comets, and galaxies.
2) There is evidence that the universe began in a massive explosion called the Big Bang around 13 billion years ago, and has been expanding ever since.
3) Key evidence for the Big Bang theory includes the Doppler effect, which shows that distant galaxies are moving away from us, and the discovery of cosmic microwave background radiation filling the universe.
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Please check all question included in this tutorial below
SCI 151 Final Exam
1. The Sun, Moon, and the Planets follow an imaginary line through the sky called the ecliptic. The reason this occurs is that
2. Another name for Sirius is the ____Brightest (Dog) Star________. This star is located __8.6_____ Light years from Earth
3. Select the best answer. When it is Dec 21 on Earth.
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Please check all question included in this tutorial below
SCI 151 Final Exam
1. The Sun, Moon, and the Planets follow an imaginary line through the sky called the ecliptic. The reason this occurs is that
2. Another name for Sirius is the ____Brightest (Dog) Star________. This star is located __8.6_____ Light years from Earth
3. Select the best answer. When it is Dec 21 on Earth.
For more course tutorials visit
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Please check all question included in this tutorial below
SCI 151 Final Exam
1. The Sun, Moon, and the Planets follow an imaginary line through the sky called the ecliptic. The reason this occurs is that
2. Another name for Sirius is the ____Brightest (Dog) Star________. This star is located __8.6_____ Light years from Earth
3. Select the best answer. When it is Dec 21 on Earth.
4. When the Moon lies directly between the Earth and the Sun the Phase of the Moon at that time is called ____ _____ and it is possible at that time to have an event called a _____ _________
This is the HW assigned for Honors Earth Science, Period 1 and 3. It is due on Monday 22, (the Monday we come back from break) It will be graded and count as three HWs.
For more course tutorials visit
uophelp.com is now newtonhelp.com
www.newtonhelp.com
Please check all question included in this tutorial below
SCI 151 Final Exam
1. The Sun, Moon, and the Planets follow an imaginary line through the sky called the ecliptic. The reason this occurs is that
2. Another name for Sirius is the ____Brightest (Dog) Star________. This star is located __8.6_____ Light years from Earth
3. Select the best answer. When it is Dec 21 on Earth.
4. When the Moon lies directly between the Earth and the Sun the Phase of the Moon at that time is called ____ _____ and it is possible at that time to have an event called a _____ _________
This is the HW assigned for Honors Earth Science, Period 1 and 3. It is due on Monday 22, (the Monday we come back from break) It will be graded and count as three HWs.
UiPath Test Automation using UiPath Test Suite series, part 4DianaGray10
Welcome to UiPath Test Automation using UiPath Test Suite series part 4. In this session, we will cover Test Manager overview along with SAP heatmap.
The UiPath Test Manager overview with SAP heatmap webinar offers a concise yet comprehensive exploration of the role of a Test Manager within SAP environments, coupled with the utilization of heatmaps for effective testing strategies.
Participants will gain insights into the responsibilities, challenges, and best practices associated with test management in SAP projects. Additionally, the webinar delves into the significance of heatmaps as a visual aid for identifying testing priorities, areas of risk, and resource allocation within SAP landscapes. Through this session, attendees can expect to enhance their understanding of test management principles while learning practical approaches to optimize testing processes in SAP environments using heatmap visualization techniques
What will you get from this session?
1. Insights into SAP testing best practices
2. Heatmap utilization for testing
3. Optimization of testing processes
4. Demo
Topics covered:
Execution from the test manager
Orchestrator execution result
Defect reporting
SAP heatmap example with demo
Speaker:
Deepak Rai, Automation Practice Lead, Boundaryless Group and UiPath MVP
Smart TV Buyer Insights Survey 2024 by 91mobiles.pdf91mobiles
91mobiles recently conducted a Smart TV Buyer Insights Survey in which we asked over 3,000 respondents about the TV they own, aspects they look at on a new TV, and their TV buying preferences.
GraphRAG is All You need? LLM & Knowledge GraphGuy Korland
Guy Korland, CEO and Co-founder of FalkorDB, will review two articles on the integration of language models with knowledge graphs.
1. Unifying Large Language Models and Knowledge Graphs: A Roadmap.
https://arxiv.org/abs/2306.08302
2. Microsoft Research's GraphRAG paper and a review paper on various uses of knowledge graphs:
https://www.microsoft.com/en-us/research/blog/graphrag-unlocking-llm-discovery-on-narrative-private-data/
Builder.ai Founder Sachin Dev Duggal's Strategic Approach to Create an Innova...Ramesh Iyer
In today's fast-changing business world, Companies that adapt and embrace new ideas often need help to keep up with the competition. However, fostering a culture of innovation takes much work. It takes vision, leadership and willingness to take risks in the right proportion. Sachin Dev Duggal, co-founder of Builder.ai, has perfected the art of this balance, creating a company culture where creativity and growth are nurtured at each stage.
Slack (or Teams) Automation for Bonterra Impact Management (fka Social Soluti...Jeffrey Haguewood
Sidekick Solutions uses Bonterra Impact Management (fka Social Solutions Apricot) and automation solutions to integrate data for business workflows.
We believe integration and automation are essential to user experience and the promise of efficient work through technology. Automation is the critical ingredient to realizing that full vision. We develop integration products and services for Bonterra Case Management software to support the deployment of automations for a variety of use cases.
This video focuses on the notifications, alerts, and approval requests using Slack for Bonterra Impact Management. The solutions covered in this webinar can also be deployed for Microsoft Teams.
Interested in deploying notification automations for Bonterra Impact Management? Contact us at sales@sidekicksolutionsllc.com to discuss next steps.
Essentials of Automations: Optimizing FME Workflows with ParametersSafe Software
Are you looking to streamline your workflows and boost your projects’ efficiency? Do you find yourself searching for ways to add flexibility and control over your FME workflows? If so, you’re in the right place.
Join us for an insightful dive into the world of FME parameters, a critical element in optimizing workflow efficiency. This webinar marks the beginning of our three-part “Essentials of Automation” series. This first webinar is designed to equip you with the knowledge and skills to utilize parameters effectively: enhancing the flexibility, maintainability, and user control of your FME projects.
Here’s what you’ll gain:
- Essentials of FME Parameters: Understand the pivotal role of parameters, including Reader/Writer, Transformer, User, and FME Flow categories. Discover how they are the key to unlocking automation and optimization within your workflows.
- Practical Applications in FME Form: Delve into key user parameter types including choice, connections, and file URLs. Allow users to control how a workflow runs, making your workflows more reusable. Learn to import values and deliver the best user experience for your workflows while enhancing accuracy.
- Optimization Strategies in FME Flow: Explore the creation and strategic deployment of parameters in FME Flow, including the use of deployment and geometry parameters, to maximize workflow efficiency.
- Pro Tips for Success: Gain insights on parameterizing connections and leveraging new features like Conditional Visibility for clarity and simplicity.
We’ll wrap up with a glimpse into future webinars, followed by a Q&A session to address your specific questions surrounding this topic.
Don’t miss this opportunity to elevate your FME expertise and drive your projects to new heights of efficiency.
The Art of the Pitch: WordPress Relationships and SalesLaura Byrne
Clients don’t know what they don’t know. What web solutions are right for them? How does WordPress come into the picture? How do you make sure you understand scope and timeline? What do you do if sometime changes?
All these questions and more will be explored as we talk about matching clients’ needs with what your agency offers without pulling teeth or pulling your hair out. Practical tips, and strategies for successful relationship building that leads to closing the deal.
Accelerate your Kubernetes clusters with Varnish CachingThijs Feryn
A presentation about the usage and availability of Varnish on Kubernetes. This talk explores the capabilities of Varnish caching and shows how to use the Varnish Helm chart to deploy it to Kubernetes.
This presentation was delivered at K8SUG Singapore. See https://feryn.eu/presentations/accelerate-your-kubernetes-clusters-with-varnish-caching-k8sug-singapore-28-2024 for more details.
Transcript: Selling digital books in 2024: Insights from industry leaders - T...BookNet Canada
The publishing industry has been selling digital audiobooks and ebooks for over a decade and has found its groove. What’s changed? What has stayed the same? Where do we go from here? Join a group of leading sales peers from across the industry for a conversation about the lessons learned since the popularization of digital books, best practices, digital book supply chain management, and more.
Link to video recording: https://bnctechforum.ca/sessions/selling-digital-books-in-2024-insights-from-industry-leaders/
Presented by BookNet Canada on May 28, 2024, with support from the Department of Canadian Heritage.
GDG Cloud Southlake #33: Boule & Rebala: Effective AppSec in SDLC using Deplo...James Anderson
Effective Application Security in Software Delivery lifecycle using Deployment Firewall and DBOM
The modern software delivery process (or the CI/CD process) includes many tools, distributed teams, open-source code, and cloud platforms. Constant focus on speed to release software to market, along with the traditional slow and manual security checks has caused gaps in continuous security as an important piece in the software supply chain. Today organizations feel more susceptible to external and internal cyber threats due to the vast attack surface in their applications supply chain and the lack of end-to-end governance and risk management.
The software team must secure its software delivery process to avoid vulnerability and security breaches. This needs to be achieved with existing tool chains and without extensive rework of the delivery processes. This talk will present strategies and techniques for providing visibility into the true risk of the existing vulnerabilities, preventing the introduction of security issues in the software, resolving vulnerabilities in production environments quickly, and capturing the deployment bill of materials (DBOM).
Speakers:
Bob Boule
Robert Boule is a technology enthusiast with PASSION for technology and making things work along with a knack for helping others understand how things work. He comes with around 20 years of solution engineering experience in application security, software continuous delivery, and SaaS platforms. He is known for his dynamic presentations in CI/CD and application security integrated in software delivery lifecycle.
Gopinath Rebala
Gopinath Rebala is the CTO of OpsMx, where he has overall responsibility for the machine learning and data processing architectures for Secure Software Delivery. Gopi also has a strong connection with our customers, leading design and architecture for strategic implementations. Gopi is a frequent speaker and well-known leader in continuous delivery and integrating security into software delivery.
State of ICS and IoT Cyber Threat Landscape Report 2024 previewPrayukth K V
The IoT and OT threat landscape report has been prepared by the Threat Research Team at Sectrio using data from Sectrio, cyber threat intelligence farming facilities spread across over 85 cities around the world. In addition, Sectrio also runs AI-based advanced threat and payload engagement facilities that serve as sinks to attract and engage sophisticated threat actors, and newer malware including new variants and latent threats that are at an earlier stage of development.
The latest edition of the OT/ICS and IoT security Threat Landscape Report 2024 also covers:
State of global ICS asset and network exposure
Sectoral targets and attacks as well as the cost of ransom
Global APT activity, AI usage, actor and tactic profiles, and implications
Rise in volumes of AI-powered cyberattacks
Major cyber events in 2024
Malware and malicious payload trends
Cyberattack types and targets
Vulnerability exploit attempts on CVEs
Attacks on counties – USA
Expansion of bot farms – how, where, and why
In-depth analysis of the cyber threat landscape across North America, South America, Europe, APAC, and the Middle East
Why are attacks on smart factories rising?
Cyber risk predictions
Axis of attacks – Europe
Systemic attacks in the Middle East
Download the full report from here:
https://sectrio.com/resources/ot-threat-landscape-reports/sectrio-releases-ot-ics-and-iot-security-threat-landscape-report-2024/
JMeter webinar - integration with InfluxDB and GrafanaRTTS
Watch this recorded webinar about real-time monitoring of application performance. See how to integrate Apache JMeter, the open-source leader in performance testing, with InfluxDB, the open-source time-series database, and Grafana, the open-source analytics and visualization application.
In this webinar, we will review the benefits of leveraging InfluxDB and Grafana when executing load tests and demonstrate how these tools are used to visualize performance metrics.
Length: 30 minutes
Session Overview
-------------------------------------------
During this webinar, we will cover the following topics while demonstrating the integrations of JMeter, InfluxDB and Grafana:
- What out-of-the-box solutions are available for real-time monitoring JMeter tests?
- What are the benefits of integrating InfluxDB and Grafana into the load testing stack?
- Which features are provided by Grafana?
- Demonstration of InfluxDB and Grafana using a practice web application
To view the webinar recording, go to:
https://www.rttsweb.com/jmeter-integration-webinar
Let's dive deeper into the world of ODC! Ricardo Alves (OutSystems) will join us to tell all about the new Data Fabric. After that, Sezen de Bruijn (OutSystems) will get into the details on how to best design a sturdy architecture within ODC.
1. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
Name: ___________________________ Period: _____ Date:__________________
Page #___
A. What is Astronomy?
Astronomy is the scientific study of matter in outer space, especially the positions,
dimensions, distribution, motion, composition, energy, and evolution of celestial objects
and phenomena. (phenomena: is a hard to explain or almost magical occurrence)
B. There are many different Celestial Objects in our Universe
Celestial objects appear in the sky during day and night. They include:
-The Sun -The Moon
- Planets -Stars
-Comets -Asteroids
-Meteorites -Black Holes
C. But where did these objects originate?
-This Big Bang, which actually sounded more like a low hum, is estimated to have
occurred between 12-15 billion years ago!!!
-According to the Big Band Theory, all the matter in the universe started out as a
single point! That point was extremely dense. It became unstable and exploded
outward.
-Today the universe continues to expand this is called Hubble’s Law – which states
that nearby galaxies are moving away slowly while more distant galaxies are moving
away more quickly.
2. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
L
Page #___
D. The Universe is still expanding! Here is the proof!
Scientists have two major pieces of evidence that support the Big Bang Theory.
1) The Doppler Effect
2) Cosmic Background Radiation
Figures A & B: Raisin bread analogy of
the expanding universe
E. So what is the Doppler Effect?
When an object is moving relative to an
observer it distorts the way the observer
perceives the object’s electromagnetic
radiation. Whoa! What does that mean? Think
about when an ambulance drives by, going very
fast. The pitch of the siren changes as the
ambulance approaches you and passes you.
This is because the sound waves’ frequency is
increased as it approaches you and decreased
as it drives away. Visualize this concept using
this diagram and the animation on my eboard.
In 1929, Edwin Hubble observed a similar phenomenon
occurred with the light emitted from stars.
He discovered that if an object is moving toward
earth it’s light shifted toward the blue end of the
electromagnetic spectrum since the wavelength is
“squeezed together” producing a shorter wavelength.
This is called blue-shift! (Blue to You)
But if the object is moving away from earth, its light
is shifted toward the red end of the spectrum, since
the wavelength is “stretched out” making it longer.
This is called Red-shift! (Red Away)
All galaxies show red-shift in their spectra,
meaning they are moving away from us.
3. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
Page #___
F. How big is the Universe?
It is very humbling to contemplate the size of our Universe because it is unbelievably
BIG and therefore it can make you feel VERY small. However it’s also impressive that
our civilization has acquired such great knowledge, and it reminds us that we as people
are a part of larger system. It is important for us to respect the natural equilibrium
of our planet and the universe to whom it belongs. We must work to limit our
environmental impact and continue to educate our peers about the delicate balance of
this system.
G. Measuring Distance: In order to grasp and describe the vast size of our Universe,
we must first develop a measurement standard.
• Distances between celestial objects are extremely large.
• Rather than miles, astronomers refer to a ____________________ as a
standard unit of distance.
• One light-year is the distance light travels in one year.
• The speed of light is 186,000 mps (300,000 kps).
• Thus, one light-year is about 6 trillion miles.
• The nearest star to us (Proxima Centauri) is 4.2 light-years away.
Astronomical unit:
• Another unit of distance is the _________________________ (AU).
• One AU is the distance from the Earth to the Sun (93 million miles)
• Distances to other objects are given in multiples of AU.
What is (approximately) the size of the solar system?
Have you ever heard someone say that you’re seeing the past when you look up at the
stars? It sounds romantic and perhaps even silly, but it is correct. For example, when
an astronomer views the Andromeda galaxy, he/she is seeing how it was 2.5 million
years ago. This is because it has taken that long for the light to reach us here,
offering a window into the past that no history book ever could!
H. Did you know…
A light year is the distance light travels in a single year – 9,460,528,000,000
kilometers. So the light we see coming from Proxima Centauri left the star 4.2 years
ago. Even being the nearest star, Proxima Centauri is incredibly far away. It would
take our fastest spacecraft more than 50,000 years to make the journey.
4. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
Page #___
I. Components of our Universe.
The best definition of the Universe is: EVERYTHING!
We are all apart of the universe along with everything else you can think of.
Outside of the edge of the universe is nothing. This is confusing because its hard to
imagine “nothing”. The universe is expanding into nothing because nothing is in it’s way.
All matter makes up the universe.
I like to think of the components like a system of “Russian Dolls.” These components
are organized from largest to smallest and they fit inside of each other:
The universe is made of billions of Galaxies
Galaxies are made of billons of Stars
Stars are the Center Solar Systems
Solar Systems are made of planets, moons, comets, asteroids and meteorites.
Planets moons comet, asteroids and meteorites are made of matter.
J. Galaxies
A ______________ is a collection of
millions or billions of stars. Galaxies
can be spiral, elliptical, spherical or
irregular in shape. The Sun is part of
the _________ galaxy, which is a
spiral galaxy. The Sun is located on
one of the spiral arms, far from the
galactic center. When you look up on a
clear night there is a hazy lighter
band that runs across the sky. When
you look at this band you are looking at
the side of the spiral arm that is
adjacent to the arm that our sun is in.
Each arm is made of millions of stars.
The stars themselves are too far away
to see individually, but together their
light combines to make the sky lighter
in that area.
5. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
K. Billions of Stars make up a galaxy, but what is a Star… are they all the same?
Page #___
Must Know Facts about Star Characteristics
A) A star is a huge, shining massive ball of gas in space that produces a large amount of
light and energy.
B) About 75% of stars are apart of groups that orbit each other.
C) They are grouped in large structures called galaxies. (Milky Way).
D) Stars have life-cycles like humans.
E) A stars color depends on surface temperature.
F) Stars vary in their size, mass, density, temperature and composition.
G) ____________________ is the actual brightness of a star.
H) Luminosity depends only a star’s _____________ and __________
I) Most stars have planets that orbit them because of their immense gravity
Composition
Stars are primarily made of
__________________ and Helium.
Many other elements are present in stars
in small amounts. A star’s composition can
be determined by
___________________________.
Spectral Analysis
_____________________ is the
study of the electromagnetic spectrum
emitted by a star, using a
_______________________.
Each element in the star emits radiation
is a specific set of ______________
Color and Temperature
A Star’s color that we see with the
naked eye depends upon its surface
temperature.
As materials become hotter, their
color changes from:
Red to Orange to Yellow to White to Blue
What color are the stars in the
Constellation Orion? (ESRT p 15)
Betelgeuse is ________
Rigel is ____________
How Do Stars Radiate Energy?
A stars energy is the result of nuclear
fusion, in which Hydrogen atoms combine
to form Helium atoms, releasing energy.
This Electromagnetic energy is radiated by
stars.
6. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
The Main Classifications of Stars:
______________
______________
______________
______________
______________
Our Sun is classified as a
__________________
__________________
The H-R Diagram
The Hertzsprung-Russell
(H-R) Diagram on the right
is a graph of stars, comparing
luminosity and temperature.
Stars are categorized according
to these two properties!
Page #___
The H-R Diagram
• The Main Sequence is the band
into which most stars fall. They
lie somewhere in between a:
High temperature, high luminosity
&
Low temperature, low luminosity
• Red Giants and Supergiants –
cooler, very luminous stars that
are very large
• White Dwarfs are hotter, low
luminosity stars that are small
Star Life Cycles
• Stars are born in a cloud of gas and dust,
called a _________________.
• Most stars remain as
______________________ stars, until
their hydrogen fuel is depleted
• An average star, like the sun, would go
through the Red Giant phase, eventually
becoming a _____________________.
• A large star would become a
___________________, then explode
as a supernova. The result may be a
neutron star, pulsar or black hole.
7. Unit 2: Astronomy Earth Science- Ms. Gill Note Packet #3A
The Main Classifications of Stars:
______________
______________
______________
______________
______________
Our Sun is classified as a
__________________
__________________
The H-R Diagram
The Hertzsprung-Russell
(H-R) Diagram on the right
is a graph of stars, comparing
luminosity and temperature.
Stars are categorized according
to these two properties!
Page #___
The H-R Diagram
• The Main Sequence is the band
into which most stars fall. They
lie somewhere in between a:
High temperature, high luminosity
&
Low temperature, low luminosity
• Red Giants and Supergiants –
cooler, very luminous stars that
are very large
• White Dwarfs are hotter, low
luminosity stars that are small
Star Life Cycles
• Stars are born in a cloud of gas and dust,
called a _________________.
• Most stars remain as
______________________ stars, until
their hydrogen fuel is depleted
• An average star, like the sun, would go
through the Red Giant phase, eventually
becoming a _____________________.
• A large star would become a
___________________, then explode
as a supernova. The result may be a
neutron star, pulsar or black hole.