Hi fellow bloggers, it's me Reilly. Hope all of you are alright and well. I'm sharing with you today an unfinished project of my science report that I created for our science tests. It's about my test that I did on paper planes and how far it would go if I changed the wingspan every test. I would change it by 2 cm every time.
Kia ora, I am a student at Mairehau High School, Welcome - Haere Mai. This is a place where I will be able to share my learning with you. Please note my work may include spelling or other errors because some of it will be my first drafts. I would like to get your feedback - comments, thoughts, questions and ideas to help me Learn Create Share.
Friday, August 28, 2020
Thursday, August 6, 2020
My Acids & Bases Report
Hi fellow bloggers, it's me Reilly. Hope all of you are alright and well. I'm sharing with you today an unfinished project of my Acids & Bases Report that I created. It's from this science project that i'm doing with acids and bases. Hope you guys like it because it took quite a bit of research to do.
Stay safe and well.
Reilly.
Stay safe and well.
Reilly.
Monday, August 3, 2020
The Aurora Polaris
Hi bloggers, I'm sharing with you this activity that I'm doing. It's on the polar lights, southern and northern lights. Polar lights (aurora polaris) are a natural phenomenon found in both the northern and southern hemispheres that can be truly awe inspiring. Northern lights are also called by their scientific name, aurora borealis, and southern lights are called aurora australis.
The origin of the aurora begins on the surface of the sun when solar activity ejects a cloud of gas. Scientists call this a coronal mass ejection (CME). If one of these reaches earth, taking about 2 to 3 days, it collides with the Earth’s magnetic field. This field is invisible, and if you could see its shape, it would make Earth look like a comet with a long magnetic ‘tail’ stretching a million miles behind Earth in the opposite direction of the sun.
The origin of the aurora begins on the surface of the sun when solar activity ejects a cloud of gas. Scientists call this a coronal mass ejection (CME). If one of these reaches earth, taking about 2 to 3 days, it collides with the Earth’s magnetic field. This field is invisible, and if you could see its shape, it would make Earth look like a comet with a long magnetic ‘tail’ stretching a million miles behind Earth in the opposite direction of the sun.
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